Govind Swarup

@article{Saikia2021GovindS,
  title={Govind Swarup},
  author={D. J. Saikia},
  journal={Resonance},
  year={2021}
}
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References

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Atomic hydrogen is a fundamental constituent of galaxies, and is the primary fuel for star formation. Understanding how the atomic hydrogen content of galaxies evolves with time is thus critical to…
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This article describes the origin and development of the radio astronomy group of Tata Institute of Fundamental Research (TIFR), which later became the National Centre for Radio Astrophysics in Pune…
The Journey of a Radio Astronomer: Growth of Radio Astronomy in India
In this autobiographical account, I first describe my family, then childhood and education in India. During 1953–55, I worked in the new field of radio astronomy at the Division of Radiophysics of ...
A tribute to Professor Govind Swarup, FRS: the Father of Indian Radio Astronomy
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A technique is described for adjustment of phase paths within large antenna arrays or paraboloidal surfaces which are now in use, or are planned, for radio astronomy. After large paraboloids have…
Angular Size–Flux Density Relation for Extragalactic Radio Sources
Cosmology from Angular Size Counts of Extragalactic Radio Sources
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TLDR
The design, tests and preliminary results of a real-time parallel signal processor built to aid a wide variety of pulsar observations, which reduces the distortions caused by the effects of dispersion, Faraday rotation, doppler acceleration and parallactic angle variations.
Large Steerable Radio Telescope at Ootacamund, India
Lunar occultation observations for more than 150 radio sources have been made with the steerable radio telescope at Ootacamund, India. The radio telescope is also being used for the observation of…
A MODEL FOR THE SOURCES OF THE SLOWLY VARYING COMPONENT OF MICROWAVE SOLAR RADIATION
A comparison of the observations of the slowly varying component of the solar radio emission made with highresolution interferometers operating at wavelengths of 3.2, strong sources are higher at the…
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