scholarly journals Dynamics of Flare Processes and Variety of the Fine Structure of Solar Radio Emission over a Wide Frequency Range of 30 – 7000 MHz

Solar Physics ◽  
2014 ◽  
Vol 290 (1) ◽  
pp. 95-114 ◽  
Author(s):  
Gennady Chernov ◽  
Valery Fomichev ◽  
Baolin Tan ◽  
Yihua Yan ◽  
Chengming Tan ◽  
...  
Keyword(s):  
Fine Structure ◽  
Radio Emission ◽  
Solar Radio ◽  
Wide Frequency Range ◽  
Solar Radio Emission ◽  
Frequency Range

Fine structure in solar radio emission

1977 ◽  
Vol 20 (9) ◽  
pp. 975-988 ◽  
Author(s):  
P. M. McCulloch ◽  
G. R. A. Ellis
Keyword(s):  
Fine Structure ◽  
Radio Emission ◽  
Solar Radio ◽  
Solar Radio Emission

scholarly journals Bursts of microwave radio emission associated with solar flares

1959 ◽  
Vol 9 ◽  
pp. 218-221 ◽  
Author(s):  
G. B. Gelfreich ◽  
V. N. Ikhsanova ◽  
N. L. Kaĭdanovskiĭ ◽  
N. S. Soboleva ◽  
G. M. Timofeeva ◽  
...  
Keyword(s):  
Radio Emission ◽  
Solar Flares ◽  
Solar Radio ◽  
Solar Radio Emission ◽  
Frequency Range ◽  
Microwave Radio

Bursts of solar radio emission which coincide in time with solar flares are occasionally observed over the whole frequency range up to 35,000 Mc/s. The purpose of this paper is to describe briefly some bursts observed at Pulkovo at wavelength λ = 3.2 cm.

scholarly journals Development of solar flares and features of the fine structure of solar radio emission

2017 ◽  
Vol 57 (6) ◽  
pp. 738-751 ◽  
Author(s):  
G. P. Chernov ◽  
V. V. Fomichev ◽  
Y. Yan ◽  
B. Tan ◽  
Ch. Tan ◽  
...  
Keyword(s):  
Fine Structure ◽  
Radio Emission ◽  
Solar Flares ◽  
Solar Radio ◽  
Solar Radio Emission

Thermal Cyclotron Radiation from Solar Active Regions

1980 ◽  
Vol 86 ◽  
pp. 87-99
Author(s):  
V.V. Zheleznyakov ◽  
E. Ya. Zlotnik
Keyword(s):  
Fine Structure ◽  
Radio Emission ◽  
Frequency Spectrum ◽  
Solar Radio ◽  
Active Regions ◽  
Solar Radio Emission ◽  
Kinetic Temperature ◽  
Frequency Spectra ◽  
Solar Active Regions ◽  
Thermal Cyclotron Radiation

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.

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