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Multi-wavelength observation of the 3N/X3.3 flare of 28 November 1998
You, JQ; Li, H; Fan, ZY; Sakurai, T
2001
Source PublicationSOLAR PHYSICS
ISSN0038-0938
Volume203Issue:1Pages:107-117
AbstractThe 3N/X3.3 flare of 28 November 1998 was observed in multiple wavelength simultaneously. The available data include H alpha images, spectra in He i 1083 nm and Ca ii 854.2 nm from Purple Mountain Observatory (PMO), soft X-ray (SXR) and hard X-ray (HXR) images and flux from Yohkoh. Morphological relationship investigation and spectral analysis of these data show: (1) The sudden brightening at loop top above the active region and the steep increase of SXR flux before flare onset suggest that the corona there had already been heated to some extent in the preflare phase. (2) The scales of the Ca ii 854.2 nm emission areas are very similar to those of the H alpha line, but the emission profiles look like those of the Ca ii K line. Most of the He i 1083 nm emissions exist in the bright H alpha kernels and can last to the decay phase. (3) Flare spectra show that line shift and asymmetry are very common in this flare not only in the impulsive phase but also in the decay phase. The difference in the line shifts or asymmetry between Ca ii 854.2 nm and He i 1083 nm, as well as the difference between the line center and wings of Ca ii 854.2 nm imply the existence of a velocity gradient in the line-of-sight direction. (4) Post-flare loops with very deep absorption (approximate to 70%) and very-high-velocity red shifts (30-90 km s(-)1) were observed in He i 1083 nm during the decay phase. However, only a slight dip can be found in the Ca ii 854.2 nm profile.
KeywordLimb Flare Line Spectra
Subject AreaAstronomy & Astrophysics
WOS HeadingsScience & Technology ; Physical Sciences
WOS KeywordLIMB FLARE ; LINE ; SPECTRA
Indexed BySCI
Language英语
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000172172600008
Citation statistics
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/8198
Collection太阳高能及相关物理过程研究团组
Affiliation1.CAS, Purple Mt Observ, Nanjing 210008, Peoples R China
2.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
3.Natl Astron Observ, Tokyo 181, Japan
Recommended Citation
GB/T 7714
You, JQ,Li, H,Fan, ZY,et al. Multi-wavelength observation of the 3N/X3.3 flare of 28 November 1998[J]. SOLAR PHYSICS,2001,203(1):107-117.
APA You, JQ,Li, H,Fan, ZY,&Sakurai, T.(2001).Multi-wavelength observation of the 3N/X3.3 flare of 28 November 1998.SOLAR PHYSICS,203(1),107-117.
MLA You, JQ,et al."Multi-wavelength observation of the 3N/X3.3 flare of 28 November 1998".SOLAR PHYSICS 203.1(2001):107-117.
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