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Diagnostics of the Solar Plasma Using Radio Observations with the RATAN-600

Published online by Cambridge University Press:  19 July 2016

G.B. Gelfreikh
G.B. Gelfreikh*
Affiliation:
Leningrad, USSR Central (Pulkovo) Astronomical Observatory Academy of Sciences of the USSR 196140 Leningrad, Pulkovo U.S.S.R.

Abstract

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This paper summarises the methods and main results of studying physical parameters and processes in different structures of the solar atmosphere from the chromosphere to the outer corona as based on the observations with a 600-meter radio telescope the RATAN-600 (1975-1989). Diagnostics of the solar plasma have been made using the spectral-polarization measurements in the wavelength range 0.8-32 cm with high spatial resolution. The most important results concern the structure and strength of the magnetic fields at different levels of the solar atmosphere and detection of localized regions of long-lasting (several days) energy release in the lower corona.

Type
IX. Solar Radio Emission
Information
Symposium - International Astronomical Union , Volume 142: Basic Plasma Processes on the Sun , 1990 , pp. 483 - 488
Copyright
Copyright © Kluwer 1990 

References

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