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Magnetic field, helicity and the 2000 July 14 flare in solar active region 9077
Zhang, HQ
2002-05-01
Source PublicationMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume332Issue:2Pages:500-512
AbstractIn this paper we analyse the non-potential magnetic field and the relationship with current (helicity) in the active region NOAA 9077 in 2000 July, using photospheric vector magnetograms obtained at different solar observatories and also coronal extreme-ultraviolet 171-Angstrom images from the TRACE satellite.
KeywordSun : Activity Sun : Flares Sun : Magnetic Fields
Indexed BySCI
Language英语
WOS IDWOS:000175536700022
Citation statistics
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/8534
Collection太阳物理研究部
AffiliationChinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
Recommended Citation
GB/T 7714
Zhang, HQ. Magnetic field, helicity and the 2000 July 14 flare in solar active region 9077[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2002,332(2):500-512.
APA Zhang, HQ.(2002).Magnetic field, helicity and the 2000 July 14 flare in solar active region 9077.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,332(2),500-512.
MLA Zhang, HQ."Magnetic field, helicity and the 2000 July 14 flare in solar active region 9077".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 332.2(2002):500-512.
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