中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Pulsations of microwave flaring emission at low and high frequencies

文献类型:期刊论文

作者Reznikova, V. E.; Melnikov, V. F.; Su, Y.; Huang, G.
刊名ASTRONOMY REPORTS
出版日期2007-07-01
卷号51期号:7页码:588-596
关键词CORONAL LOOP OSCILLATIONS SOLAR RADIO-BURSTS GYROSYNCHROTRON EMISSION PLASMA ELECTRONS SUMER
ISSN号1063-7729
英文摘要A wavelet analysis of the flare-intensity variations has been carried out for a solar flare observed with the Nobeyama Radioheliograph at 17 and 34 GHz and the spectrometer of Purple Mountain Observatory at 4.5-7.5 GHz. The signals contain a well-pronounced periodicity with a period of P = 14-17 s and stable, coherent behavior at frequencies higher and lower than the peak frequency. We simulated the modulation of the gyrosynchrotron emission by fast sausage magnetoacoustic oscillations for the cases of low and high plasma density in the radio source. The synchronism of the pulsations at high and low frequencies can be realized only in the case of high plasma density, when the low-frequency turnover of the microwave spectrum is due to the Razin effect, not self-absorption.
WOS标题词Science & Technology ; Physical Sciences
学科主题Astronomy & Astrophysics
类目[WOS]Astronomy & Astrophysics
研究领域[WOS]Astronomy & Astrophysics
关键词[WOS]CORONAL LOOP OSCILLATIONS ; SOLAR RADIO-BURSTS ; GYROSYNCHROTRON EMISSION ; PLASMA ; ELECTRONS ; SUMER
收录类别SCI
语种英语
WOS记录号WOS:000248325400008
公开日期2012-02-04
源URL[http://159.226.72.40/handle/332002/2338]  
专题紫金山天文台_分子云与恒星形成研究团组
作者单位1.Chinese Acad Sci, Purple Mt Observ, Nanjing, Peoples R China
2.Radiophys Res Inst, NIRFI, Nizhnii Novgorod, Russia
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Reznikova, V. E.,Melnikov, V. F.,Su, Y.,et al. Pulsations of microwave flaring emission at low and high frequencies[J]. ASTRONOMY REPORTS,2007,51(7):588-596.
APA Reznikova, V. E.,Melnikov, V. F.,Su, Y.,&Huang, G..(2007).Pulsations of microwave flaring emission at low and high frequencies.ASTRONOMY REPORTS,51(7),588-596.
MLA Reznikova, V. E.,et al."Pulsations of microwave flaring emission at low and high frequencies".ASTRONOMY REPORTS 51.7(2007):588-596.

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来源:紫金山天文台

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