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Browsing Archival Collections by Author "Sastry, Ch. V"

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Observations of the brightness temperature distribution of the quiet solar corona at decametric wavelengths

Sastry, Ch. V (Indian Institute of Astrophysics, Bangalore, 1988)

The brightness temperature distribution of the quiet solar corona at a wavelength of 8.9 Meters is measured with two types of radio telescopes: (1) A “ T ” type array with a resolution of 26’x38’ and (2) A fan beam ...
Observations on the Fine Structures in Solar Decametric Radio Emission

Gopalswamy, N; Thejappa, G; Sastry, Ch. V (Indian Institute of Astrophysics, Bangalore, 1984)

The Solar decametric radio emission consists of a variety of fine structures. This reflects the complexity of the corona at this level. Two observations, viz. absorption bursts and short duration narrow band bursts are ...
Radio Emission From The Quiet Sun and Active Regions at Decametric Wavelengths

Sastry, Ch. V (Indian Institute of Astrophysics, Bangalore, 1986)

The Continuum emission from the Quiet Sun and active regions is the radiation from the solar atmosphere when there is no transient burst activity. At decametric wavelengths this radiation originates in the outer corona. A ...
Radio Observations of Compact Sources in the Outer Solar Corona

Ramesh, R; Subramanian, K. R; Sastry, Ch. V (Indian Institute of Astrophysics, Bangalore, 1997)

We have observed radio emission from the solar corona at a frequency of 77 MHz during the total solar eclipse on October 24, 1995 from our observatory at Gauribidanur. Sources of angular sizes less than or equal to 1.5' ...

Browsing Archival Collections by Author "Sastry, Ch. V"

Browsing Archival Collections by Author "Sastry, Ch. V"

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