PMO OpenIR  > 太阳高能及相关物理过程研究团组
An interpretation of a HXR flare with exceedingly long delay
Li, YP; Gan, WQ
2001-07-01
Source PublicationCHINESE ASTRONOMY AND ASTROPHYSICS
ISSN0275-1062
Volume25Issue:3Pages:326-334
AbstractThe hard X-ray (HXR) peak delay of the 3B solar flare in 1354-1624 UT on March 6, 1989 was so long as 130 seconds, while the time of rise to the peak in the lowest energy channel of HXRs was only 150 seconds. The authors explain this peculiar event with the trap plus precipitation model of electrons and find that it can be well interpreted if there existed two successive sources and the coronal density is taken to be 10(9) cm(-3).
KeywordFlare Hard X-ray Delay
Subject AreaAstronomy & Astrophysics
WOS HeadingsScience & Technology ; Physical Sciences
WOS KeywordX-RAY-BURSTS ; PLUS-PRECIPITATION MODEL ; OF-FLIGHT DISTANCES ; SOLAR-FLARES ; GAMMA-RAY ; TIME PROFILES ; TRAP MODELS ; ACCELERATION
Indexed BySCI
Language英语
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000170928800008
Citation statistics
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/8196
Collection太阳高能及相关物理过程研究团组
AffiliationChinese Acad Sci, Purple Mt Observ, Nanjing 210008, Peoples R China
Recommended Citation
GB/T 7714
Li, YP,Gan, WQ. An interpretation of a HXR flare with exceedingly long delay[J]. CHINESE ASTRONOMY AND ASTROPHYSICS,2001,25(3):326-334.
APA Li, YP,&Gan, WQ.(2001).An interpretation of a HXR flare with exceedingly long delay.CHINESE ASTRONOMY AND ASTROPHYSICS,25(3),326-334.
MLA Li, YP,et al."An interpretation of a HXR flare with exceedingly long delay".CHINESE ASTRONOMY AND ASTROPHYSICS 25.3(2001):326-334.
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