On the Possible Connection between Photospheric 5-Min Oscillation and Solar Flare Microwave Emission

被引:0
|
作者
A. G. Kislyakov
V. V. Zaitsev
A. V. Stepanov
S. Urpo
机构
[1] Nizhny Novgorod,Institute of Applied Physics
[2] Pulkovo Observatory,undefined
[3] Metsähovi Radio Observatory,undefined
来源
Solar Physics | 2006年 / 233卷
关键词
Flare; Solar Flare; Wave Frequency; Radio Telescope; Dynamic Spectrum;
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摘要
Dynamic spectra of low-frequency modulation of microwave emission from solar flares are obtained. Data of 15 bursts observed in 1989–2000 with Metsähovi radio telescope at 37 GHz have been used. During 13 bursts a 5-min modulation of the microwave emission intensity was detected with the frequency of νI = 3.2± 0.24 (1σ) mHz. Five bursts revealed a 5-min wave superimposed on a ∼1 Hz, linear frequency modulated signal generated, presumably, by coronal magnetic loop, this wave frequency is νfm = 3.38± 0.37 (1σ) mHz. Both intensity and frequency modulations detected are in good agreement with the data on 5-min global oscillations of photosphere and with the data on the umbral velocity oscillations observed in the vicinity of sunspots. Possible role of p-mode photospheric oscillations in modulation of microwave burst emission is discussed.
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页码:89 / 106
页数:17
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