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Microwave, optical, EUV, and hard X-ray signature of possible coronal loop interaction

文献类型:期刊论文

作者Huang, GL; Ji, HS
刊名SOLAR PHYSICS
出版日期2005-07-01
卷号229期号:2页码:227-236
关键词SOLAR-FLARES EXTREME-ULTRAVIOLET MASS EJECTION H-ALPHA CONFIGURATION REGION
ISSN号0038-0938
英文摘要In this paper, we present a comprehensive picture for the M2.0 class flare of September 9, 2002 with an extensive multi-wavelength analysis. The flare was observed by the Ramaty High Energy Solar Spectroscopic Imager (RHESSI), the Owens Valley Solar Arrays (OVSA), and Big Bear Solar Observatory (BBSO). At BBSO, the observation was specially made at the wavelength of H alpha-1.3 angstrom with a cadence of similar to 40ms. For this multi-kernel flare, we find two pairs of conjugate kernels. Each pair has its centroid separation curve, which is well correlated with its own optical light curve. This clearly indicates two separate energy releasing sites. The proposed picture of the two energy release sites is supported by double peaks in microwave profiles, and, especially, the presence of two different 195 A flaring loops observed by the Extreme UV Imaging Telescope (EIT) on board the Solar and Heliospheric Observatory (SOHO). Nevertheless, the two pairs surely have some intrinsic relations, which are indicated from both temporal and spatial correlations. Because of the intimate relationship, we propose that the two loop systems were interacting during the flare. In addition, one of the most pronounced features of this multi-kernel flare is that the results from microwaves are poorly correlated with those from hard X-ray (HXR) and optical data. The discrepancy is shown in two aspects: time profiles as well as emission locations. We still cannot understand the cause of the discrepancy, except that the interacting loops may have complicated the situation.
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]SOLAR-FLARES ; EXTREME-ULTRAVIOLET ; MASS EJECTION ; H-ALPHA ; CONFIGURATION ; REGION
收录类别SCI
语种英语
WOS记录号WOS:000233324100004
公开日期2012-03-07
源URL[http://159.226.72.40/handle/332002/4138]  
专题紫金山天文台_太阳活动的多波段观测研究团组
作者单位Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Peoples R China
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GB/T 7714
Huang, GL,Ji, HS. Microwave, optical, EUV, and hard X-ray signature of possible coronal loop interaction[J]. SOLAR PHYSICS,2005,229(2):227-236.
APA Huang, GL,&Ji, HS.(2005).Microwave, optical, EUV, and hard X-ray signature of possible coronal loop interaction.SOLAR PHYSICS,229(2),227-236.
MLA Huang, GL,et al."Microwave, optical, EUV, and hard X-ray signature of possible coronal loop interaction".SOLAR PHYSICS 229.2(2005):227-236.

入库方式: OAI收割

来源:紫金山天文台

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