11 December, 2014


Georg Simon Ohm 




Born :     16 March 1789 ErlangenBrandenburg-Bayreuth

Died :      6 July 1854 MunichKingdom of Bavaria

Nationality :   German

Fields :     Physics

Known for :      Ohm's law
                          Ohm's Phase law
                          Ohm's acoustic law

Notable awards :    Copley Medal (1841)

Georg Simon Ohm (16 March 1789 – 6 July 1854) was a German physicist and mathematician. As a school teacher, Ohm began his research with the new electrochemical cell, invented by Italian scientist Alessandro Volta. Using equipment of his own creation, Ohm found that there is a direct proportionality between the potential difference (voltage) applied across a conductor and the resultant electric current. This relationship is known as Ohm's law.

Early years
Georg Simon Ohm was born into a Protestant family in ErlangenBrandenburg-Bayreuth (then a part of the Holy Roman Empire), son to Johann Wolfgang Ohm, a locksmith and Maria Elizabeth Beck, the daughter of a tailor in Erlangen. Although his parents had not been formally educated, Ohm's father was a respected man who had educated himself to a high level and was able to give his sons an excellent education through his own teachings. Of the seven children of the family only three survived to adulthood: Georg Simon, his younger brother Martin, who later became a well-known mathematician, and his sister Elizabeth Barbara. His mother died when he was ten.
From early childhood, Georg and Martin were taught by their father who brought them to a high standard in mathematicsphysics,chemistry and philosophy. Georg Simon attended Erlangen Gymnasium from age eleven to fifteen where he received little in the area of scientific training, which sharply contrasted with the inspired instruction that both Georg and Martin received from their father. This characteristic made the Ohms bear a resemblance to the Bernoulli family, as noted by Karl Christian von Langsdorf, a professor at the University of Erlangen.

Teaching career
Ohm's own studies prepared him for his doctorate which he received from the University of Erlangen on October 25, 1811. He immediately joined the faculty there as a lecturer in mathematics but left after three semesters because of unpromising prospects. He could not survive on his salary as a lecturer. The Bavarian government offered him a post as a teacher of mathematics and physics at a poor quality school in Bamberg which Ohm accepted in January 1813. Unhappy with his job, Georg began writing an elementary textbook on geometry as a way to prove his abilities. Ohm's school was closed down in February 1816. The Bavarian government then sent him to an overcrowded school in Bamberg to help out with the teaching of mathematics.

The discovery of Ohm’s law
Ohm's law first appeared in the famous book Die galvanische Kette, mathematisch bearbeitet (tr., The Galvanic Circuit Investigated Mathematically) (1827) in which he gave his complete theory of electricity.  In this work, he stated his law for electromotive force acting between the extremities of any part of a circuit is the product of the strength of the current, and the resistance of that part of the circuit.
The book begins with the mathematical background necessary for an understanding of the rest of the work. While his work greatly influenced the theory and applications of current electricity, it was coldly received at that time. It is interesting that Ohm presents his theory as one of contiguous action, a theory which opposed the concept of action at a distance. Ohm believed that the communication of electricity occurred between "contiguous particles" which is the term he himself used. The paper is concerned with this idea, and in particular with illustrating the differences in this scientific approach of Ohm's and the approaches of Joseph Fourier and Claude-Louis Navier.
A detailed study of the conceptual framework used by Ohm in producing Ohm's law has been presented by Archibald. The work of Ohm marked the early beginning of the subject of circuit theory, although this did not become an important field until the end of the century.

Ohm’s acoustic law
Ohm's acoustic law, sometimes called the acoustic phase law or simply Ohm's law, states that a musical sound is perceived by the ear as a set of a number of constituent pure harmonic tones. It is well known to be not quite true.



30 November, 2014

Alexander Graham Bell


              Alexander Graham Bell (March 3, 1847 – August 2, 1922)was an eminent Scottish-born scientist, inventor, engineer and innovator who is credited with inventing the first practical telephone.
              Bell's father, grandfather, and brother had all been associated with work on elocution and speech, and both his mother and wife were deaf, profoundly influencing Bell's life's work. His research on hearing and speech further led him to experiment with hearing devices which eventually culminated in Bell being awarded the first U.S. patent for the telephone in 1876. Many other inventions marked Bell's later life, including groundbreaking work in optical telecommunications, hydrofoils and aeronautics. In 1888, Bell became one of the founding members of the National Geographic Society.
   
Early Life
     Alexander Bell was born in Edinburgh, Scotland, on March 3, 1847 to a professor father and housewife mother.He had 2 brothers who later died of TB.
        As a child, young Alexander displayed a natural curiosity about his world, resulting in gathering botanical specimens as well as experimenting even at an early age. His best friend was Ben Herdman, a neighbor whose family operated a flour mill, the scene of many forays. Young Aleck asked what needed to be done at the mill. He was told wheat had to be dehusked through a laborious process and at the age of 12, Bell built a homemade device that combined rotating paddles with sets of nail brushes, creating a simple dehusking machine that was put into operation and used steadily for a number of years.
       Bell was also deeply affected by his mother's gradual deafness, (she began to lose her hearing when he was 12 years old) and learned a manual finger language so he could sit at her side and tap out silently the conversations swirling around the family parlour. He also developed a technique of speaking in clear, modulated tones directly into his mother's forehead wherein she would hear him with reasonable clarity. Bell's preoccupation with his mother's deafness led him to study acoustics.
          As a young child, Bell, like his brothers, received his early schooling at home from his father. At an early age, however, he was enrolled at the Royal High School, Edinburgh, Scotland, which he left at age 15, completing only the first four forms.His school record was undistinguished, marked by absenteeism and lacklustre grades.
Career     
 In 1870, at age 23, Bell, his brother's widow, Caroline (Margaret Ottaway), and his parents traveled on the SS Nestorian to Canada. After setting up his workshop, Bell continued experiments based on Helmholtz's work with electricity and sound.By 1874, Bell's initial work on the harmonic telegraph had entered a formative stage, with progress made both at his new Boston "laboratory" (a rented facility) and at his family home in Canada a big success.While working that summer in Brantford, Bell experimented with a "phonautograph", a pen-like machine that could draw shapes of sound waves on smoked glass by tracing their vibrations. Bell thought it might be possible to generate undulating electrical currents that corresponded to sound waves. Bell also thought that multiple metal reeds tuned to different frequencies like a harp would be able to convert the undulating currents back into sound. But he had no working model to demonstrate the feasibility of these ideas. In 1875, Bell developed an acoustic telegraph and drew up a patent application for it.
Breakthrough        
      Continuing his experiments in Brantford, Bell brought home a working model of his telephone. On August 3, 1876, from the telegraph office in Mount Pleasant five miles (eight km) away from Brantford, Bell sent a tentative telegram indicating that he was ready. With curious onlookers packed into the office as witnesses, faint voices were heard replying. The following night, he amazed guests as well as his family when a message was received at the Bell home from Brantford, four miles (six km) distant, along an improvised wire strung up along telegraph lines and fences, and laid through a tunnel. This time, guests at the household distinctly heard people in Brantford reading and singing. These experiments clearly proved that the telephone could work over long distances.
Awards  
     The bel (B) and the smaller decibel (dB) are units of measurement of sound intensity invented by Bell Labs and named after him. Since 1976 the IEEE's Alexander Graham Bell Medal has been awarded to honor outstanding contributions in the field of telecommunications. In 1936 the US Patent Office declared Bell first on its list of the country's greatest inventors, leading to the US Post Office issuing a commemorative stamp honoring Bell in 1940 as part of its 'Famous Americans Series'.     Alexander Graham Bell was ranked 57th among the 100 Greatest Britons (2002) in an official BBC nationwide poll, and among the Top Ten Greatest Canadians(2004), and the 100 Greatest Americans (2005). In 2006 Bell was also named as one of the 10 greatest Scottish scientists in history after having been listed in the National Library of Scotland's 'Scottish Science Hall of Fame' 
        This great scientist Bell died of complications arising from diabetes on August 2, 1922, at his private estate, BeinnBhreagh, Nova Scotia, at age 75.

27 November, 2014

Raj Reddy

 

 






















Born                        :  June 13 , 1937
                                   Andhra Pradesh 

Residence               :  United States
Nationality             :   Indian-American 

Fields                     :   Artificial Intelligence
                                   Robotics
                                   Human - Computer Interaction

Institutions             :   Carnegie Mellon University
                                   Stanford University
                                   Rajiv Gandhi University of Knowledge Technologies
                                   International Institute of Information Technology, Hyderabad

 Notable awards      :  Legion of Honor (1984)
                                  Turing Award (1994)
                                  Padma Bhushan (2001)
                                  Vannevar Bush Award (2006)               


Dabbala Rajagopal "Raj" Reddy is an Indian-American computer scientist and a winner of the prestigiousTuring Award. He is one of the early pioneers of Artificial Intelligence and has served on the faculty of Stanford and Carnegie Mellonfor over 40 years. He was the founding Director of the Robotics Institute at CMU. He was instrumental in helping to create Rajiv Gandhi University of Knowledge Technologies in India, to cater to the educational needs of the low-income, gifted rural youth. He is also the Chairman of International Institute of Information Technology, Hyderabad.


Life


Dabbala Rajagopal Reddy was born on June 13, 1937, in Katur, Chittoor district, Andhra Pradesh, India.  He received his bachelor's degree in civil engineering from Guindy Engineering College of the University of Madras (now Anna University, Chennai), India, in 1958. After that Reddy moved to Australia, and there he received a master's degree in technology from the University of New South Wales, Australia, in 1960. He also received a doctorate degree in computer science from Stanford University in 1966.

On the same year he started his academic career as an Assistant Professor in the same University. After that he joined as a member of Carnegie Mellon University faculty in 1969. He was the Founding Director of the Robotics Institute at the University from 1979 to 1991.

Now, he lives in Pittsburgh with his wife and they have two daughters.


Career


Reddy is the Moza Bint Nasser University Professor of Computer Science and Robotics in the School of Computer Science atCarnegie Mellon University. From 1960, Reddy worked for IBM in Australia. He was an Assistant Professor of Computer Science atStanford University from 1966–69. He joined the Carnegie Mellon faculty as an Associate Professor of Computer Science in 1969. He became a Full Professor in 1973, and a University Professor in 1984.

He was the founding Director of the Robotics Institute from 1979 to 1991and the Dean of School of Computer Science from 1991 to 1999. As a Dean of SCS, he helped create the Language Technologies Institute, Human Computer Interaction Institute, Center for Automated Learning and Discovery (since renamed as the Machine Learning Department), and the Institute for Software Research. He is the Chairman of Governing Council of IIIT Hyderabad and he is the Chancellor and the Chairman of the Governing Council of the Rajiv Gandhi University of Knowledge Technologies, India.

Reddy was a co-chair of the President's Information Technology Advisory Committee (PITAC) from 1999 to 2001. He was one of the founders of the American Association for Artificial Intelligence and was its President from 1987 to 1989. He serves on the International Board of Governors of Peres Center for Peace in Israel. He is a member of the governing councils of EMRI and HMRI which use technology-enabled solutions to provide cost-effective health care coverage to rural population in India.



Research


Reddy's early research was conducted at the AI labs at Stanford, first as a graduate student and later as an Assistant Professor, and at CMU since 1969. His AI research concentrated on perceptual and motor aspect of intelligence such as speech, language, vision and robotics. Over a span of three decades, Reddy and his colleagues created several historic demonstrations of spoken language systems, e.g., voice control of a robot, large vocabulary connected speech recognition, speaker independent speech recognition,and unrestricted vocabulary dictation. Reddy and his colleagues have also made seminal contributions to Task Oriented Computer Architectures,Analysis of Natural Scenes, Universal Access to Information, and Autonomous Robotic Systems. Hearsay I is one of the first systems capable of continuous speech recognition. Subsequent systems like Hearsay II, Dragon, Harpy, and Sphinx I/II developed many of the ideas underlying modern commercial speech recognition technology as summarized in his recent historical speech recognition review with Xuedong Huang and James K. Baker.

Some of these ideas—most notably the "blackboard model" for coordinating multiple knowledge sources—have been adopted across the spectrum of applied artificial intelligence. His other major research interest has been in exploring the role of "Technology in Service of Society". An early attempt in this area was the establishment, in 1981, of "Centre Mondial Informatique et Ressource Humaines" in France by Jean-Jacques Servan-Schreiber and a technical team of Nicholas Negroponte, Alan Kay, Seymour Papertand Terry Winograd. Reddy served as the Chief Scientist for the center.

One of Reddy's current research interests is the "Universal Digital Library Project".The project includes efforts to archive 1,000 newspapers for the next 1,000 years and provide online access to UNESCO heritage sites.


Awards and honors


His awards and recognitions include the following:

    He is a fellow of the Acoustical Society of America, IEEE and AAAI.


    Reddy is a member of the United States National Academy of Engineering, American Academy of Arts and Sciences, Chinese Academy of Engineering, Indian National Science Academy, and Indian National Academy of Engineering.


    He has been awarded honorary doctorates (Doctor Honoris Causa) from SV University, Universite Henri-Poincare, University of New South Wales, Jawaharlal Nehru Technological University, University of Massachusetts, University of Warwick, Anna University, Indian Institute for Information Technology (Allahabad), Andhra University, IIT Kharagpur and Hong Kong University of Science and Technology.


    In 1994 he and Edward Feigenbaum received the ACM Turing Award "For pioneering the design and construction of large scale artificial intelligence systems, demonstrating the practical importance and potential commercial impact of artificial intelligence technology".


    In 1984, Reddy was awarded the French Legion of Honour by French President François Mitterrand for his contributions as Chief Scientist at "Centre Mondial Informatique" in Paris in the use of "Technology in Service of Society".


    In 2001, Reddy was awarded Padma Bhushan, an award given by the Indian Government that recognizes distinguished service of a high order to the nation.


    In 2004, Reddy received the Okawa Prize for pioneering researches of large scale artificial intelligence system, human-computer interaction and Internet, and outstanding contributions to information and telecommunications policy and nurture of many human resources.


    He received the 2005 IJCAI Donald E. Walker Distinguished Service Award For, "His outstanding service to the AI community as President of AAAI, Conference Chair of IJCAI-79, and his leadership and promotion of AI internationally". He also received the IBM Research Ralph Gomory Visiting Scholar Award in 1991.


    In 2005, Reddy received the Honda Prize for his pioneering role in robotics and computer science which are expected to be used in the future society for a broad range of applications including education, medicine, healthcare, and disaster relief.


    In 2006 he received the Vannevar Bush Award, the highest Award of National Science Foundation in United States, for his lifetime contribution to science and long-standing statesmanship in science and behalf of the nation.


    In 2008, Reddy received the IEEE James L. Flanagan Speech and Audio Processing Award, "for leadership and pioneering contributions to speech recognition, natural language understanding, and machine intelligence".


    In 2011, Reddy was inducted into IEEE Intelligent Systems' AI's Hall of Fame for the "significant contributions to the field of AI and intelligent systems".

Contributions


    Machine Intelligence and Robotics: Report of the NASA Study Group — Executive Summary, Final Report Carl Sagan (chair), Raj Reddy (vice chair) and others, NASA JPL, September 1979


    Foundations and Grand Challenges of Artificial Intelligence, AAAI Presidential Address, 1988.


    To Dream the Possible Dream, Turing Award Lecture presented at ACM CS Conference, March 1, 1995



Posted by : Vipula Deshmukh

26 November, 2014

Antonie van Leeuwenhoek






Antonie Van Leeuwenhoek (October 24, 1632 – August 26, 1723) was a Dutch scientist. He was born in Delft, Dutch Republic, on October 24, 1632. He is also known as "the Father of Microbiology".  He is known for his work on the improvement of the microscope and for his contributions towards the establishment of microbiology. He was the first to observe and describe single-celled organisms, which he originally referred to as animalcules, and which are now referred to as microorganisms. He was also the first to record microscopic observations of muscle fibers, bacteria, spermatozoa, and blood flow in capillaries. Leeuwenhoek discoveries came to light through correspondence with the Royal Society, which published his letters.

Leeuwenhoek’s interest in microscopes and a familiarity with glass processing led to one of the most significant insights in the history of science. By placing the middle of a small rod of soda lime glass in a hot flame, Leeuwenhoek could pull the hot section apart to create two long whiskers of glass. Then, by reinserting the end of one whisker into the flame, he could create a very small, high-quality glass sphere. These spheres became the lenses of his microscopes, with the smallest spheres providing the highest magnifications.

 By the end of the 17th century, Leeuwenhoek had a monopoly on microscopic study and discovery. His contemporary Robert Hooke, an early microscope pioneer, bemoaned that the field had come to rest entirely on one man's shoulders. To the disappointment of his guests, Leeuwenhoek refused to reveal the cutting-edge microscopes he relied on for his discoveries, instead showing visitors a collection of average-quality lenses. Leeuwenhoek realized that if his simple method for creating the critically important lens was revealed, the scientific community of his time would likely disregard or even forget his role in microscopy. He therefore allowed others to believe that he was laboriously spending most of his nights and free time grinding increasingly tiny lenses to use in microscopes, even though this belief conflicted both with his construction of hundreds of microscopes and his habit of building a new microscope whenever he chanced upon an interesting specimen that he wanted to preserve. He made about 200 microscopes with different magnification.

 Leeuwenhoek made more than 500 optical lenses. He also created at least 25 microscopes, of differing types, of which only nine survived. His microscopes were made of silver or copper frames, holding hand-made lenses. Those that have survived are capable of magnification up to 275 times. It is suspected that Leeuwenhoek possessed some microscopes that could magnify up to 500 times. Although he has been widely regarded as a dilettante or amateur, his scientific research was of remarkably high quality.

Leeuwenhoek used samples and measurements to estimate numbers of microorganisms in units of water. He studied a broad range of microscopic phenomena, and shared the resulting observations freely with groups such as the English Royal Society.

In 1673, Leeuwenhoek began writing letters to the newly-formed Royal Society of London, describing what he had seen with his microscopes -- his first letter contained some observations on the stings of bees. For the next fifty years he corresponded with the Royal Society; his letters, written in Dutch, were translated into English or Latin and printed in the Philosophical Transactions of the Royal Society, and often reprinted separately.

 Such work firmly established his place in history as one of the first and most important explorers of the    
microscopic world.

Leeuwenhoek's main discoveries are:
1) The infusoria (protists in modern zoological classification), in 1674
2) The bacteria, (e.g., large Selenomonads from the human mouth), in 1676
3) The vacuole of the cell.
4) The spermatozoa in 1677.
5) The banded pattern of muscular fibers, in 1682.

By the end of his life, Leeuwenhoek had written approximately 560 letters to the Society and other scientific institutions concerning his observations and discoveries. Even when dying, Leeuwenhoek kept sending letters full of observations to London. The last few also contained a precise description of his own illness. He suffered from a rare disease, an uncontrolled movement of the midriff, which is now named Van Leeuwenhoek's disease. He died at the age of 90, on August 26, 1723 and was buried four days later in the Oude Kerk (Delft).

In 1981 the British microscopist Brian J. Ford found that Leeuwenhoek's original specimens had survived in the collections of the Royal Society of London. They were found to be of high quality, and were all well preserved. Ford carried out observations with a range of microscopes, adding to our knowledge of Leeuwenhoek's work.

References: www.google.com/wikipedia
Posted by
Prachi Shewale

 

25 November, 2014

Prof.Govind Swarup


PROF. GOVIND SWARUP


        
 
BornMarch 23, 1929 (age 85)
Thakurdwara, Uttar Pradesh
ResidencePune
NationalityIndian
FieldsRadioastronomy
InstitutionsTIFR;
Known forRadioastronomy; R&D;
Notable awardsPadma Sri;Bhabha Award for Lifetime Achievement by the Prime minister of India; S S Bhatnagar;




Professor Govind Swarup, (born Mar 23, 1929 in Thakurdwara, Uttar Pradesh India) of the Tata Institute of Fundamental Research (TIFR), is an internationally renowned radio astronomer and one of the pioneers ofradio astronomy. He is known not only for his many important research contributions in several areas of astronomy and astrophysics, but also for his outstanding achievements in building ingenious, innovative and powerful observational facilities for front-line research in radio astronomy. He has been the key scientist behind concept, design and installation of the Ooty Radio Telescope (India) and the Giant Metrewave Radio Telescope (GMRT) near Pune. Under his leadership, a strong group in radio astrophysics has been built at Tata Institute of Fundamental Research that is comparable to the best in the world.


Early life and Education

Govind Swarup was born at Thakurdwara, Uttar Pradesh in 1929. He received B.Sc. degree in 1948 and M.Sc. in Physics in 1950 from theAllahabad University and Ph.D. from Stanford University in 1961. He was awarded Doctor of Engineering (Honoris Causa), University of Roorkee in 1987 and Doctor of Science (Honoris Causa), Banaras Hindu University in 1996. He was at the National Physical Laboratory, New Delhi (1950–53 and 1955–56), CSIRO, Australia (1953–55), Research Associate at Harvard University (1956–57), Research Assistant at Stanford University (1957–60) and Assistant Professor at Stanford University (1961–63). Doctor of Science (Honoris Causa), Banaras Hindu University in 1996 and Pt. Ravishankar Shukla University, Raipur in 2010.

Career

Initially he joined National Physical laboratory for two years. Returning from St anford to India in March 1963, he joinedTIFR as a Reader at the request of Dr. Homi Bhabha. In 1965, he became Associate Professor, Professor in 1970, and Professor of Eminence at in 1989. He became Project Director of the GMRT in 1987, Centre Director of the National Centre for Radio Astrophysics (NCRA) of TIFR in 1993 and retired from TIFR in 1994.

Major Contribution

During 1953-65 Prof. Swarup made the discovery of 'Type U' solar radio bursts; developed a gyro-radiation model for explaining the microwave solar emission and made studies of the radio emission from the Quiet Sun. In 1959 he developed a round trip transmission technique for phase measurements, which has been used in almost all the radio interferometers in the world. In 1962 he found the first example of a steep spectrum 'bridge' of radio emission between the two radio lobes of the powerful radio galaxy, Cyg-A, using the Stanford Compound Interferometer; such bridges allow estimates of the age of a radio galaxy.
During 1963-70, he constructed a 530 m long and 30 m wide parabolic-cylindrical radio telescope of a unique and innovative design at Ooty in South India, which was placed on a suitably inclined hill so as to make its long axis of rotation parallel to that of the earth, enabling it to track celestial radio sources in hour angle for 9.5 hrs. Using the method of lunar occultation, it provided for the first time high-resolution angular data (1 to 10 arc sec) for more than 1,000 weak radio sources, which provided an independent evidence for the Big Bang model. Ooty Occultation observations of the galactic centre source, Sgr-A, yielded the first 2-dimensional separation of its thermal and non-thermal emission. During the 1980s, Swarup studied characteristics of jets, cores and hot spots of quasars based on polarization observations.
During 1984-96, he conceived and directed the design and construction of the Giant Metrewave Radio Telescope(GMRT), consisting of 30 fully steerable parabolic dishes of 45m diameter that are located in a Y-shape array of about 25 km in extent in Western India. A novel concept developed by him made it possible to construct such large antennas very economically. GMRT is a highly versatile instrument. It is the world's largest radio telescope operating in the frequency range of about 130-1430 MHz. At present he is making observations with the GMRT of the emission and absorption of atomic hydrogen from objects in the early Universe. Recently, along with S.K. Sirothia, he has investigated deficiency of radio sources at 327 MHz towards the prominent cold spot of the cosmic microwave background radiation. To summarize, during the last 40 years he has made important contributions in areas such as solar radio emission, interplanetary scintillations, pulsars, radio galaxies, quasars and cosmology. He has published over 125 research papers and edited 4 books. He has two patents.

Awards and Memberships of technological Committees

Membership of Professional Societies: Royal Society, London; Indian National Science Academy; Indian Academy of Sciences; National Academy of Sciences, Allahabad, India; Third World Academy of Sciences; Indian Geophysical Union; Maharashtra Academy of Sciences; Institution of Electronics & Telecommunication Engineers; Indian Physics Association; Indian Physical Society; International Academy of Astronautics; Pontifical Academy of Sciences; Royal Astronomical Society, London;Astronomical Society of India (President 1975-77); International Astronomical Union (IAU) (President, Commission 40 on Radio Astronomy, 1979–82); Executive Committee, Inter Union Commission for Frequency Allocation (IUCAF till 1995); IAU Working Group for Future Large Scale Facilities (1994-2000); Chairman, Indian National Committee for International Union of Radio Science (URSI) (1986-88 & 1995-97); Post-detection Sub-Committee of SETI of International Astronautical Federation (Chairman, 1994–98); Chairman, URSI Committee for Developing Countries (1996-2002); URSI Standing Committee for Future General Assemblies (1999-2002). Editorial Boards, Indian Journal of Radio & Space Physics (1990-2000), National Academy of Sciences, India; (1997-2000).
Awards: 
                   1973 Padma Shri; 1972 S.S. Bhatnagar, Council of Scientific & Industrial Research, India; 1974 Jawaharlal Nehru Fellowship for 2 years; 1984 P.C. Mahalanobis Medal, Indian National Science Academy; 1986 Biren Roy Trust Medal, Indian Physical Society, Calcutta; 1987 Dr. Vainu Bappu Memorial Award, Indian National Science Academy; 1987 Tskolovosky Medal, Federation of Cosmonautics, USSR; 1987 Meghnad Saha Medal, National Academy of Sciences, India; 1988 The Third World Academy of Sciences Award in Physics; 1990 John Howard Delinger Gold Medal, International Union of Radio Sciences; 1990 R.D. Birla Award in Physics, Indian Physics Association; 1991 FIE Foundation Award for Eminence in Science & Technology, Ichhalkaranji, India; 1993 Gujar Mal Modi Science Award, Modi Foundation, India; 1993 The C.V. Raman Medal, Indian National Science Academy; 1994 Sir Devaprasad Sarbadhikari Medal, Calcutta University; 1995 M.P. Birla Award, Birla Institute of Astronomy and Planetarium Sciences, Calcutta; 1999 12th Khwarizmi International Award, Iran; 2001 H.K. Firodia Award; 2005 Herschel Medal of the Royal Astronomical Society; 2006, Lifetime Achievement Award by the University of Pune; 2007 Grote Reber Medal; 2007, Presidents Medal by the Indian Science Congress; 2009 Homi Bhabha Award for Lifetime Achievement by the Prime minister of India.

   Refernces : www.google.com
                    
Name: Gore Dhanashree Nivrutti