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Annual Report 2000 - 2001

Autonomous Institutions

Agharkar Research Institute, Pune

Research at the Agharkar Research Institute focuses on the area of Life Sciences and is carried out under three areas, viz. Animal Sciences, Microbial Sciences and Plant Sciences. Presented below is the area wise report:

Animal sciences Biometry & Nutrition

Analysis of the longitudinal database on adolescent growth of rural children revealed that (i) sitting height of an individual is likely to be influenced by intra-uterine genetic factors while leg height is governed by postnatal environmental influence. (ii) delayed adolescent growth coupled with early age at marriage increased the risk of pregnancy wastage in rural girls. Shorter the period between onset of menarche and first conception larger was the risk.

Studies on Maternal Nutrition and Birth Outcome revealed that: (i) Maternal intake of ALNA rich foods was associated with birth size in rural undernourished mothers suggesting that when diets are inadequate in macronutrients, foods rich in micronutrients such as GLV, can play an important role in improving fetal growth. (ii) Strenuous activities of rural women were observed to have adverse effect on birth weight. This suggests that reducing maternal activity specifically at late gestation could be a modifiable factor for improving fetal growth. In urban affluent mothers among macronutrients maternal fat intakes in early gestation influenced birth size while among the micronutrients, the foods rich in antioxidants showed relation with birth size among urban mothers.

Experiments were carried out on Wistar rats to examine the effect of nutritional rehabilitation and dehabilitation on growth of rats and on their biochemical profile in adult life. It was observed that maternal nutrition during lactation is more critical than during gestation for growth of pups. There is sex dependent and permanent change in organ weight of rats due to protein restriction during critical periods of development particularly on kidney and pancreas.

Energy costs other than resting were measured for 4 additional activities - walking, walking with load (5kg), bending & sweeping and cycling on ergometer. Prediction equation for RMR was revised and compared with other reported studies. The equation based on body weight as an independent factor was comparable with that reported for populations in other countries while the equation based on fat free mass (FFM) for Indian was significantly different than the reported ones. This indicates the importance of body composition in prediction of RMR.

Comparison of daily Vs weekly supplementation of iron folic acid showed similar improvement in Hb in non-pregnant as well as pregnant women. Efficacy of weekly supplementation was similar to that in daily, with respect to weight gain during pregnancy, when the supplementation was initiated from pre-conception stage. This finding indicates importance of pre-conception stage as also of weekly supplementation adequacy.

While studying the growth during early infancy and risks for adult diseases it was observed that individuals who were undernourished in early life but have higher body weight as adults had higher systolic B.P. than those who were undernourished in early life and remained thin as adults. The analysis indicated that the imbalance of growth in early life is risk factor for hypertension in adult life.

Statistical models are being developed to investigate linkages of micronutrient status and health. Several socioeconomic, environmental, dietary and biochemical factors were examined for their influence on erythrocyte membrane zinc status in adults using multiple logistic regression analyses. A significant correlation was observed between intakes of fruit, GLV and milk products with zinc status. Cereal and pulse intakes, environmental conditions, and family size were observed to be good predictors of Zn deficiency. Logistic regression analyses of micronutrient deficiencies in early anemic humans indicated stronger interactions of copper and zinc with iron than any of the vitamins.


In the project on Pheromones and Semiochemicals repellent formulations for honeybees based on thioethers were identified and patented. These are useful for preventing honeybee visits in areas sprayed with pesticides. The major constituent of Nosnov gland pheromone of Apis mellifera maintained in India was found to be nerol and a minor constituent, neral was found from bees from cooler areas.

Geology & Palaeontology

The foraminiferal studies of the clays of Gulf of Kachchh showed the dominance of forms belonging to Milioliina and Rotaliina. The diversity is low and foraminiferal tests are thin and fragile. This may be due to lack of adequate precipitation of CaCO3 to be used for thickening of the shell. Such conditions may arise where there is absence of normal salinity due to fresh water influx. The magnetic studies revealed the presence of magnetite in the profile and s-ratio indicated relative increase of magnetic mineral flux approximately 1.5 meter below the surface.

Palynological evidences favour dense vegetation, heavy precipitation and high moisture conditions in and around Dhamapur during Holocene. The absence of such conditions at present may be attributed to ecological shifts, tectonic adjustment at local level and anthropogenic influence.

While making a factual assessment of the view that the Marwar Supergroup is Neoproterozoic-Eocambrian in age, it was realized that the evidences cited in support of a Cambrian age for a part of the Marwar Supergroup are not unequivocal. Field investigations and palaeontological studies undertaken for the purpose revealed the presence of Planolites in the Bap Formation. It was also found that trace fossil reported as 'Chordophyceous remains' by earlier workers from the Jodhpur Sandstone is in fact a product of weathering.

Palaeontological studies pertaining to the Kurnool Group and the Cuddappah Supergroup revealed that the so-called trace fossils from the Gulcheru Quartzite, in reality are pseudofossils. The ichnogenus Planolites from sediments in vicinity of Nagarjuna Sagar was identified as P. beverleyensis. Remains of Procaryotic algae as carbonaceous filaments were found to occur in the Koilkuntla Limestone. One of the forms is tentatively identified as Grypania spiralis.


In studies on genotoxicity assessment, the mouse bone marrow micronucleus assay to detect potential clastogens and aneugens in mice was studied using fluorescent in situ hybridization (FISH) of centromeric satellite DNA probe. Initial observations indicated that VBS and MMC can serve as positive controls in assessment of potential aneugens and clastogens of plant origin.

In developmental biology, the role of FGF in early development of the nervous system was studied by blocking endogenous FGF function. Preliminary results show that about 50% embryos treated with anti-FGF antibody developed abnormally. Neural tissue was severely affected in all such embryos. The abnormalities included inhibition of closure of neural tube along the entire axis and hole in the forebrain. Amongst these embryos, 37% also showed misplaced somites. These studies confirm the role of FGF in early chick development.

Microbial Sciences

The research activities in the areas of Microbial Sciences are spread over three major thrust areas viz. metal-microbe interactions and their applications, microbial treatment of industrial wastes and fermentation of industrially important compounds. The highlights are:

Nanometer-scale semiconductor quantum crystallites are important in modern electronics and computer technology. We have successfully synthesized cadmium sulfide and other metal-sulfide nanocrystallites by adopting a microbiological route. UV absorbance, Fluorescence, X-ray diffraction and Transmission Electron Microscopy studies showed that the nanocrystallites thus synthesized were size reproducible and had sharp particle size distribution. The purified CdS nanocrystallites were used to fabricate a heterojunction with poly (p-phenylenevinylene (PPV). The result is superior to the diodes fabricated similarly using chemically synthesized cadmium sulfide nanocrystallites.

Monocrotophos and Dimethoate are among the widely used but hazardous organophosphorus pesticides. Hence their biodegradation was studied. Monocrotophos was found to be completely degraded to carbon dioxide by Bacillus, Arthrobacter and Pseudomonas species with methylamine and acetic acid as the intermediate metabolites. Biodegradation of Dimethoate was found to be plasmid associated in Pseudomonas aeruginosa.

The lipase of anaerobic bacterium Selenomonas lipolytica was found to contain two forms namely Lipase I & Lipase II. Lipase I had a mole wt. of 240 kda and exhibited maximum enzymic activity at pH 6.0 and temperature 45oC. N terminal sequence of first ten amino acids was found to be different from that of known Lipases. Lipase II on the other hand was found to be a low mole wt. protein (29 kda).

The acid tolerant strain belonging to genus Methanobrevibacter was studied further for its 16S rRNA sequence. On the basis of this sequence and acid-tolerance characteristics the strain was identified as a novel species and named as Methanobrevibacter acididurans (Type strain ATM).

A fibrin specific fibrinolytic enzyme (EC.NO. was purified from the spent broth of a thermophilic Streptomyces sp. The process for production of this enzyme was patented as Actinokinase. This prokaryotic enzyme resembles urokinase, an eukaryotic protein.

Methanogens produced tryptophan when indole and serine were supplemented in the medium of an immobilized cell system. The isolated tryptophan was about 99% pure. By the similar process phenylalanine was also obtained by supplementing phenylpyruvate and glutamate.
In studies on 'metabolic flux in methane producing bacteria, the rate of glycogen synthesis, methanogenesis and ATP formation were found to be related to each other. Methanogenesis was completely inhibited by 2-bromoethane sulfonate (BES) affecting ATP formation also.

Disposal of waste plastics has become a very serious problem. Hence attempts were made to initiate microbial degradation of polyethylene based plastics. Microbial consortium comprising of Bacillus and Pseudomonas sp. has been obtained by enrichment technique from soil. The culture is found to grow on polyethylene (PE) film and polybag (carrybag) pieces. In case of polybags there was visible damage in the surface of the film.

Plant Sciences


Germplasm collection of wild plant resources and medico-botanical studies are the major thrust areas of Botany group.

Under the collection and conservation project on germplasm of Carissa, Azadirachtra, Aloe, Asparagus and Bruhat Panchmula group of species, multiplication through various means has been attempted.

Leaves of Neem tree (Azadirachta indica A.Juss) have been investigated for comparative antiinflammatory action between normal bitter type and its variant non-bitter types.The medicinally promising genus Asparagus is being studied for chemical analysis and agronomic trials.

Thirteen species of endemic/rare trees were located at 14 different spots in South Konkan regions and their germplasm was procured for nursery evaluation.Work on seed bank collection and standardization of cultivation techniques for commercially important medicinal plants like Boerhavia, Eclipta, Rubia, etc. is initiated in collaboration with Ayurveda Research Institute.

Under Medico-botany thrust area the methanol extract of defatted Jatropha curcus roots were evaluated for local, systemic acute and sub-acute models in animals with positive results. The same extract was fractionated to locate active antidiarrhoeal fraction in albino mice.

Crude extract of Sterculia foetida leaves was purified by column chromatography. A white crystalline triterpenoid and another crystalline compound was obtained by column chromatography. Study of chemical reactions and spectral analysis of the derivatives is in progress. Spectroscopic studies of Curcuma amada rhizome extract showed presence of chemical compounds with hydroxyl, ester. carbonyl and olefin functionalities. The extract showed significant dose-dependent anti-inflammatory activity in acute and chronic administration in Albino rats.

A new project on comparative pharmacognostical studies in some important bark drugs is initiated. In this project six bark drugs are selected for pharmacognostic evaluation due to seasonal variations. Of this, Madhuca , Mimusops and Nyctanthus are studied with macroscopical characters and physical constants.

The finding of a mangrove fern of family Polypodiaceae from the Nawargaon intertrappean beds of Wardha district, Maharashtra, is significant as it forms the oldest record of its kind which has geological and palaeobiogeographical implications. The present permineralized remains of a mangrove fern from the Late Cretaceous Intertrappean beds of India also opened up new vistas as there was a possibility of an ancient sea way, Tethyian influence across Central India prior to the initiation of volcanic eruptions.

Genetics and Plant Breeding

The research in this area is concentrated on genetic improvement of soybean, wheat and grapes.

Soybean varieties MACS-693 and MACS-694 developed at ARI Centre ranked first and second in Southern Zone. MACS-693 ranked second in North Eastern Zone also. Six varieties from this centre are included in All India co-ordinated trials across the zones. The centre has supplied 729.20 quintals breeder seed and 11.50 quintals nucleus seed to different seed multiplying agencies in Maharashtra and Madhya Pradesh. In Frontline Demonstrtions, MACS-450 recorded the highest yield of 3582 kg/ha which was the highest in the country.

A Durum wheat variety MACS-3125 developed at this centre ranked first in Peninsular Zone and has surpassed the yields of bread wheat. Likewise, MACS-3208 has performed well in Central Zone. About 225.6 quintals breeder seed was supplied to multiplying agencies. In Frontline demonstrations, MACS-2694 gave highest yield of 61.5 qtls/ha and the average yield of improved technology was 16.4% higher than the control variety HD-2189.

Eleven genotypes/species of wild relatives of grapes were collected. Out of these, 3 species were found to be tolerant to drought. 282 F1 hybrid seedlings were raised. 31 hybrids were evaluated for their fruit quality and four were found to be promising. Likewise, 102 hybrid seedlings were evaluated for powdery mildew resistance and 68 found to be resistant.

Agricultural Biotechnology: Genetic relationships in cultivated grapes, Vitis vinifera and other Vitis species were analyzed by Random Amplified Polymorphic DNA analyses. A total of 44 genotypes analyzed formed 3 distinct clusters. Wild species and rootstocks were distinctly different from cultivated grapes and formed a separate group. Within cultivated grapes vinifera and labrusca types formed two distinct groups.

Mycology & Plant Pathology

The lichen unit at ARI has been recognised as a collaborating centre of AICOPTAX for the research on lichens of Western Ghats of India under Ministry of Environment & Forestry, Govt. of India.

Lichen species Bulbothrix setschwanensis has been successfully cultured in vitro, producing lichen metabolites atranorin and salazinic acids. The effect of various culture conditions on the growth of Bulbothrix setschwanensis in vitro with special reference to the production of salazinic acid and on bioactivities like inhibition of tyrosinase and superoxide dismutase (SOD) like activites have been studied.

Over 300 lichen specimens have been collected from the western ghats in Maharashtra.

In the Identification Service For Plant Pathogens/Other Fungi, several interesting fungi, new taxa, new diseases, some entomogenous fungi and fungi isolated from specialized habitats were identified. The newly started fungal culture collection houses about 50 cultures of a variety of fungi belonging mainly to ascos and deuteros. 190 specimens were added to Ajrekar Mycological Herbarium which included 25 type specimens.

Three edible mushroom species namely, P. cystidiosus, P. ëous and P. eryngii were grown on media containing the trace elements Zn, Mn and Cu, Se in different concentrations, ranging from 10 to 100 ppm and 0.1 to 0.5 ppm respectively. The growth was enhanced in comparison to the control by addition of some of these elements. The laccase reaction of the filterate of these cultures indicated that the production of laccase by the three strains was higher, in presence of Cu ++. P.eryngii and P. cystidiosus produced higher amounts of laccase than Pleurotus ëous.

Birbal Sahni Institute of Palaeobotany, Lucknow

The Institute has been carrying out researches on various aspects of Palaeobotany and allied subjects under following Thrust Areas:

  • Antiquity of Life
  • Gondwana Supercontinent: Regional geology, floristics, terrane accretion, plate tectonics and configuration
  • Biopetrology of Indian coals in relation to coal bed methane
  • Floristics of petroliferous basins, and
  • Quaternary vegetation, climate and monsoon.

Significant contributions and discoveries

  • First record of metazoan fossils like vertical burrows/ichnofossils and medusoid remains from Neoproterozoic Panium Quartzite of Kurnool Basin indicates the appearance of animal life in Indian shield area.
  • Discovery of Early Permian plant remains and Late Asselian palynomorphs from Karakoram Terrane provides crucial clue regarding the palaeogeographic reconstruction of the Karakoram-Himalayan block in the Permian. The Karakoram Terrane was close to the Salt Range. The micro-continents accreted with Indian Plate during Cimmerian orogenic cycle. Permian plant fossils from Arunachal Pradesh indicate presence of Glossopteris floral elements comparable with the flora of Barakar Formation of peninsular India. Among the Gondwana group of plants, dichotomous development pattern in Glossopterid has been analysed on the basis of morphological features of leaves and fructifications.
  • Palynological study of intra-cratonic Gondwana sequences indicate palynofloral transition from Late Triassic to Early Jurassic sequences particularly in Rajmahal Basin. Neocomian palynofossil investigations demonstrate continuity of Upper Jurassic-Early Cretaceous sequences in Indian Craton. Petrological investigations of Permian Barakar coals from Kanhan area of Satpura Gondwana Basin indicate coals within the threshold of methane generation.
  • Plant bearing Tertiary sediments of Warkala Formation, Kerala coast and Mahuadanr, Bihar have been found to contain insect remains in resin lumps. The productive resins are suitable for the study of fossil DNA. A collaborative study has been initiated with Centre for Cellular and Molecular Biology, Hyderabad.
  • On the basis of fossil angiospermic remains from Tertiary sediments of Arunachal Pradesh existence of tropical evergreen to littoral and swampy forests conditions were deduced. The flora also shows the migration of some plants from Malaysia. Prevalence of evergreen semi-evergreen forest under warm humid climate is interpreted around Bilaspur in the Himalayan foot-hills on the basis of leaf impressions recovered from Siwalik sediments. Moist conditions with plenty of rainfall have been interpreted on the basis of fossil woods of Intertrappean sediments of Kachchh. Further discovery of mango fossil leaf in Meghalaya confirms the earliest record of mango in North East Himalayan region of India during Palaeocene (55 Ma).
  • Selective association and distribution of microfossils from Eocene rocks of Morni Hills (H.P.) indicate fluctuating environment of deposition due to sea level changes. Palynology of Siwalik sediments of Nadah area (Haryana) suggests presence of wet grassland with open and mixed flora during Pinjor sedimentation. Botryococcus, an oil forming green algae have been recovered from Eocene rocks of Jammu and Kashmir. The study is helpful in understanding the source rock evaluation which might help in the discovery of oil fields in the foot-hills of Himalayas.
  • Pollen analysis of sedimentary profile from Punlota Lake, Nagaur District (Rajasthan) has revealed successive climatic phases 9200-8050 yrs B.P. arid, 8050-3810 yrs. B.P. warm moist, around 3810-1325 yrs B.P. decrease in warm and moist conditions, and lastly comparatively drier or more or less similar conditions as in preceding phase. Silty clay sediments from the lake bed, Priyadarshini, Eastern Antarctica have been processed. A low hydrolysing periglacial depositional environment is deduced. Pollen analysis identifies three pollen zones based on the fluctuations in the retrieved palynomorph which apparently manifest palaeoclimatic oscillations during Holocene.
  • The evidence of carbonised botanical remains from archaeological site at Mesolithic Damdama in Pratapgarh District (U.P.) indicates the shift from the hunter-gatherer economy of Stone age people to the sedentary life style of early Neolithic agriculturalists in the Ganga Valley. The tree ring chronology prepared from samples of Abies pindrow growing around Dokriani Bamak Glacier extending back to 1614 A.D. exhibits periods of low and high growth which might be linked with glacial fluctuation of this region. The chronology of palynologically analysed peat samples from Phulera, Kumaon (U.P.) works out to 15900±150 yrs B.P. (C-14 age). The sample from Priyadarshini Lake, Antarctica is dated as 7190±300 yrs B.P.
  • During the year 61 research papers and 54 abstracts were published and 57 papers were accepted for publication. Thirty-five research papers were presented in International and National Conferences. In International Conferences 2 scientists were deputed while 28 scientists attended the Conferences organised in the country.

Forensic Palynology

  • In order to carry out researches on forensic palynology a core group of scientists of Quaternary palynologist is formed to undertake the study in collaboration with the organisations dealing with forensic sciences in New Zealand and USA. This is the emerging new application of palaeobotanical researches in forensic science and useful for Police Department.

Integrated Long Term Programme

- A project entitled "Floral and climatic evolution based on Geologic and Biotic events during Precambrian and Phanerozoic Time" has been initiated under ILTP of co-operation in Science and Technology between BSIP (India) and Russian Academy of Sciences (Russia). BSIP has been chosen as the nodal agency under the umbrella of Earth and Planetary Sciences on palaeoclimatic researches.


The Palaeobotanist volumes 49 (1 & 2) have been published, the latter consisting of research papers on North-East, India. Newsletter 2000 and bilingual Annual Report 1999-2000 were published, highlighting Institute's research and other activities. A Monograph entitled "An introduction to Gymnosperms, Cycas and Cycadales" of Prof. D. D. Pant, Allahabad is being processed for publication.

Consultancy services

The Institute has rendered consultancy services to the personnel from various organisations in radiocarbon dating, electron microscopy, palynology and identification of fossil remains.

Web Site and Internet access:

The Institute web site ( has been launched on November 14, 1999. The Institute has registered a domain "" on the Internet. Internet access to scientists has been provided at 60 nodes throughout the institute.

Bose Institute, Calcutta

Through the 83 years of glorious existence since its foundation by Acharya Jagadis Chandra Bose in 1917, Bose Institute has emerged as a potential, scientifically active multidisciplinary research Institute in India. Research and training in various fields of physical and biological sciences are undertaken in ten Departments and Sections viz., Physics, Chemistry, Botany, Microbiology, Biochemistry, Biophysics, Animal Physiology, Plant Molecular and Cellular Genetics, Immunotechnology and Environmental Sciences. Through years of its existence the prestigious Institute has proved itself to be pioneer in the frontiers of modern Physical and Life Sciences. Its work and achievements have attracted attention of Scientists from our country and abroad. Many of our faculties are Bhatnagar awardees, Fellows of National Academies and recipients of National and International awards, and have intra-, inter- institutional and International research collaborations.

Bose Institute is conducting research in the following main areas (Institute Projects) :

  • Improvement of Plant Productivity, Nitrogen Fixation and Photosynthesis using modern Biotechnology and Plant Breeding.
  • Chemical and biological studies of Plant and Marine organisms.
  • Studies on structure, function and dynamics of biomolecules.
  • Studies on ecology, environmental pollution and related problems.
  • Studies on microbes and parasites for industrial and medical applications.
  • Problems in condensed matter, intermediate energy physics and related interdisciplinary areas.

Major Achievements:

Considerable progress has been achieved in the areas of neutron dosimetry, quantum disentanglement, teleportation, propagation of strangelets through the terrestrial atmosphere, cosmological dark matter and quantum antiferromagnets, among other areas. Enrichment of medically important EPA and DHA has been made from Sting Ray Oil. Hepatoprotective role of the herb Desmotrichum filmbriatum has been demonstrated for the first time. A novel reagent has been developed for the N-formylation of (hetero) arylamines. A beneficial role of MIM in Cat II TB patients has be indicated. ABRE-based promoter has been constructed and to overexpress Samdecarboxylase, the cDNA has been ligated into Ti-based plasmid. To inhibit ethylene biosynthesis in fruit, transgenic tomato plants have been generated. A number of in vitro grown plantlets of Teak, Kalmegh and Ambroma augusta were transferred to The Department of Science & Technology, Govt. of West Bengal. SoxA, SoxB and SoxC genes in sulfur oxidizing operon in Thiobacillus have been identified by PCR based genome walking technique. The effect of the side chain on the backbone conformation, structural features of the cis peptide bonds and the microenvironment around different protein residues have been elucidated. The structure of the Calotropin DII and Acetanilide - Cox interaction complex are fully characterised. A few medically important potential substrate - receptor, drug-receptor, protein-protein interaction at structural level has been characterized by computer modelling and deposited in Protein Data Bank. Carbofuran, a pesticide, showed mobilization of cholesterol molecules from fish hepatic cytosol to plasma membrane with inhibition of membrane Ca2+ - ATPase activity. The cytosolic inositol synthase(s) from Oryza and Porteresia have been completely sequenced. A full length cDNA for cytosolic FruP2ase from Porteresia has been sequenced and submitted to Gene Bank (Accession number Af 218845). Bioaccumulation of aflatoxin from liver of farm animals in the consuming individual is possible and continuous accumulation of the toxin may be determined. Protein A (PA), the cell wall protein of Sta[ju;pcpccis aireis, has been found to initiate pro-proliferative signals to the immunocytes and pro-apoptotic signals to the tumor cells of the same host. Two peptides, 16 and 20 mer as derived from PA by protease digestions, have been found to mimic many of these functions of the mother protein.

Patents filed/Technology Transfer :

  • Superheated Drop Detector Technology developed in the Department of Physics, B.I. has been transferred to Defence Research Laboratory, Jodhpur and also to Indira Gandhi Centre for Atomic Research.
  • Technology developed in the Department of Chemistry for the production of EPA (patented), a potent medicine for atheroschlerosis and thrombosis (cardiovascular diseases) has now been transferred to P.G. Hospital, Calcutta.
  • A simple process for the preparation of iodoquinol, an antiamoebic compound has been developed in the Department of Chemistry and patented and is awaiting for transfer to industry.
  • Technology of using a bioimmunomodulator for reducing morbidity and mortality of poultry chicken developed in the Department of Chemistry and patented, is awaiting for transfer.
  • Technology developed for clonal propagation of economically important plants, mass culture of spirulina developed in the Department of Botany is awaiting for transfer.
  • Management of Tapping Pannel Dryness Syndrome in Rubber Derived in the Department of Botany has been transferred to Ruber Research Institute and Rubber Board of India.
  • Biotechnical and Ecophysiological components of seed Vigour for Direct Seeding Cultivation in rice developed in the Department of Botany has been transferred to Directorate of Rice Research, ICAR.
  • Technologies viz. Protein Purification, Measurement of Photochemical Reaction, Cell Culture and Regeneration of Plants, Recombinant DNA work to study Gene Cloning etc. developed in the Department of Botany awaiting transfer.
  • PCR-based techniques for rapid identification of Vibrio cholerae and mycobacteria developed in the Department of Microbiology awaiting transfer.
  • Technologies viz. Expression of heterologous proteins, Improvement of Plant Productivity, Studies of microbes and parasites for industrial and medical applications, Molecular characterisation of Thalassaemia in local population developed in the Department of Biochemistry awaiting transfer.
  • Technologies on better production of fish (triploid catfish, H. Fossils and rapid ovarian development in freshwater prawn, M. rosenbergii developed in the Animal Physiology Section awaiting field transfer.
  • Technology for better production of silk developed in the Animal Physiology Section awaiting transfer.
  • Technologies developed in the PMCG Section viz. Genetically modified homogeneous diosgenin yielding Costas speciosus, Batch-culture pyrethrin production for commercial purpose, Alien gene transfer techniques in chickpea, mungbean and mustard, Micropropagation protocols for industrially important poplar genotypes awaiting transfer.
  • ELISA kit for detection of Aflatoxin, Techniques for identification and separation of IgG antibody molecule developed in the Immunotechnology Section awaiting transfer.
  • An water filter to decontaminate arsenic has been developed in the Environmental Science Section.
  • Technology developed in the Department of Botany for isolation of acrylamide from plant sources awaiting transfer.
  • Technology developed in the Department of Botany on Generation and demonstration of tissue culture-based raised planting materials - teak and medicinal plants Endrographio pAnicclata transferred to Department of Science & Technology, Govt. of West .Bengal.
  • Technology developed in the Department. of Botany for Downstream processing in tissue culture awaiting transfer.
  • Technology developed in PMCG Section patented in USA on Plastid transformation of arabidopsis thaliana transferred to Rutgars Univ., USA where the collaborative research undertaken.
  • Technology for Removal of Sulphur from coal by Microbial process transferred to Burn Standard Co., the funding agency.

Indian Association for the Cultivation of Science, Calcutta

The Indian Association for the Cultivation of Science (IACS), established in 1876, has been continuing its efforts for excellence in scientific research. The various scientific activities and achievements during the year are summarized below :

Materials Science

Research work was carried out in the following disciplines during this period : transport properties of magnetic/metallic multilayers and intermetallic compounds, Colossal magnetoresistance and low temperature properties of polyaniline blends. Electronic structure calculation for strongly correlated systems, Synthesis of binary and ternary semiconductors for fabrication of thin film solar cells. Nanostructured materials in thin film form, hard coating materials : Diamond and nitride (c-BN and AIN) films, Transparent and doped conducting oxide film using sol-gel technique, Rapid thermal processing (RTP) for the fabrication of large area solar cells; Metal-conducting Polymer Schottky Contact, X-ray crystal structure determination of some nucleosides, natural products and organic crystals, Studies on morphology, growth and characterization of non-linear optical materials, Characterization of lattice defects from x-ray powder profile analysis of metals, alloys, thin films, composites and industrial materials; Evidence of single electron capture into excited states in N2++-N2 collisions in ion beam scattering experiment. Angular distribution of photofragments in intense field multiphoton dissociation. New technique of population inversion by chirped lasers.

Solid State Physics

Recently single crystal epr studies on bi-metallic copper-bis-ethylene diamine manganese tetrachloride have been made elucidating new information about the nature of exchange coupling in this low D-magnetic compound. High field Zeeman study on the CdCsCl-type single crystals also showed interesting results. To find the conditions of geometric frustration at low temperature in ferro and antiferromagnetic RE-pyrochlorates, importance of single ion magnetic anisotropy and its relative strength w.r.t dipolar and exchange interactions have been shown. Structural change in the glass-network structure in Bi2O3-P2O5 glass has been detected by acoustic method. A density modification technique has been developed to improve the E-map obtained from the direct method for a known protein complex. A new scaling formalism for the conductivity spectra of ionic glasses indicating a relation of relaxation dynamics with glass structure has been developed. Light -emitting devices (LEDs) have been fabricated fabricated based on Langmuir-Blodgett films of a porphyrin derivative and decacyclene. LEDs have also been fabricated based on layer-by-layer self assembled films. A high pulsed magnetic field arrangement has been developed to study colossal magnetoresistive materials. Relaxor type ferroelectric transition have been observed, for the first time, in multicomponent glassy materials ambedded with nanocrysalline ferroelectric BaTiO3 particles/clusters. It has been established that in the Bi based Bi-Sr-Ca-Cu-Mn-O etc. glasses becomes superconductor with nanocrystalline (<20nm) grains/or clusters. It is not possible to prepare single phase high Tc superconductors with grain size >20nm. Many multicomponent transition metal oxide glasses are also found to contain nanocrystalline clusters of different sizes and there is a critical size of the nano-clusters above which thermal, electrical and other properties show nonlinear variations indicating a glass to glass type phase transition. This work is being done in collaboration with Prof. H Sakata of Tokai University, Japan. Effect of magnetic polarons on the electrical transport mechanism in colossal magnetoresistive materials like Ca-Pb-Mn-Cr-O oxides has been observed from the temperature and magnetic field dependent Seebeck coefficient data. Dielectric relaxation behaviour in some ferroelectric liquid crystals (for example, SC-1013) have been studied using the new facility developed in the department mostly funded by AvH Foundation Germany. This work is being done in collaboration with Prof. W Haase, Technical University, Darmstadt, Germany, and Prof. E Okabe (Schisso petrochemicals Corporation, Japan).


Preliminary calculation of angular correlation in doubly excited states have been made for ground and low lying excited states of two electron systems. Allowed and forbidden transition properties of closed and open shell atoms and highly stripped isoelectronic ions have been studied using time dependent perturbation theory. Excited states and spectroscopic parameters by HDHF Method Spectroscopy of foreign atoms under liquid He environment, spectroscopy of highly stripped exotic ions and those of photo-biological systems by quantum mechanical approach have been initiated. Ab-initio study on above threshold multiphoton dissociation and non-dissociative autoionisation in hydrogen reproduced observed photoelectron energy spectrum, Photodissociation dynamics of LiH molecule by using Fourier Grid method, Lasing without population inversion in small molecules in presence of coherent light and squeezed light are being investigated. Measurements on the charge transfer processes in doubly charged nitrogen molecular ion using Transitional Energy Spectroscopy have been initiated. Laser Raman spectroscopic studies on crystalline state photodimerisation reaction, Surface enhanced Raman scatering using LB technique, a systematic investigation of Raman profiles of some double molecules have been carried out and further extension of the programmes are contemplated. Studies of spontaneous polarisation and Response time of a new electro-optical material based on Ferroelectric liquid crystal dispersed in a polymer matrix, which is suitable for large area displays has been made. Electro-optic and dielectric spectroscopy in the SmC* and SmCa* phases of a liquid crystal material are in progress in a frequency range from 10Hz - 13MHz. Studies on photophysical/ photoconductive and photoinduced electron transfer reactions within several electron donor and acceptor systems, synthesis of several biochromphores, mimic to photosynthesis devices, studies on photoluminescence quenching in a regular polythiopene in pristine and annealed films using Ti:Sapphire laser and streak camera with CCD have been successfully carried out. Twisted molecular charge transfer has been identified in S-N,N-dimethylaminocinnamaldehyde from theoretical and experimental stand point which seems to compete with hydrogen bonding interaction in protic solvent. Encapsulation of this molecule by a- and b- cyclodextrin brings forth new interesting complexes. Dark and Photo-conduction properties of some organometallic compound have been carried out with special emphasis on checking the temperature dependent fluctuations in the factor (g). Investigations on the non-linear behaviour of some organometallic compounds in the vapour-adsorbed state, both by electrical and spectroscopic methods are in progress.

Theoretical Physics

In atomic and molecular physics positron-hydrogen scattering of ortho positronium off helium target, ionisation of atoms by various means and ionisation and excitation in the presence of a laser have been studied. In positron-hydrogen scattering, the effect of target inelastic channels is found to be significant. The total cross section for the ortho-positronium scattering is in good agreement with measurements carried out at University College London. In particle Physics, the decay of heavy hadrons within and beyond the standard model has been carried out with particular emphasis on the decay of the rare B and D mesons. Neutrino induced muon production and gamma ray induced interactions have been the theme of astroparticle physics research. Work done in the area of biophysics and environmental science centres round the statistical analysis of the coding and non coding parts of DNA. Heavy metal pollution and its effect of marine life has been studied. Research in statistical physics nonlinear dynamics etc. has led to the analytical observation that the plane Conetle flow that is known to be stable at all Reynold's number can because unstable if there is a small imperfection in the plate geometry.

Energy Research Unit

The process of setting up of a prototype plant for the production of large area multijunction a-Si solar modules has been started under a project funded by Department of Science and Technology and Ministry of Noncon-ventional Energy Sources. Transparent conducting Zinc Oxide films have been developed by r.f. magnetron sputtering. Using a layer of ZnO as back Reflector in double junction solar cells (area~1cm2), 11.7% increase in efficiency has been achieved. The integrated electrical-optical modelling programme set up in this laboratory, has been used to analyse the junction of two component subcells in tandem solar cells. The role of substrate temperature on the phase transition between amorphous and nanocrystalline/ microcrystalline silicon films have been studied using x-ray diffraction, Raman scattering, SEM, TEM and conductivity measurements. The intrinsic mc-silicon layer with low light induced degradation has been developed for the active layer of solar cells. Work on solid phase crystallisation of a-Si films have been started. A new project has started jointly with a French group to develop a new variety of Si:H alloy which has been termed "polymorphous silicon". Preliminary studies have shown that the material has lower degradation compared to standard a-Si:H. Under a DST sponsored project studies on glow discharge plasma has been made by optically emission spectroscopy and Laugmuir probe. Under a project funded by Aeronautical Development Agency(DRDO) process for depositing Radar opaque optically transparent coating on polycarbonate substrate has been developed.

MLS Processor's Unit

Newer types of nanocomposites have been designed and synthesized. Composites of nickel-zinc ferrite and nanosized iron particles show interesting magnetic properties - it now seems possible to make materials with desired magnetization and coercivity in a wide range. Nanocrystalline oxides when grown within a suitable gel matrix exhibit unusual electrical conductivity which has been ascribed to an interfacial amorphous phase. Metallic nanowires have been grown within a polymeric film as well as nanopores of a silica gel.

Biological Chemistry

Oligosaccharides related to the antigen from Shigella dysenteriae types 3,4 and 9, S. boydii type 5 and D-parosamine have been synthesised as a part of our work towards the development of carbohydrate based antibacterial vaccines. Lectin-carbohydrate interaction plays a major role in infection process as demonstrated by enhanced infection to jute seedling by phytopathogen. Macrophomina phaseolina in presence of its extra cellular agglutinin as well as jute cell wall carbohydrates. Influence of different plant growth hormones on the mycelial growth and lectin production has shown acid gibberellic acid to be the most potent among many others, viz. Kinetin and indole acetic acid. Secondary structures of somatic and excretory-secretory antigen of Ascaris lumbricoides helminth have been determined by circular dichroism study. Among IgE-reactive antigenic proteins in Rohu, Hilsa and Pomfret fishes, the same present in Hilsa has been found to cause high degree of food allergy in patients allergic to fish studied among population in greater Calcutta. Swollen chitosan beads and gels prepared from shrimp shells have been found to be very efficient in removing metal ions from effluent. The beads and gels after treatment can be reused for number of times. Isolation of lactose from whey using chitosan gel as demineralising agent is being studied. It has been found to remove metal ions from whey without increasing its volume. With the objective to understand the differentiation process, a new project was initiated. Differentiated plant tissues (carrot, Solanum nigrum and Dalbergia sissoo) have been transformed to undifferentiated callus. An alpha-turn mimetic, g-turn induced hairpins and 5-membered NH….N hydrogen bonded rings (a novel motif) have been successfully designed in model pseudopeptides and peptides using nonprotein amino acids with aims to mimic protein structural elements and to create novel motifs that are not found in nature.

Inorganic Chemistry

The activity of the Department centres around : synthesis of metal bound azo anion radicals, oxorhenium(V) complexes and their reactivity toward diphosphines, new organometalalics through insertion of alkynes/ isonitriles in M-C bonds, polyol chelation in oxovanadium species, metal-promoted regioselective aromatic ring amination processes at coordinated diaza ligands, redox and spectral properties of di- and poly-metallic complexes involving RuII-CuII, OsII-CuII etc., new Tri- and tetra-aza macrocycles, photoluminescent copper(I) complexes, reactivity of Pd(II) chelates with vitamin-B6 molecules, electron transfer pathways in bridged manganese(III,IV) systems, low temperature magnetic interactions in one-dimensional bridged copper(II) polymers, water-soluble polymeric dioxovanadium(V) compounds with extended helical structures, binuclear molybdenum(VI) complexes with multidentate N,O donors, reversible oxygen binding in high-spin cobalt(II)-pentacoordinated species.

Organic Chemistry

The continuing research efforts have unfolded novel methods of carbon-carbon bond formations mediated by photocycloaddition reaction, metal mediated selective bond formations, transition metal induced radical reactions, Lewis acid catalysed and microwave assisted processes. These have been successfully applied for the total synthesis of some bioactive monoterpenes and sesquiterpenes and related compounds containing unusual carbo- and heterocyclic structures. A number of nitrogen and sulfur heterocyclic systems have been synthesised employing transition metal induced cyclisations and these will be of use for studying structure-activity relationships. A total of 15 papers have been published in reputed journals.

Physical Chemistry

Recording and analysis of single vibronic level luminescence and Hole-burning spectra of organic molecules, observation and analysis of ultrafast solvation dynamics in lipids and sol-gels, correlating features of excited state intramolecular proton transfer (ESITP) with the nature of the potential energy surfaces on which the transfer takes place and the use of ESIPT as a probe for polymer-surfactant interaction highlight the experimental research activities of the department. In theory, remarkable results obtained by us include prediction of core effects on the ionization potentials of heavy atoms by relativistic coupled cluster based linear response theory, demonstration of environment induced dynamical chaos and tracing the origin of the symmetry that exists between the growth and decay of fluctuations in thermalised quantum systems.

Polymer Science

During the year under review researches in the following areas were carried out : conducting polymer colloids, controlled/living radical polymerization, polymer blends, polymer crystallization, polymer gelation, elastomer blends and polymer-surfactant interactions. Conducting polymer colloids provide a valuable method of processing the intractable conducting polymers. We have investigated mechanisms of the formation of polyniline (a conducting polymer) colloids so that better colloids can be prepared and utilized. Controlled/Living radical polymerization has emerged as a very important means of producing various polymers with controlled chain length, well defined end groups and polymer molecules of nearly uniform chain lengths. Such materials are greatly sought after in fabricating advanced materials. We have explored the applicability of the method for water soluble polymers such as polyacrylamide. Crystallization behaviour of polymers has been studied for polymer blend systems comprising of poly(ethylene terephthalate)(PET), an important commodity polymer, and poly(vinylidene fluoride) (PVF2), a piezoelectric polymer. The study suggests that these two polymers are miscible in the melt. In another study which involves blending the crystalline piezoelectric polymer PVF2 with an amorphous polymer, poly(methyl acrylate), gels were found to be formed and these gels were proved to contain solvents which are complexed with the polymers. Furthermore, detailed investigations are in progress for characterizing some conducting polymer gels e.g. polyaniline sulphonic acid gels and poly(3-hexylthiophene) gels. Systematic studies were carried out on the covulcanization of blends of rubbers which vary greatly in polarity and unsaturation. Some of these blends may exhibit improved properties and therefore may find commercial utilization. Polymer surractant mixtures have great application potentials. A fundamental understanding of these systems is also of great theoretical interest. In this vein a detailed study on the solution properties of some cationic detergents in presence of the water soluble polymer hydroxypropylcellulose was pursued. Investigations w ere also carried out on the solution properties of micellar solutions of mixtures of ionic and nonionic surfractants which may yield surfactant systems with novel properties.

Indian Institute of Astrophysics, Bangalore

The major activity of the Institute during the above period was directed towards the preparations for the installation of the Optical/Infrared Telescope of 2-meter aperture at the Indian Astronomical Observatory (IAO) at Hanle in Ladakh, at an altitude of 15000 feet above mean sea level, the highest astronomical site in the world. This telescope being capable of remote operation, the Satellite Communication and Control Station had to be established at the Centre for Research and Education in Science & Technology (CREST) campus of the Institute at Hosakote near Bangalore. The dedicated team of scientists and engineers of the Indian Institute of Astrophysics working in close cooperation with various agencies of the Government and institutions in the private sector accomplished these challenging and multifaceted tasks with speed, economy and efficiency.

The following facilities were established at Hanle to be in readiness to install the telescope that was expected to arrive there in the summer of 2000:

  • Solar Power Plants, 2 Nos., each of 30 KW peak power with adequate storage for operating the telescope for 3-nights without additional input.
  • Liquid nitrogen plant, for cooling the CCD cameras.
  • Satellite based communication links (2 Nos.) to the remote control and operation station at Hosakote, one 2 Mbps duplex and one 64 kbps duplex.
  • Dome of 10.5m diameter and 16m high with innovative design (by IIA), capable of automatic operation.
  • Cmputational facilities for a variety of purposes such as, control of power, the focal plane instruments, the dome, communication system etc..
  • Facilities for scientists, engineers and technicians to stay.
  • Facilities for archiving the data.
  • Power and communication cables interconnecting the various units.
  • The road from the valley to Mt. Saraswati.

The CREST on the land donated by the Government of Karnataka in Hosakote, was equipped to complement the infrastructure at Hanle. The control and operation centre at Hosakote was equipped with communication equipments; computers and office space for round the clock activities. Suitable facilities are also created for archiving the astronomical data.

The Vainu Bappu Observatory (VBO) at Kavalur also made important observations during the year and new facilities were commissioned at the Observatory. The Liquid Nitrogen Plant installed on the Observatory grounds provides more than 5 liters of LN2 per hour and all the requirement of the coolant for the CCD-cameras. A new medium-resolution spectrograph commissioned to work with the Vainu Bappu Telescope is functioning satisfactorily.

The readiness of the facilities at VBO may be seen from the recent multi-band observations from VBO of the after-glow of the gamma ray burst GRB000301c, which was detected by the All-Sky Monitor on board the Rossi X-ray Timing Explorer on 2000 March 1, 4108 UT (universal time) and also by Ulysses and NEAR. The coordinates of the event, R. A. =16h 20m 21s.5 and declination = +29024'56".37 within an error box of 50" x 50", was communicated internationally to all observers, and within three hours of the receipt of the electronic-mail, the multi-band photometric observations were commenced at VBO, and these provided important anchor points for delineating the light- curve of the after-glow of the gamma ray burst.

More details of the scientific research and development activities during the year are given below.

Scientific Research

Sun And The Solar System

Solar Physics

The Kodaikanal Solar Observatory operated by the Institute has a large database consisting of daily full disk white light solar images over a period of several decades (1906 - 1987). The long-term programme of analysing these images is continuing. Recently, Institute's scientists in collaboration with scientists from some other institutions in the world have succeeded in measuring the positions and areas of all sunspots (numbering 332620) to an accuracy of about 0.5 arc see from 18,900 images covering the 82 year period. Two important measurable quantities have been extracted from this data set, namely, (i) the solar rotation rates at different solar latitudes and the variation of the rotation rate with the solar cycle, and (ii) the tilt angles of spot groups (i.e., the angle between the line joining the centroids of the Leading and the Following spots in the group and the local parallel of latitude). From the measurements of the rotation rates of the spots two important results have been established, namely (a) bigger spots generally rotate slower than the smaller spots and (b) the residual rotation rate (in degree per day) of all spots shows that the rotation during the years of solar minimum is faster than that during the solar maximum years. These results as well as those of the tilt angle measurements of the spot groups have important implications for the dynamics of the solar interior, in particular, for the structure and dynamics of the solar magnetic field, which are being studied in details.

A Stokes Polarimeter was developed and successfully installed at the Kodaikanal Tower Telescope to study the vector magnetic field of sunspots. A sunspot KKL 21263 (NOAA 8516) was observed with this instrument and the associated magnetic field parameters were successfully determined. This instrument is expected to provide many valuable data pertaining to solar magnetic fields in the years to come.

A continuing puzzle in solar physics is the unknown mechanism by which the Sun is able to maintain a very hot atmosphere (called "chromosphere") above its surface without losing the heat through conduction to the surface. The main sites in the chromosphere where the heat is thought to he generated are the so-called "bright points". There are generally two opposing schools of thought regarding the nature of these bright points, one claiming association of these bright points with magnetic phenomena and the other modelling them as purely of hydrodynamic origin. In this context, recent work by Institute's scientists have provided strong support to the magnetic association hypothesis by firmly establishing the association of the bright points in the interior Of the Calcium 11 K line network in the solar chromosphere with the underlying sub are see magnetic elements at the photospheric level.

In another piece of work on solar chromosphere, by analysing data provided by the SOHO, Institute's scientists have found evidence for the existence of the so--called "meso-scale granulation" in the solar upper chromosphere, of roughly the same size as observed earlier in the photosphere and lower chromosphere. These meso-granulations, which are convective cells arising from the solar convection zone and having horizontal sizes in the "medium" range of few thousand kilometers, are found mostly in the photosphere and are generally not seen to extend to the chromosphere. Thus, this new result, if confirmed by future detailed studies, has important implications for the energetics of solar convection process.

There has also been important theoretical work done in the Institute on the problem of solar chromospheric beating with the aim of identifying the precise mechanism by which energy is transported from the photosphere to the chromosphere through the magnetic flux tubes. In this direction work has been done to study the excitation of oscillations in the magnetic network of the Sun through the foot point motion of photospheric magnetic flux tubes located in the intergranular lanes. Result of this study shows that in order to transport enough energy on a sufficiently steady time scale to account for chromospheric beating, one need to include the effect of turbulent convective flows on flux tubes in intergranular lanes.

The problem of explaining the heating of the solar corona and maintaining it at a temperature of - a million degrees constitutes one of the most enigmatic of all the major unsolved problems in solar physics. Institute's scientists have used the coronal spectroscopic data from the ground-based Norikura Solar Observatory of National Astronomical Observatory of Japan and the space-based SOHO images to throw light on this problem. From the power spectral analysis of the time-series of line intensity, line width and Doppler velocity data obtained from the time sequences of the coronal emission line spectra in Fe X 63740 A and Fe XIV 53030 A, strong evidence for coronal oscillations with periodicities in the range of a few minutes to a few tens of minutes has been established. In particular, a 3-minute periodicity is consistently seen in both green and red line spectra reported earlier by scientists elsewhere using independent data. These results lend strong support to the hypothesis that magnetohydrodynamic (MHD) waves of short periods (- minutes) are responsible for the energy transport to and heating of the corona.

In another piece of work, Institute's scientists have discovered interesting correlationship between the magnetic activity in some persistent active regions of the Sun and the enhancement of the 53030 A coronal green line emission, a result that might have important bearing on the role of magnetic fields in the coronal heating problem.

Study of the Sun in radio wavelengths is continuing in the Institute using the Gauribidanur radio telescope operated by the Institute. Radio emission associated with transient Extreme Ultraviolet (EUV) jets from polar regions of the Sun was identified for the first time with the Gauribidanur radio heliograph. This instrument has also provided important data on the coronal mass ejection events of April 13, 1997 and September 12, 1998.

Solar Terrestrial Physics

The Solar Terrestrial Physics (STP) group of the institute participated in the Equatorial Spread F (ESF) campaign held during April 1999 under the Indian Solar-Terrestrial Energy Program (I- STEP). Regular data acquisition in the monitoring mode continued with the experimental facilities (IPS42 digital ionosonde, HF Doppler Radar and Magnetometer) at Kodaikanal Observatory.

A comprehensive study of the ionospheric storm of November 4, 1993 in the Indian equatorial region was undertaken in the Institute because of, the absence hitherto of an assessment of the response of equatorial upper atmosphere to this magnetic storm. The study, based on data from the ionosonde and magnetometer networks in the country, brought to light several new facets of the storm-time behavior of the equatorial ionosphere, indicating, in particular, a significant electrodynamic coupling between high- and low latitude ionosphere.

Work is continuing in the Institute on the inter-relationships between solar wind, magnetosphere and ionosphere. The global manifestation of the waveform of the geomagnetic storm sudden commencement (SC) of November 18, 1993 has been evaluated using high time resolution data of several magnetometer networks coupled with HF Doppler Radar measurements at Kodaikanal. The work revealed that the dip equatorial appearance of the preliminary reverse impulse (PRI) of the SC deviated quite significantly from the pattern established by previous statistical studies as well as the one predicted by currently available theoretical models of SC.

Institute's scientists are also involved in detailed study of the effects of Meteor Showers on the ionosphere. In particular, the effect of Leonid meteor showers during the years 1996 through 1998, on the characteristics of sporadic-E layers at equatorial latitudes has been studied using data of rapid ionospheric soundings at several stations in the country. The results showed an increase in the occurrence of Es layers at altitudes in the range 100-140 km throughout the equatorial region at the times of peak shower activity. The finding underscores the need for further studies to ascertain the origin of the observed changes in Es behavior, in particular the relative roles of deposition of metallic ions due to shower activity and the physical mechanisms that cause ion-convergence and lead to Es layers.

Solar System Objects

Following the earlier observations of the Comet Hale-Bopp at the Vainu Bappu Observatory (VBO), Institute's scientists are currently involved in determining the physical nature of the cometary grains in this comet. The porosity and organic fraction of the grains have been determined by comparing the computed variation of polarization of the light scattered by an ensemble of grains of various different assumed porosity and organic fraction with observational data. In addition, by modelling the spectro-polarimetric observations of the Comet Hale-Bopp done earlier at VBO, new information on the grain composition, namely, the proportion of glassy versus crystalline silicates has been obtained.

Stars And Stellar Systems


The study of stars of various types - their composition, structure and evolution - constitutes a subject of intense research activity in the Institute.

Important new insights have been obtained on the nature of the so-called R Coronae Borealis (RCB) stars. These stars are photometrically distinct from other stars by their decline at unpredictable times by one to several magnitudes, as a cloud of carbon soot obscures the stellar photosphere for weeks to months. Spectroscopically, the distinctive signature of an RCB is weak Balmer lines which indicate an atmosphere deficient in hydrogen. What are the evolutionary paths by which some stars with their normal hydrogen-rich atmospheres are converted to RCBS with helium-rich atmospheres? And what are the physical processes that trigger and control the development of the unpredictable photometric decline of these stars? These are two of the fundamental questions about RCB stars that researchers are currently trying to answer.

A set of high-resolution optical spectra of R CrB star acquired before, during and after its 1995-96 decline has been analyzed by Institute's scientists in collaboration with scientists from several other Institutions in the world in order to attempt to answer the second of the above questions. This novel data set provides new information on the decline of the star. This includes the discovery that the onset of the decline is marked by distortions of absorption lines of high-excitation lines, and quickly followed by emission in these and in low-excitation lines. This 'photospheric trigger' implies that dust causing the decline is formed close to the star. An outcome of the above analysis is that R CrB might have a compact companion surrounded by an accretion disk. This suggestion has been submitted as a proposal to the Hubble Space Telescope (HST) for high resolution UV spectroscopy in collaboration with scientists from several other Institutions in the world. The proposal has been accepted and 13 orbits have been allocated for this study.

Among other works on RCB stars, the surface abundance analysis of 18 R CrB stars has been completed. In an interesting piece of work, the presence of cool gas (T ~ 1100 K) in the atmosphere of the R CrB star V854 Cen during a deep minimum has been detected by the analysis of C2 molecular lines. This is an important observation which indicates that dust nucleation occurs in the atmospheres of these hot stars (Teff ~ 7000 K) after passage of a shock wave.

In the context of stellar evolution, work on the atmospheric abundances and physical properties of intermediate temperature He stars is being pursued in the Institute using high resolution spec troscopy and model atmospheres exclusively developed for this programme.

Another area of stellar astronomy in which significant new results have been obtained by Institute's scientists is the so-called post-AGB (post-asymptotic giant branch) phase of stellar evolution. During this phase in the advanced stage of evolution of typically low-mass stars, substantial mass loss occurs from the outer envelop of the star. The ejected mass, which forms a shell around the hot central star, is ionized by the radiation from the hot central star and is visible as a planetary nebula. The central star, subsequently cools, contracts and ends up as a white dwarf.

One of Institute's scientists in collaboration with a team of international scientists has studied the rapid evolution of a newly horn planetary nebula - the so--called Stingray Nebula - by analyzing the images of this nebula obtained with the Hubble Space Telescope. This study has provided new insights on the early structure and evolution of planetary nebulae.

Interstellar Medium

Work is being done on the so-called Young Stellar Objects (YS0s). Stars are born in the cores of interstellar molecular clouds. In their early pre-main-sequence phase, these "stars" or YS0s are still surrounded by their parent cloud envelop and often have circumstellar disks that drive bipolax jets and outflows and also cause polarization of star light by scattering. Institute's scientists are studying YS0s in several star forming regions by emission-line imaging, spectroscopy and polarimetry, and have so fax observed about 25 of these objects. This study is likely to yield important insight into the process of star formation.

Gamma Ray Bursts

Sustained efforts over the past few years fructified this year when Institute's scientists were able to make early observations of the afterglow of the Gamma Ray Burst (GRB) GRBOO0301c. Multi-band observations of the Optical Transient (OT) associated with GRBOO0301c was carried out between 2-4 March 2000 using the 2.34-m Vainu Bappu Telescope (VBT) at Kayalur. When combined with other reported data, the initial decline in the R-band magnitude with log (t - to), the time since the burst, is fit with a slope a1 = -0.70 + 0.07 which steepens after about 6.0 days to a slope of a2 = -2.44 + 0.29. It is found that this change in slope does not occur smoothly, rather there is an indication of a possible bimodal distribution. The available measurements of the evolution of (B-R) color do not show any discernible evolution in the first 12 days. These observations have important implications for the GRB models which are currently under investigation.

Theoretical Asrophysics

Radiative Transfer

Radiative transfer continues to be one of the major areas of research activity in Theoretical Astrophysics in the Institute.

Using detailed radiative transfer calculations, the Institute's scientists had shown in the previous year that the observed linear polarization in the molecular lines of C2, MgH, ete in the spectrum of the quiet sun is caused by coherent scattering processes in the solar atmosphere as in the case of atomic lines. Extending that work further, the parameters such as the oscillator strengths, the inelastic collision rates, and depolarizing elastic collision rates for a number of observed molecular transition lines in the solar atmosphere have now been obtained, which have important implications for the states of various molecules in the solar atmosphere.

Radiative transfer calculations were used to understand the nature of the recently discovered brown dwarf Gliese 229B. In particular, the formation of methane line at 2.3 micron in Brown Dwarf Gliese 229B was studied. By fitting the synthetic continuum, spectra with the observed spectra at a wide range of wavelengths, the physical properties of the object such as the elective temperature and surface gravity were determined.

Magnethydrodynamics (MHD)

A remarkable fact about the large-scale magnetic fleid in the Sun is that it is mostly concentrated in isolated magnetic flux tubes at the visible surface and also in the form of coronal loops where the field strengths are of order 1500 Gauss. Why flux tubes rather than uniformly distributed magnetic field? Institute's scientists are engaged in attempts to answer this question by studying the relaxation of a compressible plasma to equilibrium configuration with flow. Three classes of equilibrium solutions corresponding to energy extrema satisfying the constraints of conservation of mass, energy, angular momentum, cross helicity and relative magnetic helicity, have been found. One of these solutions with increasing radial density profile has been identified to be relevant for solar flux tubes. Further studies exploring the stability of these solutions are in progress.

Plasma physics and accretion process

A kinetic theory of the Jeans instability of a dusty plasma has been developed. The effect of grain charge fluctuations due to the attachment of electrons and ions to the grain surface has been considered. It is demonstrated that the grain charge fluctuations alter the growth rate of the gravitational collapse of the dusty plasma.

It is shown that a certain class of flare models for variability from accretion disk coronae are subject to beam-plasma instabilities. These instabilities can prevent significant direct acceleration and greatly reduce the variable X-ray emission argued to arise via inverse Compton scattering involving relativistic electrons in beams and soft photons from the disk.

The process of formation of quasar black holes from magnetized accretion of a collapsed disk has been studied. It is shown that, in a self-similar accretion flow model, for typical halo parameters, about IOSMD accretes (thus forming a black hole) via small magnetic stresses (or alternatively by self-gravity induced instability) in ~ 108 years. A model of self-gravitating evolution of a compact magnetized disk has also been studied. The formalism can be applied to other contexts like formation of protostellar disks as well, and has important implications for dwarf galaxy formation and a residual large scale seed magnetic field.

Galactic Dynamics

It is known that more than 90% of the material content of the Universe is in the form of some unknown, invisible matter. The nature and distribution of this so-called "dark matter" in the Universe is one of the major unsolved problems of contemporary cosmology. This dark matter, widely believed to he constituted of some unknown weakly interacting particles of small mass, is a major component of the total masses of individual galaxies, including that of our own Galaxy, the Milky Way, as well as the masses of clusters of galaxies. Institute's scientists are engaged in trying to decipher the phase space distribution of these dark matter particles in our Galaxy from various observational data. An efficient Poisson Equation solver for axisymmetric mass distributions has been developed for this purpose using the method of spherical harmonics expansion of the gravitational potential of dark matter in the Galaxy. This code has been used to self-consistently solve the phase space distribution of the dark matter coupled to the visible matter in the Galaxy. The results show that in order to explain the Galactic rotation curve data and the dynamics of the dwarf spheroidals in the outskirts of the Galaxy, the velocity dispersion of the dark matter particles in the solar neighbourhood has to be >~ 570 km s-1, a value significantly larger than the usually assumed value of ~ 270 km s-1. This result is important in the context of interpretation of the data from various experiments that are currently underway at various laboratories in the world to directly detect the dark matter particles in cryogenic detectors, and implies important constraints on the nature of the dark matter particles.

Important new results have also been obtained in the study of galaxy dynamics by means of numerical N-body simulations. These include a study of the tidal effects on a satellite galaxy caused by a centrally concentrated massive perturber, an investigation of oscillations of galaxies, a study of the process of violent relaxation in elliptical galaxies, and several other related issues.

Atomic Astrophysics

Atomic Astrophysics is another branch of Theoretical Astrophysics in which important work has been done in the Institute in the past year. A knowledge of excitation energies and oscillator strengths of allowed as well as forbidden transitions is crucial for the determination of abundances and temperatures of a variety of astronomical objects. Relativistic many-body calculations of the oscillator strengths of the allowed, intercombination and magnetic quadrupole transitions of the berrylium sequence have been done using the multi-configuration Dirae-Fock approach. This work highlights the significance of electron correlation in these studies. Using a variant of the multi- reference many-body perturbation theory known as the effective valence Hamiltonian method, the excitation energies, ionization potential, electric dipole moments and oscillator strengths for cyclic and linear isomers of the C3H radical were calculated. This radical is present in the interstellar medium like the dark molecular cloud TMC1 and in the circumstellar shell of highly evolved carbon star IRC+10216.

High Energy Astrophysics, Astroparticle Physics and Cosmology

Neutron Stars and Pulsars

Neutron Stars and Pulsars is an area of research in which Institute's scientists have made major contributions over the years. The main theme of the work done in this area in the past year has been the study of General Relativistic effects pertaining to physics in and around pulsars which are strongly magnetized rotating neutron stars.

By studying the General Relativistic effects on the propagation of light in the vicinity of pulsars, it has been shown that the spacetime curvature introduces a shrinking of the magnetic field lines towards the magnetic poles by a small magnitude. This tends to overcome the divergence of the pulsar beam caused by the light bending effect. It is proposed that these relativistic effects may be observable in the case of millisecond pulsars. In addition, it has been shown that these relativistic effects, together with various observational constraints on pulsars, put severe constraints on the equation of state (EOS) of the neutron star matter. In particular, very soft EOS's are preferred, as would be the case, for example, if the neutron stars were actually the so-called "strange stars" made up of u, d, and s quarks instead of neutron matter.

Important constraints on the EOS of neutron star matter have also been obtained by studying the properties of accretion disks around rapidly rotating -neutron stars with low surface magnetic fields in Low Mass X-ray Binaries (LMXBS) including the full General Relativistic effects. In particular, using the EXOSAT data on the X-ray spectrum of Cygnus X-2, it has been inferred that the neutron star in Cygnus X-2 rotates close to the centrifugal mass-shed limit.

The General Relativistic effects on Joule heating of neutron stars have also been studied. It is found that, although the effect of space-time curvature produced by the intense gravitational field of the star slows down the decay rate of the magnetic field, the modification of the initial magnetic field configuration and the initial field strength by the space-time curvature results in increasing the rate of Joule heating. This gives strong support to the hypothesis that Joule heating is responsible for maintaining a relatively high surface temperature which is consistent with the observation.

Astroparticle Physics, Cosmology and Early Universe

A model for the origin of MeV emission from blazars has been developed, that involves the produc- tion of MeV gamma rays through Inverse Compton (IC) scattering of electrons in the blob of the blazar jet with the UV photons of the accretion disk around the central supermassive black hole. The OSSE and the COMPTEL spectra of the blazar PKS 0528 + 134 have been fitted with the computed MeV gamma ray fluxes of this model. Possible emission of TeV energy photons through synchrotron self compton (SSC) processes in this model has also been suggested.

Stringent constraints on the mass and charge of photon were put based on the arrival times of radiation at different wavelengths (radio, optical and gamma rays) from the gamma ray burst GRB 990123. Also, limits on certain parameters (such as the string scale) relevant to quantum gravity theories were obtained. Analogous to the situation in SN 1987A, from the various delay times, stringent limits were put on deviations from the validity of the Einstein equivalence principle for photons over a wide (12 orders of magnitude) energy range.

Recently there have been attempts to revive alternative cosmological models different from the standard Big Bang model, which are supposedly able to account for both the microwave background and light element abundances. Theoretical work done in the Institute has, however, shown that the cosmic neutrino background in these alternative models would he vastly different both in energy and number density from that predicted in the standard Big Bang model. One can thus envisage future neutrino based observations which can differentiate between these models.

Important theoretical work has been done in the Institute on the process of black hole evaporation. By applying ideas of non-equilibrium thermodynamics initially developed for glassy systems, this work has shown that the Hawking temperature of the primordial black holes formed in the early Universe would always be much lower than the corresponding ambient temperature, which would inhibit the evaporation of these black holes. This result has important implications for observability of primordial black holes through the Hawking radiation process.

The abundance and the size distribution of the so-called "quark nuggets" (QNs), a possible relic from a first order phase transition from quark-gluon matter to hadron in the early Universe, have been calculated. It is found that a significant fraction of QNs may have been formed with initial baryon number large enough that they survive through their subsequent evolution, so that QNs may significantly contribute to a baryonic component of the dark matter in the Universe.

A stringent constraint on the total mass density of the Universe has been derived from the Sunyaev- Zel'dovich (SZ) effect - the distortion of the Cosmic Microwave Background (CMB) due to scat- tering with the hot electrons in a cluster of galaxies. It is found that a low matter density (including dark matter) Universe is favored, indicating that there may be significant amount of "vacuum en- ergy" (contributing as a cosmological constant term in the Einstein equation) for a critical Universe. In addition, the effect of cooling flows in clusters of galaxies on the determination of the Hubble constant from SZ effect, as well as SZ distortions of the GMB due to galactic winds at high redshifts have been studied.

An impressive variety of recent observations which include luminosity evolution of high red shift supernovae strongly suggest that the cosmological constant (A) is not zero. Even though the A- term may dominate cosmic dynamics at the present epoch, such a value for the vacuum energy is actually unnaturally small, and is difficult to explain. Theoretical work done in the Institute, based on ideas of phase transitions in the early Universe, has shown how such a small residual cosmological constant term of the correct magnitude can arise from fundamental physics. In addition, the role of gravitational spin interactions in generating a residual cosmological term has also been explored.



Experimentation on Adaptive Optics is in progress in the Institute. The piezo tilt mirror has been calibrated in the laboratory using the Zygo Interferometer. The algorithm to measure the centroid correction has been tested. The calibration of the CMOS CCD is in progress. Efforts are on to procure a Shack Hartmann sensor to develop the laboratory Adaptive Optics system.

Work is also being done on wavefront sensing. The algorithm to retrieve the phase from a single shearing interferometric record is being developed. The results from different approaches are being compared for their efficiency in terms of minimum duty cycle per operation. In the mean time efforts are on to build a Shack Hartmann sensor to compare the two methods.

In theoretical optics, scattering of light by a rough phase grating has been studied. Light scattered by a pure phase grating is known to have a periodic structure with respect to the angle of scattering. In the present work it is shown that while roughness smears out the sharpness of this structure, the broadening of the peaks is dependent on the nature of the randomness (whether Gaussian or Cauchy type, etc.). Thus the hidden periodic structure can be detected by observing the pattern at different wavelengths. Detectibility of such periodic structures hidden behind randomness is one of great importance, e.g., in remote sensing.

Foundations of Quantum Theory

A resolution of the celebrated Einstein-Podoisky-Rosen (EPR) nonlocality puzzle in quantum mechanics has been proposed. The EPR puzzle is one Ofethe most discussed fundamental problems in physics. A seemingly inescapable feature of the standard version of quantum mechanics is its nonio- cality - it seems to require the existence of apparently superiuminal and mysterious communication between the space-like separated subsystems of an initially correlated, entangled quantum system. The present work has shown that the quantum correlations of space-like separated entangled particles can be reproduced starting from local probability amplitudes, quantities that preserve the relative phase information. Use of complex number amplitudes circumvents the widely discussed Bell's theorem on the impossibility of a local realistic description of quantum correlations. The objective reality in this formulation is at the level of initial phases that cannot be measured, and there is no determinism. The result implies that there is no 'spooky action-at-a-distance' in the correlations and resolves the EPR nonlocality puzzle. Also, they imply that the present interpre- tations of seemingly nonlocal phenomena like quantum teleportation and entanglement swapping are not correct.

A related issue is the so-called Complementarity Principle which is a basic foundational principle in the Copenhagen interpretation of quantum mechanics. It derives its roots from the uncertainty principle and has never been seen violated in interference experiments. Usual interpretation of the principle invokes the analogy with the Heisenberg microscope thought experiment where the physical origin of complementarity is traced to the position-momentum uncertainty principle. Loss of interference in atom interferometry experiments, where the "which-path" information can he obtained without disturbing the spatial wavefunction of the atoms, could not be explained within this picture and has been a subject of extended debate in the last decade. Recent work done in the Institute has shown that the physical origin of complementarity in this case is a discrete, but random phase change arising from the de-excitation of the atom, equivalent to the rotation of a spinor though 180 degree. This clarifies how complementarity can arise without Heisenberg back-action on momentum, and settles a recent debate on this issue.

Gravitation and Black Holes

A new way to test relativistic gravitation has been suggested. It is suggested that modern techniques of radio ranging, when applied to study the motion of the Moon, can improve the accuracy of tests of relativistic gravitation obtained with currently operating laser ranging techniques. Other auxiliary information relevant to the Solar system would also emerge from such a study.

An investigation into the empirical question of possible shielding of gravity by matter has been done. This question is at present outside the scope of the standard theory of gravitation. This is mainly due to the fundamental feature of gravity that there is only one type (sign) of gravitational charge. On the other hand, the question whether gravity could be shielded or absorbed by an intervening medium has been important from an empirical point of view. The issue has been addressed experimentally during the last century in several laboratory experiments and astronomical tests, and theoretically by several physicists. The experimental activity was brought to focus by Q. Majorana who conducted several high precision experiments with a weighing balance between 1920 and 1930 to see whether there was absorption of gravitational interaction by intervening matter. A tiny shielding effect was detected. The results of an experiment being conducted at the Physik-Institut, University of Zurich to measure the gravitational constant was recently analyzed by a scientist of the Institute in collaboration with another scientist from the University of Virginia, USA. This analysis has yielded a rather tight constraint on the Majorana gravitational shielding factor. The limit obtained in this analysis is two orders of magnitude lower than the positive results obtained by Majorana and a factor of about 5 better than the constraint obtained by Braginsky in a more modern laboratory experiment.

The long-term research project investigating Black holes in non-flat backgrounds in General Relativity is continuing in the Institute. The research pertaining to black holes has so fax been focused mainly on isolated stationary ones (Schwarzschild and Kerr). These two properties are equivalent to asymptotic flatness and time symmetry respectively. In a realistic situation, considering external influences such as local mass distribution or the expanding universe, neither of these properties may be valid. It is extremely important therefore to find out whether the known properties of black holes are modified, radically altered or retained unchanged. Towards this end the study of black holes in non-flat backgrounds has been undertaken. As a first step in this complicated investigation, the condition of asymptotic flatness has been relaxed retaining time symmetry. New results have been obtained regarding the geometry of the Kerr black hole embedded in the static Einstein universe and the properties of the energy-momentum tensor. Specializing to the non- rotating case, a composite model consisting of vacuum Schwarzschild black hole joined on to the Einstein Universe has been constructed. This enables the study of physical phenomena in the gravitational field of such a black hole in a non-flat background such as scattering of waves.

Non-Accelerator Particle Physics (NAPP)

Significant advances have been made in the Institute in the area of Non-Accelerator Particle Physics (NAPP) research.

On the theoretical side, work on Parity Non-Conservation (PNC) has continued. It has been recognized for about a decade now that PNC in atoms is an important non-accelerator probe of physics beyond the Standard Model. However, in order to make progress, it is necessary to improve the accuracy of the present atomic PNC theory. Relativistic and many-body effects play a crucial role in the theoretical determination of the PNC observable. Institute's scientists have been involved in the development of the relativistic version of an all-order many-body theory known as the coupled-cluster method for the last three years. Calculations based on this theory are highly computer-intensive. The major part of the work last year was the development and testing of parallel computer codes to carry out calculations of a number of different properties of Cs, Tl and Ba+ with an eye to determining the accuracies of the PNC calculations for those three atoms. These properties include ionization potential, magnetic hyperfine constants and transition amplitudes. Calculations were carried out successfully of the correlation energy of Tl+ with all the core electrons excited. The purpose of this work was to demonstrate the importance of core correlation for Tl PNC. The effects of nuclear structure on Cs PNC was also studied using the relativistic mean field theory. Studies of this kind are necessary for the analysis of atomic PNC as a probe of physics beyond the Standard Model.

On the experimental side, strong efforts are being made to equip the NAPP laboratory for pursuing several frontier experiments in Physics. A cylindrical ion trap has been designed and fabricated in collaboration with Indian Institute of Science, Bangalore. The necessary electron gun for ionizing the atoms has been fabricated. An air-core transformer has been designed and built to provide the necessary stepped-up RF voltage from a RF source. Initial experiments will be focused on trapping large number of ions. Necessary electronics for detecting the trapped ions is being developed. The vacuum system has been reconfigured into a differential pumping scheme to ensure better signal-to-noise ratio.

The "Casimir Balance" to measure the finite temperature correction to the short range Casimir force arising from confining the quantum vacuum modes of electromagnetic radiation is being tested. A new autocollimator using an array of high intensity LEDs as the source, spatially modulated by a high precision grid, and a CCD detector is fabricated and being assembled. This will be used for the measurement of the Casimir force at boundary separations ranging from 30 microns to 1 mm. A similar torsion balance designed to probe short range forces, hypothesized on the basis of results from scenarios motivated by string theory is also being fabricated. The goal is to search for possible new forces with a strength comparable to that of gravity, and a range as small as a millimeter.

Experiments on laser cooling of Helium metastable atoms is being done in collaboration with the laser cooling group at Ecole Normale Superieure, Paris (ENS), Paris. The cooled Helium atoms have been loaded into a magneto-optical trap and preliminary measurements on the trap life time has been done. The present goal is to load the cooled atoms into a magnetostatic trap in which the atoms are spin polarized. The collision loss rate due to ionizing Penning collisions are expected to be suppressed by a factor of about 105 for spin polarized atoms. After a measurement of the Penning loss rates, it is planned to proceed to experiments on evaporative cooling and Bose-Einstein condensation of metastable Helium.

Geodynamics of Continental Deformation

Experimental test of a hypothesis concerning the mechanism of continental deformation is being done by Institute's scientists using sub-centimeter precision Global Positioning System (GPS). Mathematical model of the process whereby continents deform in response to plate tectonic stresses is the major prerequisite for quantifying earthquake hazard and for refining our understanding of planetary dynamics generally. Global coordinates of marked points on earth with millimeter precision now make it possible to discriminate between contrasting hypotheses of this process by measurements of strain rate gradients across major faults in the deforming region. Ladakh Himalayas lying north of the Indo-Eurasian plate boundary, it being the fastest deforming region of the globe, is manifestly the most promising area for addressing this question. An experiment was accordingly designed in 1998 to determine strain rates along and south of the gigantic Karakoram fault which appears most prominently on satellite imageries as a deep 1000 km long gash in the earth stretching from the Pamirs to Mount Kailash in Tibet.

While a detailed analysis of the contemporary strain rate field in the region is in progress, preliminary studies clearly show that the intra-continental region in Ladakh bound by the Great Himalayas in the south and the Karakoram fault in the north does not deform as a nearly rigid plate, but as a viscous continental plate possessing a layered cake rheology.

Facilities for Instrumentation Development

This year saw major achievements by the facilities and instrumentation development and support groups of the Institute. The major activities of the various groups are briefly decribed below :

Electronics and Electrical Engineering Division

  • Linear CCD Camera for Autocollimators: A scheme to measure very small angular displacements (of the order of 10-9 radians) was developed using a Linear CCD camera.
  • This instrument will be used in one of the major fundamental physics experiments (the "Casimir Balance" experiment) being done in the Institute.
  • A Mosaic CCD Camera System has been developed using a set of Thomson-CSF 2K x 2K CCDs (THX7897M) in a 2 x 2 configuration for astronomical observation applications. The necessary data acquisition software to operate the mosaic camera system has also been developed, and after successfully testing the system in the lab, a few test runs were conducted with the 1-meter telescope at VBO, Kavalur.
  • Digital Spectrograph for Radio Observations: A new digital spectrograph for observations of Solar radio burst emission in the frequency range 30-80 MHz was constructed and installed at the Gauribidanur Radio Observatory of the Institute. The instrument is in successful operation since November 1999. Observations of solar radio bursts with this instrument coupled with imaging observations carried out with the existing Cauribidanur radio heliograph are expected to provide a valuable data base containing information on the location of the burst sources.
  • TAXI Board: A high speed general purpose data link PCB has been designed and is being fabricated. The data throughput rate can go up to 4 MBPS. The electronics is capable of transferring/receiving 32 bit parallel data over a serial link, and the board uses TAXI chip pair (Am7968 and Am7969) for transmitting/receiving parallel data.
  • Hardware Based Data Compression: A hardware approach to data compression has been implemented in order to compress/de-compress on-line CCD data as well as stored data. A high performance adaptive loss-less data compression (ALDC) processor, ALDCI-20S-HA from IBM, is used to implement compression/de-compression.
  • Recabling and Rewiring Activity at the 1-m Telescope: The vacuum tube version of the control electronics of the 1-m Carl Zeiss Telescope of the Institute installed in 1972 at VBO, Kavalur, was replaced with the state of the art telescope drive system, display system, dome drive system etc.. The cables and wires in the telescope at various locations were found to be weak in insulation properties and had turned brittle due to aging and environmental factors. To improve the reliability of the telescope, steps were taken to replace the cables and wires in a phased manner. High quality rubber cables and wires were used in the telescope rewiring. The entire recabling work of the telescope was completed in about three months and the telescope was released for observations from January 1, 2000. A detailed technical manual incorporating all relevant drawings, cabling details, modifications/changes has been prepared.
  • Optical Imager for the 2-m Telescope: A CCD cryostat for the optical imager for the Hanle 2-meter telescope has been developed in-house and tested for its performance in all respects.
  • A New High-Speed Link to Hanle : A new communication system ha's been procured from TIW, U.S.A., for establishing high speed (up to 2 MBPS) link between Hanle and Hoskote. This point-point link is intended for the remote operation of the 2-meter telescope at Hanle. The system has been installed and tested at both Hoskote and Hanle.
  • Dome Automation Software for the 2-m Telescope: In connection with the dome automation work, the various units like encoders, motors, inverter, converter and some i/o cards have been procured and tested in the lab. A 64 turn, 16 bit absolute position encoder from BEI Motion Control and System, USA, is used for dome position encoding. A circuit to test the encoder has been developed. Software routines have been developed to test the converter and all inverter functions from a PC. A test setup was made in the lab to carry out an integrated test on the inverter, motor and the encoder. The complete control algorithm was written in C language under DOS and tested.
  • Computer Centre - Installation of Sun Ultraspare Systems: A new set of eight Ultrasparc systems were installed in the computer centre to facilitate image data analysis. These Systems have 330 MHz Ultra spare CPU with 128 MB RAM and 40 GB hard disk. These have been networked through a 12 port 3 COM switch. A directory structure with YP has been installed to facilitate simple management. Several IBM PC's have been added with LINUX software for general use.

Mechanical Engineering Division

In addition to regular maintenance work, the Mechanical Engineering Division of the Institute undertook major design, development, fabrication, and installation work mostly in connection with the development of various major facilities at IAO, Hanle. These include the work on the domes and buildings for the 50-cm and the 2-m telescopes, communications antannae at CREST, Hosakote and IAO, Hanle, the tower for monitoring microthermal variations in the atmosphere at Hanle, filter unit for the CCD imager for the 2-m telescope, etc.. In addition, design, development and fabrication works were undertaken for (i) an interface unit for the SILFID spectrograph for the VBO telescope, (ii) the mechanical mount for the antennae for the GPS at Kodaikanal, Hanle, Almorah, etc., (iii) the dewar for the CCD to be used in the Hanle telescopes, (iv) filter wheel assembly for the spectropolarimeter at the VBO, Kavalur, and so on.

Photonics Division

Major facilities development and instrumentation work done in the Photonics Division include (i) the completion of the grinding work of the primary mirror of the 40-inch telescope, (ii) completion of a new design concept of the optical head for the Long Trace Profilometer. (LTP) in connection with the optics for the Synchrotron Radiation Beam Line (SRBL) project, (iii) fabrication and polishing (to a mirror finish) of a set of thin copper and aluminum plates for the Torsion Balance apparatus for measuring possible new millimeter range Yukawa type force - an experiment on fundamental physics being done in the Institute, and so on.

Collaborative Activities with other Institutions

Major collaborative activities were started with the following Institutes:

  • University of Calicut, March 1999: Mutual cooperation in the common interests of teaching and research in Astronomy and related subjects.
  • Copenhagen University Astronomical Observatory, Denmark, April 1999: Collaboration in the fields of galactic and extragalactic astronomy, and as a specific step towards building and utilization of a low dispersion spectrograph called "Hanle Faint Object Spectrograph & Camera" (HFOSC).
  • MeDonnell Center for Space Sciences, Washington University, St. Louis, USA, June 1999, to collaborate in the field of astronomical transient phenomena, as a specific step towards cooperation on the installation and utilization of two 50-em aperture telescopes forming the Antipodal Transient Observatory.
  • Centre for 'Development of Advanced Computing (C-DAC), Bangalore, November 1999, to collaborate in the field of storing rare archival documents, viz., printed astronomy books, written manuscripts, old correspondence and photographs in a specific digitized format towards the goal of establishing a digital library.
  • Wadia Institute of Himalayan Geology (WIHG), Dehra Dun, December 1999, to foster cooperative researches in Geodynamics of Ladakh Himalayas; a GPS receiver and a broad band seismograph provided by the WIHG will be installed at the Indian Astronomical Observatory, Hanle.
  • ISRO Satellite Center, Bangalore, February 2000, for optical polishing at IIA of the sun- shield panels of the INSAT-3D spacecraft imager and sounder.
  • Steward Observatory, Univ. of Arizona, Tucson, USA : March 2000, to develop astronomy from the high altitude site at Hanle, Ladakh. The principal goal of this collaboration is to build a large telescope, of order 6.5 to 8.4 meter aperture at Hanle.

Indian Institute of Geomagnetism, Mumbai


  • to promote, guide and conduct research in all branches of Geomagentism
  • to establish and maintain in the country, suitably located geomagnetic
  • to establish, maintain and manage laboratories, workshops and/or other units to
    assist scientific research in Geomagnetism.
  • to record, collect, scrutinize, process, publish and supply geomagentic data.
  • to undertake the design, development, construction calibration and standardization
    of magnetic instruments.
  • to organize training facilities and to train the staff of the Institute and other
    interested organizations in geomagentic work and arrange lectures, seminars and
    symposia in pursuance of the academic work of the Institute and for diffusion of
    scientific knowledge.
  • to invite Scientists from India and abroad who are actively engaged in research in
    geomagnetism, to deliver lectures and participate in the research activities of the
  • To institute and award fellowships, scholarships, prizes and medals.
  • To cooperate and collaborate with other National and/or foreign institutions and
    international organizations in the field of Geomagentism.
  • To publish scientific papers, bulletins and journals.
  • To disseminate information on matters concerning geomagnetism


The Indian Institute of Geomagnetism (IIG) is a premier research organization under the Department of Science and Technology devoted to the study of Geomagnetism from all possible point of views. Modern Geomagnetism is truly multidisciplinary science encompassing various disciplines like geophysics, fluid dynamics, space plasma physics, applied mathematics, aeronomy and atmospheric sciences etc. The study of Geomagnetism at longest time scales is relevant to understand the origin of planetary magnetism. The short-term geomagnetic variability, on the other hand, has found several important applications related to Sun-Earth connection as well as for geophysical prospecting, earthquake precursor mechanisms, satellite communication and for space weather forecasting. With new technological breakthroughs for accurate geomagnetic field measurements on ground and in space and the advent of modern computers, it is now possible to monitor even weak magnetic and electromagnetic precursory signals in the earthquake prone region. State of the art instrumentation like digital magnetometers and long period magnetotelluric units have been acquired to study the complex physical problems related to space weather and precursory signals.

The Research activities of the Institute are divided into three areas:

1. Observatory and Data Analysis
2. Upper Atmospheric Sciences
3. Solid Earth Geomagnetism

Activities during the year

The Honorable Minister for Science and Technology Prof. Murli Manohar Joshi on May 21, 1999 laid down foundation stone for the Geomagnetic Research Laboratory (GRL), Allahabad, a proposed regional center of the Institute for advanced research on Solid Earth Geomagnetism. Prof. V. S. Ramamurthy, Secretary, Department of Science & Technology, Dr. D. N. Tiwari, Member Planning Commission and several other dignitaries together with members from IIG, DST, Mehta Research Institute and Allahabad University attended the function. The activities of the GRL, Allahabad will include techniques of magnetovariational and magnetotelluric methods for imaging the deeper structures of the Himalayan and Indo-Gangetic Plains. Geomagnetic and geoelectrical precursors can provide vital input to the earthquake prediction studies. Other facilities planned at GRL, Allahabad are establishment of laboratories for Paleomagnetic and magnetic Petrology (rock studies) and some experiments for the Upper Atmospheric Studies.

Continuous recording of the ground magnetic measurements are carried out at permanent magnetic observatories, Tirunelveli, Pondicherry, Alibag, Ujjain, Nagpur, Visakhapatnam, Shillong, Gulmarg, Silchar, and a semi-permanent magnetic observatory at Maitri, in Antarctica. Magnetic Observatory at Trivandrum, established in the year 1957 in the campus of Kerala University, was closed down on 30 October 1999. Under a newly initiated Geomagnetic Activity Forecasting Program, one state of the art digital magnetometer has been installed at Tirunelveli Magnetic Observatory. The data from this magnetometer would be received at Colaba, HQ in near real time and will be used for geomagnetic data based research and predicting geomagnetic activity, especially from low latitudes.

The short-term variability in the geomagnetic field during the total solar eclipse of August 11,1999 was studied using the magnetic observatory chain operated by IIG and the special observations taken at Akola and Baroda in the path of totality. The gradient of the field was found to be different in pre-totality and post-totality times. Such types of gradients were not observed at the same time on controlled days.

A few sudden commencement great geomagnetic storms recorded during the solar cycle 22 were studied by analyzing magnetic records from selected low latitude Indian stations. Strong daytime equatorial enhancement in intensity of the geomagnetic Pc5-6 pulsation during several magnetic storms was observed from an array of 5 Indian stations. Solar flare effect has been studied by analyzing the magnetic data of Indo- USSR chain of magnetic observatories extending from magnetic equator to pole.

The Institute participated in the summer and winter expeditions to Antarctica. Data of three fluxgate magnetometers operating simultaneously at Maitri, Dakshin Gangotri and Orvin Mountains in Antarctica were analyzed for the magnetic pulsation with periods between 30 sec and 3000 sec. Pulsations during disturbed conditions are interpreted in terms of the mobile auroral current systems that drift over the stations. A Fluxgate magnetometer and a Riometer recording the 30 MHz cosmic radio noise were simultaneously operated at Maitri to study the characteristics of ionospheric absorption caused by magnetosphere-ionosphere particle precipitation.

The Equatorial Geophysical Research Laboratory (EGRL) at Tirunelveli made good progress during the year. The partial reflection (PR) drifts at 98 km measured by the medium frequency (MF) radar are shown to have the combined effects of mesospheric winds and the equatorial electrojet. Observations of mesospheric winds in the altitude region 84-98 km with the PR radar at Tirunelveli and the ground-based geomagnetic data from the low latitude Indian sector have been used to identify the signatures of the quasi-2-day (QTD) planetary waves in the equatorial electrojet (EEJ). It is found that there is a reasonable correlation between occurrence times of the quasi-2-day oscillation in the EEJ strength and the mesospheric winds.

Amplitude scintillation on 250 MHz radio signals recorded at a network of stations in the Indian sector during the last five years have been analyzed to study the characteristic features of ionospheric irregularities. Scintillations recorded on the 250 MHz radio beacon at Mumbai and Pondicherry were analyzed to look for the possibility of field line resonances at equatorial latitudes. Dual frequency data for fluctuations in the total electron content ( TEC ) along the path of GPS signals to the equatorial station Ancon ( 1.5O dip), sampled at a rate of 1 Hz, has been used to separate this contribution from the slower TEC variations. A theoretical model, using the transmission line analogy, has been developed to investigate the coupling between the E and F regions through field-aligned currents (FACs).

An all-sky imager with 180o field of view has been operating at Kolhapur to study the ionosphere-thermosphere dynamics through imaging of 630.0 nm oxygen emission line. A large number of equatorial ionospheric plasma bubbles or depletions are characterized by the development of strong equatoriaI ionization anomaly. Analysis of the airglow data obtained during the ISTEP-II campaign period of March 12-21 and April 10-22, 1999, showed north-south aligned intensity depletions, which are the optical signature of large scale ionospheric F-region plasma bubbles, on most of the nights.

A fully electromagnetic linear theory for the generation of broadband plasma waves observed in the low latitude boundary layer by POLAR has been developed. It is shown that electron acoustic wave instability can offer a possible generation mechanism for the broadband electrostatic noise (BEN) observed in auroral acceleration region, plasma sheet boundary layer, and polar cusp region. A theoretical model for the large amplitude electrostatic ion - cyclotron modes in an auroral beam - plasma system is developed. The numerical solutions of the non-linear evolution equation could reproduce several essential features of the observed waveform by FAST and POLAR satellite.

A direct mechanism for the generation of waves in the intermediate frequencies between the water-group and the proton gyrofrequencies in cometary environments is suggested in an unstable wavelength band when the solar wind is sufficiently mass-loaded by cometary material. The mirror mode structures at comet Giacobini-Zinner are detected in a region just adjacent to the magnetic tail, and they have scale sizes of ~ 12 H2O group ion cyclotron radii. It is shown that nonlinear evolution of Alfvén waves, propagating in streaming solar wind plasma with non-uniform densities and inhomogeneous magnetic fields, is governed by the modified derivative nonlinear Schrödinger (MDNLS) equation.

Analysis of Ulysses magnetometer data revealed the presence of magnetic field decreases (MDs) over the heliospheric polar regions. The MDs have minimum spatial scale sizes of 25 proton thermal gyroradii, and are typically bounded by tangential or rotational discontinuities. Charged particle interactions with the MDs can lead to particle guiding center displacements and hence particle cross-field diffusion.

The resistive hydromagnetic equations are solved numerically in a two dimensional box to simulate the dynamics of geomagnetic tail during substorm events by applying the Flux Corrected Transport ( FCT ) code. Three different widths for the initial current sheet are investigated. For wider current sheet the reconnection starts later than the case of narrower current layer. It is found that pre-substorm earthward flows deduced from satellite data could be explained by the wider current sheet case.

The deep electrical structure beneath the Vindhyan basin and Deccan Volcanic province has been studied over the Damoh - Jabalpur - Mandla - Anjaneya region using the magnetotelluric techniques. These studies have delineated about 5 km thick Vindhyan sediments in the Damoh- Katangi region. A prism shaped conductive feature is observed between Jabalpur and Mandla, intruding into the upper crust from the mid crustal depths. This feature coincides with the gravity high and heat flow high in this region.

The geomagnetic induction response functions, deduced from the number of geomagnetic deep sounding experiments in the frontal Himalaya and contiguous Indian shield, have been used to map geoelectrical structures of the Frontal Himalayas. The anomalous induction features have shown presence of an elongated conductive structure embedded in high seismicity zone emerging out of the Himalayas. The nature of electrical conductivity distribution along a profile extending from the Indian shield to higher Himalayas shows evidence of a mid-crustal conductor beneath the Indo-Gangetic Plains. Beneath the frontal Himalayas, top surface of the mid-crustal conductor correlates with a plane defined by hypocenters of moderate earthquakes. It also defines the cut-off depth of crustal micro-seismicity.

A magnetometer array study was undertaken within and around the intracratonic Parnai'ba Basin, north-northeast Brazil. The analysis of various frequency and polarization parameters indicates that anomalous behavior of the magnetovariational fields, with periods longer than one hour is determined by currents induced in the seawater and perhaps in the raised asthenosphere beneath the oceanic region.

Ground magnetic surveys were conducted over the Cuddapah basin, Chitradurga basin and Krishna-Godavari basin with data being collected at every 10 km interval. Anomaly maps have been prepared for both total field and vertical field after correcting for IGRF and normal variations. The Eastern Ghat folding and the thrust zone are clearly evident on the anomaly maps of the Cuddapah basin.

Core samples from the Mansar Lake, Jammu, Navlakhi mudflat, Saurashtra were analysed for magnetic mineralogy determinations with an objective to decipher the past precipitation changes, and for ascertaining the potential link between the deep sea oceanographic framework and the less understood sequences of the land.

A 73 site GPS geodetic network has been established to estimate the crustal deformation strain field in the earthquake prone region of Western Maharashtra in Peninsular India. Repeat GPS surveys were done and the data have been collected at each site. GPS survey in the Chamoli earthquake region was carried out in collaboration with NGRI. The data is being analyzed using the latest post-processing software and IGS precise ephemeredes.

The Instrumentation Laboratory developed various instruments that are used in the Observatories as well as in surveys. A Data logger has been interfaced to the existing model of 1 nT PPM to make it a portable magnetometer suitable for surveys. Work on two models of 0.1nT PPM is nearly complete. Fabrication of a Fluxgate Magnetometer using a small sized, high sensitivity sensor is at advanced stage.

Indian Institute of Tropical Meteorology, Pune

The Indian Institute of Tropical Meteorology functions as a National Centre for basic and applied research in Tropical Meteorology. Its primary functions are to promote, guide and conduct research in the field of Meteorology and Atmospheric Sciences in all its aspects with special reference to the tropics and sub-tropics.

The Institute has developed infrastructural facilities like buildings, specialised and sophisticated data acquisition and storage systems, modern laboratory equipment, latest computers and a well equipped library to facilitate the research work of the scientists. The computational facilities of the Institute include the ND-560/CX, the RISC based HP-9000/735 Workstation, the Power Challenge XL Super Computer of the Silicon Graphics Inc., USA, two Indy Graphics Workstations and the Secondary Data Utilization Centre (SDUC) for receiving cloud imageries and meteorological data, all along-with latest accessories and system softwares. An INTERNET launched through the VSAT has been provided to all the divisions through the local area network. A web page for the Institute has been established on the INTERNET. The Data Bank available with the Institute would be made available in the web page.

The Institute organises man power development programmes by arranging specialised training programmes in different areas of atmospheric sciences. Several distinguished scientists from India and abroad visit the Institute and have useful discussions with the scientists of the Institute. Scientists of the Institute are also deputed abroad for training and participation in the international seminars, symposia and collaborative research programmes. The Institute promotes scientific collaborations with the universities and other research organisations.

The Institute collaborates in the national and international collaborative research programmes, and also arranges field experiments of its own and through participation in the multi-agency missions.

The Institute has several projects on hand and also plans for the future, to address the need. The Institute continues to play an important role in the activities of Inter Governmental Panel on Climate Change (ICRP), International Geosphere Biosphere Programme (IGBP) and Indian Climate Research Programme (ICRP) to ensure national and international co-ordinates of the relevant research programme.

The Institute has made considerable progress in Science and Technology in the field of Meteorology and Atmospheric Sciences. The highlights of the progress made during the year are summarised below:

Technology Development Projects:

Input for Monsoon Forecast

Forecasts for Monsoon -2000 were prepared based on statistical methods and communicated to the Director General of Meteorology, India Meteorological Department, New Delhi. The predicted monsoon is in the positive side of the normal.

Long period rainfall series are vital in studies of climate variability and also useful for calibration and verification of palaeoclimatic reconstructions. Based on the longest available instrumental records, the summer monsoon, post-monsoon and annual rainfall series have been prepared for Northwest India, North Central India, Northeast India, West Peninsular India, East Peninsular India, South Peninsular India and relatively-plain-and-contiguous India (combined area of the stated six zones). Rainfall series of each of the four seasons and the annual total of the North Mountainous India (NMI) (combined area of Hills of Uttar Pradesh, Himachal Pradesh and Jammu and Kashmir) have also been prepared. Some of the series extend back to 1813, and all are updated up to 1997.

For the purpose of extrapolating the decadal variability into the future, the low frequency smoothed series up to 1997 plus the series 1998-2007, filled with long term mean was subjected to the Variable Harmonic Analysis (VHA). An objective technique was applied to select a few harmonics whose linear combination showed a Correlation coefficient (CC) of -0.85 with the smooth series. The generated rainfall amount from the selected harmonics would be the prediction for the period 1998-2007. Presently the study provides a tentative inference that the rainfall fluctuation across the country is likely to be around the long-term mean over the next 10-year period.

Using 85-year rainfall data for all-stations in the Krishna basin and its neighbourhood estimates of maximum 1-day rainfall for different return periods of 2 to 100 years were made by Gumbel's statistical method. With the help of these data 2 and 1000 year generalized rainfall chart for 1-day duration, a frequency interpolation nomogram has been prepared. Maximum 1-day rainfall obtained by this nomogram method for different return periods have been found to agree within limits of ± 4% of the computed values obtained by the Gumbel's technique.

Estimates of maximum 1-day rainfall for all having long records of rainfall data stations in West Bengal have been made by using Hershfield's (1961) statistical techniques for 2 to 100 years return periods. It is seen that estimates of 1-day maximum rainfall for stations in the region vary from about 13.8 to 35.3 cm for 10-year return period while for 100 year these values range from 19.7 to 49.3 cm.

Capabilities of various features of scientific computing under FORTRAN-90 environment were studied and analysed for their computational merits and demerits. This study was made for the use of FORTRAN-90 in developing modular meteorological application software tools. FORTRAN-90 is extremely modular and has good features of other contemporary languages like - Pointers, Recursion, Functions Returning Arrays. Allocated Scalars and Arrays. Allocated objects, users Defined Data Types (structures in FORTRAN-90), Precision based memory allocation, optional Arguments etc. FORTRAN-90 does not support features like Exception Handling and Genesic software tools. In spite of its inherent weaknesses FORTRAN-90 can be effectively used in developing high quality modular scientific/meteorological software. C++ environment on UNIX platform was further explored by using Component Object Modelling (COM). COM studies are based on UNIX Standard Laboratories standard C++ Components available on HP workstation.

Field Mills and Gerdien apparatus were fabricated in the Institute for the research work to be carried out on Global Electric Circuit under the IIG/DST project. An experiment to study the evaporation of water drops in vertical electric field was being conducted. Different types of electrodes were fabricated and tested for suspension of water drops in the vertical electric field in a vertical wind tunnel.

Distortion of water drops suspended in a small vertical wind tunnel was studied by taking photographs with a 16-mm movie camera. The data were analyzed to study the effect of horizontal electric field on the distortion of drops. Results showed that the deformation of the drop increases with the size of the drop and also with the increase in electric fields.

A dispersion unit and a pre-air filter unit to get proper air supply from the compressor were fabricated for the study of the process of collision/coalescence of water drops.

Basic Research Projects

Several global and regional predictors have been identified and regression equations have been developed for seasonal forecasting of all India monsoon rainfall. Studies have also been carried out to examine the relationship between the monsoon rainfall activity and meteorological factors such as El Nino, La Nina, ENSO, NAO, NPO, temperature and pressure anomalies, planetary waves etc.

Study of the dynamic instability characteristics of synoptic scale, waves embedded in the combined zonal and meridional flow prior to the onset phase of the south west monsoon study helped to understand the occurrence of transient disturbance which leads to the onset of the south west monsoon.

Interactive mechanism between ENSO and North Atlantic Oscillation (NAO) and its relationship with Indian summer monsoon variability, was explored by using 107 years data (1881-1987). The analysis was carried out on monthly, seasonal and annual time scale. From the analysis it is seen that there was an inverse relationship between NAO and SO significant at 1% level. From the analysis it was also found that these two oscillations behave in the opposite phase before the onset of Indian Summer monsoon. Once the monsoon sets, the relationship suddenly reverses. Behaviour of these two oscillations were monitored during the contrasting monsoon years (i.e. Drought, good and normal monsoon years). The study revealed that during the drought years these two oscillations are not in a proper phase while in the good and normal monsoon, these oscillations are in the proper phase.

To understand the role of global atmospheric thermal conditions on the occurrence and variability of the southwest and northeast monsoons of India, correlation of zonal, hemispheric as well as upper air temperatures with the all-India southwest and northeast monsoon rainfall was examined. Based on a well spread network of 63 radiosonde stations surface air and thickness-derived upper air temperature anomaly (troposphere 850-300 hPa, tropopause 300-100 hPa and surface-100 hPa series (1958-1996) were prepared for different zones, the hemisphere and the globe.

A detailed analysis was made of the simulated impact of greenhouse gas (GHG) warming on the characteristics of ENSO and Monsoon rainfall over India and their relationship. Monsoon rainfall over Indian land grids and the autumn (September-November) surface temperature over Nino-3 region were used for the analysis. The impact of transient GHG forcing was compared with the results of control (CTL) simulation which has a fixed greenhouse gas forcing representing 1990. The results of this study suggested that both monsoon rainfall and the Nino-3 temperatures show strong increasing trends into the future, indicating increase in mean characteristics as well as in the variability. Although there are changes in the statistical characteristics of simulated ENSO and the Indian monsoon rainfall, the interannual correlations between the two are robust throughout the 240 year simulation in both CTL and GHG simulations. Further, the GHG simulation shows an increase in the mean monsoon rainfall despite a change towards a warmer mean state of ENSO in Niño-3 region. The GHG simulation suggested decrease in the impact of El Niño events on monsoon as the greenhouse gas concentrations are increased, while the impact of La Niña on monsoon remains largely unchanged despite a skewness towards strong and more frequent La Niña events in the simulation.

In the absence of tropical disturbances like depressions and cyclonic storms during monsoon season low pressure areas (LPA) under favourable meteorological conditions can cause normal or even above normal rainfall over north Indian plains, central India and northern half of the Indian Peninsula. LPAs having sea origin cause more rainfall than those which originate from land. It was also observed that LPAs having longer life spans and traversing the country from east to west cause well distributed rainfall. Well marked LPAs moving one after another in quick succession, cause a continuous spell of rain which resulted in the flooding of rivers in the regions over which they pass.

The role of baroclinic and barotropic components of the atmospheric flow in the global energetics was examined. The daily TOGA global grid point analyses of u and v on 14 standard pressure surfaces during July 1991 were utilised. Global energetics of the aforesaid components over the troposphere and stratosphere were computed. Triangular truncation at wavenumber 30 was used for computations. From the vertical profile of KZ 700 hPa may be considered as the approximate global average barotropic level during the northern hemisphere summer. Further, the vertical profiles of KE indicated that the global baroclinic perturbation flow is stronger than the total flow throughout the vertical region between 1000 to 10 hPa. This confirms that the global atmosphere is baroclinic throughout the vertical region between 1000 to 10 hPa.

Markov chain models of first, second and third order have been used to provide a probabilistic description of thunderstorm phenomenon in the pre-monsoon season (March-June) over Pune. The data of thunderstorms occurred over Pune during 11 year period i.e. 1970-1980 have been used for this purpose. The results reveal that the Markov chain of the first order, perhaps, is the best model that describes the thunderstorm phenomenon, over Pune region.

Technologies Transferred/Commercialized :

Special observations of atmospheric aerosols using the Argon ion lidar and radiometric techniques were carried out at the IITM and at the Mulshi dam sites on 6,20 January, 3, 13 February, 2,8 Marc, 1,18,25 April, 3, 19 May 2000 and also at the Khadadwasla dam site on 1,4,10,30 January, 18, 24 February, 13, 20 March, 6,14,30 April, 9,24 May 2000 in synchronization with overpasses of ISRO's IRS-P3/P4/INSAT-IC/ID polar orbiting satellite over Pune.

A pilot study to examine the levels of various aerosol and gaseous pollutants prevailing at different traffic junctions using direct and remote sensing instruments has been undertaken for the first time in the Pune city. Under this programme, special observations of total column and surface ozone, aerosol, water vapour, total suspended particulate, aitken nuclei, wind, temperature, humidity and traffic density were carried out at five prominent traffic junctions during 1-5 May 2000.

As requested by the authorities of the Utkal Alumina Project the following analyses were carried by using the rainfall data of the five hearby observatory stations, for the period 1968-1997:

Estimation of statistical parameters such as mean and standard deviation on different time scales like daily, monthly seasonal and annual,

Estimation of rainfall intensities of different durations viz., 12-hr, 24-hr, 48-hr and 72-hr for different return periods

Technology Demonstration Projects undertaken in the area of Socio-economic Development:

Special field programmes to collect observations of atmospheric aerosols, trace gases, ozone and water vapour over Kullu and Kothi, and at New Delhi were organised in the Himalayan region in collaboration with G.B.Pant Institute of Himalayan Environment and Development, Shamshi, Himachal Pradesh during 18 May-7 June and at New Delhi during 2-5 June 2000 respectively.

A state-of-art atmospheric chemistry model which treats radiation, dynamics and chemistry interactivity was developed for the entire altitude range from surface to 120 km, specifically to study the relative importance of natural and human activities on atmospheric composition and thermal structure of this region. The changes arising from variations in solar activity and human activities on atmospheric composition and thermal structure of the middle atmosphere, especially in the ion composition, were accessed using this model. These results revealed that the changes from anthropogenic activities are less in magnitude but permanent in nature and changes due to variations in the solar activity are comparatively higher but periodic.

The impact of anthropogenic activities during the Dussera festival 1999 on the physical and chemical characteristics of aerosols was studied. The aerosol observations carried out at Kullu, H.P. before, during and after the festival have been used for the study. The results indicated that (i) the average concentration of Total Suspended Particulates (TSP) during the Dussera period (360 (g / m3) was about three times higher than that during the period before and after the festival (118 (g / m3) and (ii) the ionic components of water soluble (Cl, SO4, NO3, NH4, Na, K, Ca and Mg) and acid soluble (Fe, Al, Cu, Zn and Mn), were found to be higher (About 2-5 times) during the Dussera festival period. Thus the study revealed increased pollution levels during the Dussera festival which are attributed mainly to increase in fuel burning and vehicular traffic and burning of fire crackers.

Using 14-year flood data of 1986 to 1999 the frequency of floods of G/D sites of Indian rivers have been examined which have experienced 50 floods during the period. It is seen that such high frequency floods have occurred in northeast and north Indian rivers. Thus frequency of floods varied from 150 to 177 in the 14-yr period. The magnitude of floods at different sites varied from 5m to 18m above their respective danger level (D.L.).

Research Highlights :

The Institute has made significant contributions in the challenging areas of Atmospheric Sciences like Weather Forecasting, Climatology, Hydrometeorology, Monsoon Studies, Climate Modelling, Weather Modification, Cloud Physics, Atmospheric Chemistry, Atmospheric Electricity and studies relating to Land-Surface processes. The important highlights are summarised below:

NWP Modeling and Model Diagnostics

Numerical experiments were performed to see the sensitivity of the cyclone tracks to the merging of only mass fields (pressure and temperature) and wind field of the artificial vortex. Results showed that merging of wind improved the cyclone track.

The response of surface sensible heat flux to total cloud cover and daily rainfall was studied using MONTBLEX (Monsoon Trough Boundary Layer Experiment) observations of 1989 and 1990 at two stations, Jodhpur in the western end sector of monsoon trough and Kharagpur in the eastern sector. The transition hours just after sunrise and around sunset have shown quick response in altering or modifying the surface fluxes. A general inverse relationship between total cloud cover and surface-sensible heat-flux at these hours is well established. The surface sensible heat fluxes respond to soil wetness at these locations in association with rainfall due to low-pressure systems.

Objective Analysis including satellite input for NWP Models

Objective analysis of monthly rainfall for the month of August 1972 has been carried out. The experimental Cumulative Semi Variogram weights have been computed on the basis of 20 years of monthly rainfall data (August 1971 - August 1990). Due to high spatial variability and non-normal distribution of rainfall, cubic roots of rainfall was considered for necessary computation and analysis.

Extended Range Prediction

The correlation analysis of cyclonic storms over North Indian Ocean, with the north Atlantic Oscillation (NAO) and Southern Oscillation (SO) has been carried out separately. The analysis has been carried out for 100 years (1891-1990) data. From the analysis it is noticed that frequency of cyclonic storms over Indian ocean shows a statistically significant negative relationship with NAO (significant at 1% level). It means that, during the weak phase of NAO (i.e. in low index phase epoch) the frequency of cyclonic storms over north Indian Ocean is likely to be more than normal and vice versa. The analysis of the frequency of cyclonic storms with SO reveals a positive relationship which is significant at 1% level. The analysis also reveals that during the ENSO epoch the frequency of cyclonic storms is less than normal over north Indian ocean and vice versa.

Monsoon Studies and Forecasting

Analysis of monthly momentum transport of zonal waves at 850 hPa for 1979 to 1993, between 30°S and 30°N for January to April, using zonal (u) and meridional (v) components of wind taken from the ECMWF reanalysis field, showed a positive correlation (0.1% level of significance) between Indian summer monsoon rainfall (June through September) and the momentum transport of wave zero over latitudinal belt between 25°S and 5°N during March. Northward (Southward) momentum transport of wave zero observed in March over the belt subsequently leads to a good (drought) monsoon season over India which is found to be true even when the year is marked with El Nino event. The zone of westerlies in March over the Indian Ocean affects the momentum transport of wave zero over the belt and also influences the monsoon circulation (rainfall activity) during June to September, over Indian region, through its annual meridional oscillation.

Sensitivity experiments on ENSO-Monsoon relationship

A set of atmospheric general circulation model (AGCM) experiments were conducted forcing ECHAM3 (T21) model with different sea surface temperature (SST) patterns in the Indian and the Pacific Oceans to understand various issues concerning the secular changes in monsoon-ENSO relationships. The possible impact of recent continental warming on the connection between the Indian monsoon activity and the SSTs in the Indo-Pacific region is also assessed with additional sensitivity experiments by doubling the CO2 concentration with fixed SST patterns in the Ocean. The sensitivity experiments suggest significant differences in the response of Indian summer monsoon to the differences in the SST patterns associated with different ENSO events. The Indian Ocean SSTs generally have much less impact on the monsoon variability compared to the Pacific Ocean. Also, the impact of ENSO on the Indian monsoon is found to be much less in presence of strong continental warming, suggesting that the enhanced land-sea gradient and an enhanced monsoon due to general warming could counter the negative impacts of El Niño on the monsoon to a large extent and thereby weakening the connection between these two important global climate phenomena.

Dendroclimatological Studies

Comparative studies of western Himalayan and Nepal tree-ring chronologies have been carried out to look for common climatic information on low frequency scale responsible for tree-growth. Principal component analysis of these chronologies indicates that 1st components of western Himalayan and western Nepal chronologies are highly correlated. However 3rd components of central and eastern Nepal show good correlations with the 1st component of western Himalayan chronologies. This implies that wide network of Himalayan tree-ring chronologies including Indian Himalaya and Nepal Himalaya represents spatially extensive common variations which may be due to large scale climate anomalies.

Preliminary tree-ring analysis of teak (Tectron grandis) from Allapalli forest division of Chandrapur District. Central India indicates high dendroclimatic potential of the species. Analysis of about 46 tree cores shows high common variance, mean sensitivity and signal to noise ratio which implies the usefulness of the species for dendroclimatic studies. In response function analysis, a significant negative relationship was found between ringwidth parameters (total ring width and latewood width) and mean temperature in November of previous year. The significant relationship between chronologies and monthly total precipitation was observed only in previous and current October (beginning of dry season).

Hydrometeorological Studies

Among the 12 major tributaries of the Brahmaputra river in Assam, Puthimari river has recorded the highest deviation of 4.65 m above its danger level in June 1993. The two gauge / discharge (G/D) sites at Dibrugarh and Nematighat in upper Assam have been experiencing high flood levels year after year. Maximum flood frequency at those G/D sites was of the order of 112 to 136 during the period 1987 to 1998. It is seen from this study that though there is not much scope for increasing irrigation facilities beyond a certain limit, there is enormous potential for hydropower generation, especially near the 'great bund' where the river enters India from Tibet.

Using the available precipitation data of about 5 stations around the peaks of Mt. Everest and Kanchenjunga in the Himalayas, since 1949 to present times, it has been seen that Kanchenjunga receives fairly greater precipitation than Mt. Everest. Perhaps because of this, there are 4 major glaciers around Kanchenjunga as compared to only 2 around Mt. Everest.

Barotropic and Baroclinic Instability of the Atmospheric Flow

Dynamic instability characteristics of synoptic scale waves embedded in the combined zonal and meridional flow prior to the onset phase of south west monsoon 1997 were investigated using quasi-geostrophic multi-level numerical model. Basic state for this study was considered as time averaged wind and temperature fields from NCEP reanalysis from surface to 200 hPa over the region EQ. - 25ºN and 50-80ºE for the period 20-31 May 1997, with the consideration that mean onset date is 1st June. Since during 1997, the monsoon arrived at Kerala coast on 9 June, one more case of basic state averaged over the period 1-8 June 1997 was also tested for instability characteristics. Growth rate spectrum for short wave synoptic scale band (1000 - 3000 km) was obtained for both the cases of basic state averaged over the period as well as viscous flow by taking into account Ekman surface friction. It was found that the preferred wavelength has e-folding time less than 10 days when the basic state is considered for the period 1-8 June. Hence it is concluded that the study is helpful to understand the occurrence of transient disturbance which leads to the onset of south west monsoon.

Simulation of Mean Monsoon Circulation and Predictabilitiy of the Monsoon Systems

In the detailed study of upper ocean response to asymmetric cyclone, different sensitivity experiments were performed by changing magnitude of asymmetry, intensity of the cyclonic storm moving in different directions and with different directions of asymmetry. It was found that the value of 30 % asymmetry on left of the northwest track, to give symmetric ULTD field, remains invariant for different cyclone intensities. Also, it is seen that for westward moving cyclones, 30 % asymmetry on the right of the cyclone is necessary to produce right bias in the ULTD field, which is absent for symmetric vortex. This magnitude of asymmetry is again independent of the cyclone intensities. In this study the model domain is 24ºS - 23ºN and 35º - 115º E.

Climate and Global Modelling

The grid point model used for the simulation is the UKMO Unified Model Version HadAM2b. It has an horizontal resolution of 2.5 lat x 3.75 long. and 19 vertical levels.

Six member ensemble integrations were made. The initial conditions are from the model dumps corresponding to 1st April of the last six years of a 17-year integration forced with climatological SSTs over global oceans. Each member of the ensemble was integrated from 1st April to 30th September. For the integrations, SST anomalies of April 2000 were superposed on the climatological SST of the month May to September. The SST data used are Optimum Interpolated (OI) SST.

The ensemble mean JJAS rainfall over Indian land area shows a departure of +7.2% above the model climatology based on a 17 year integration. However, the model indicates a strong monsoon in June and normal rainfall in July and August and above average rainfall in September. The skill with persisted SST anomalies of April month is limited. Recently carried out studies indicated that the May SST anomalies give a better forecast. Also the model has some systematic errors by which the response to SST forcing in the second half of the monsoon season is opposite to that in the first half.

Cloud Physics and Weather Modification

The association between duration and amplitude variation of Point Discharge Current (PDC) of both the polarities (+ve and -ve) was examined by analysing the data of PDC of a total of 65 thunderstorms at Pune. The result of the study suggested that the variation of current of both the polarities is quite similar but the amplitude of negative PDC is systematically larger (0.8 to 1.4(A) than that of the positive one (0.35 to 0.50(A). Further, it was also noted that the amplitude of -ve current existing for greater than 60 minutes or more is larger than that of +ve current in the range 1.4 to 2.0 times, while the amplitudes corresponding to less than 60 minute duration are quite comparable to each other. This result is consistent wit

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