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	EVIDENCE OF THE SOLAR EUV HOT CHANNEL AS A MAGNETIC FLUX ROPE FROM REMOTE-SENSING AND IN SITU OBSERVATIONS
	Song, H. Q.; Chen, Y.; Zhang, J.; Cheng, X.; Wang, B.; Hu, Q.; Li, G.; Wang, Y. M.
刊名	ASTROPHYSICAL JOURNAL LETTERS
	2015
卷号	808期号:1
关键词	magnetic reconnection Sun: coronal mass ejections (CMEs) Sun: flares
DOI	10.1088/2041-8205/808/1/L15
URL标识	查看原文
内容类型	期刊论文
URI标识	http://www.corc.org.cn/handle/1471x/4776371
专题	山东大学
作者单位	1.Shandong Univ, Shandong Prov Key Lab Opt Astron & Solar Terr Env, Weihai 264209, Shandong, Peoples R China. 2.[Song
推荐引用方式 GB/T 7714	Song, H. Q.,Chen, Y.,Zhang, J.,et al. EVIDENCE OF THE SOLAR EUV HOT CHANNEL AS A MAGNETIC FLUX ROPE FROM REMOTE-SENSING AND IN SITU OBSERVATIONS[J]. ASTROPHYSICAL JOURNAL LETTERS,2015,808(1).
APA	Song, H. Q..,Chen, Y..,Zhang, J..,Cheng, X..,Wang, B..,...&Wang, Y. M..(2015).EVIDENCE OF THE SOLAR EUV HOT CHANNEL AS A MAGNETIC FLUX ROPE FROM REMOTE-SENSING AND IN SITU OBSERVATIONS.ASTROPHYSICAL JOURNAL LETTERS,808(1).
MLA	Song, H. Q.,et al."EVIDENCE OF THE SOLAR EUV HOT CHANNEL AS A MAGNETIC FLUX ROPE FROM REMOTE-SENSING AND IN SITU OBSERVATIONS".ASTROPHYSICAL JOURNAL LETTERS 808.1(2015).

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