Cyclotron wave instability in the corona and origin of solar radio emission with fine structure

Solar Physics ◽  
1975 ◽  
Vol 44 (2) ◽  
pp. 461-470 ◽  
Author(s):  
V. V. Zheleznyakov ◽  
E. Ya. Zlotnik
1977 ◽  
Vol 20 (9) ◽  
pp. 975-988 ◽  
Author(s):  
P. M. McCulloch ◽  
G. R. A. Ellis

Solar Physics ◽  
2014 ◽  
Vol 290 (1) ◽  
pp. 95-114 ◽  
Author(s):  
Gennady Chernov ◽  
Valery Fomichev ◽  
Baolin Tan ◽  
Yihua Yan ◽  
Chengming Tan ◽  
...  

2017 ◽  
Vol 57 (6) ◽  
pp. 738-751 ◽  
Author(s):  
G. P. Chernov ◽  
V. V. Fomichev ◽  
Y. Yan ◽  
B. Tan ◽  
Ch. Tan ◽  
...  

1980 ◽  
Vol 86 ◽  
pp. 87-99
Author(s):  
V.V. Zheleznyakov ◽  
E. Ya. Zlotnik

Various frequency spectra with the fine structure resulting from the thermal cyclotron radio emission from solar active regions are discussed. The conditions in sources (distribution of magnetic field and kinetic temperature over the height) are put forward which provide the frequency spectrum as a set of cyclotron lines and high frequency cut-offs. For each kind of distribution the frequency spectrum and polarization are of peculiar character. This permits one to find the conditions in the source through the properties of the observed microwave solar radio emission. To obtain reliable data on the fine structure and judge about conditions in the sources it is necessary to study microwave solar radio emission using the swept-frequency or multi-channel receivers combined with high directional antennae.


Solar Physics ◽  
2021 ◽  
Vol 296 (3) ◽  
Author(s):  
Mahender Aroori ◽  
Panditi Vemareddy ◽  
Partha Chowdhury ◽  
Ganji Yellaiah

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