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Spatio-Temporal Features of the Development of Microwave Emission of Active Regions and Flares

Published online by Cambridge University Press:  04 August 2017

G. Ya. Smolkov
G. Ya. Smolkov*
Affiliation:
SibIZMIR, Irkutsk, U.S.S.R.

Extract

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At SibIZMIR, a stepwise commissioning of the Siberian Solar Radio Telescope is being under way (Smolkov, 1982a; Smolkov et al., 1983a). This special-purpose instrument is designed to: 1) survey and monitor during daylight hours the state of solar activity (SA) with high two-dimensional resolution on a real time basis in a wave band permitting maximum possible detectability of active regions (AR's) and flares (F's); 2) study structures and development of AR's by day and the time of their observation on the solar disk; 3) study F's; 4) study the three-dimensional pattern of development of AR's and F's jointly with the Sayan Mountain and Baikal Astrophysical Observatories of SibIZMIR (Smolkov, 1982b), and 5) to make a synoptic study of SA during one or several solar rotations in the interests of solving challenging problems of Solar Physics and STP.

Type
Contributions From the U.S.S.R.
Information
Symposium - International Astronomical Union , Volume 107: Unstable Current Systems and Plasma Instabilities , 1985 , pp. 555 - 558
Copyright
Copyright © Reidel 1985 

References

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Smolkov, G. Ya., Treskov, T.A., Krissinel, G.B., and Potapov, N.N.: 1983a, In “Issled. po geomgn. aeron. i fiz. Solntsa”, Moscow, Nauka, 64, p.130.Google Scholar
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