Heating and cooling of coronal loops observed by SDO

	Heating and cooling of coronal loops observed by SDO
	Li, L. P.1,2; Peter, H.2; Chen, F.2; Zhang, J.1
刊名	ASTRONOMY & ASTROPHYSICS
	2015-11-01
卷号	583
关键词	Sun: corona Sun: UV radiation Sun: atmosphere Sun: activity
英文摘要	Context. One of the most prominent processes to have been suggested as heating the corona to well above 10(6) K builds on nanoflares, which are short bursts of energy dissipation.
收录类别	SCI
语种	英语
WOS记录号	WOS:000365072200130
内容类型	期刊论文
源URL	[http://ir.bao.ac.cn/handle/114a11/5534]
专题	国家天文台_太阳物理研究部
作者单位	1.Chinese Acad Sci, Natl Astron Observ, Key Lab Solar Act, Beijing 100012, Peoples R China 2.Max Planck Inst Solar Syst Res MPS, D-37077 Gottingen, Germany
推荐引用方式 GB/T 7714	Li, L. P.,Peter, H.,Chen, F.,et al. Heating and cooling of coronal loops observed by SDO[J]. ASTRONOMY & ASTROPHYSICS,2015,583.
APA	Li, L. P.,Peter, H.,Chen, F.,&Zhang, J..(2015).Heating and cooling of coronal loops observed by SDO.ASTRONOMY & ASTROPHYSICS,583.
MLA	Li, L. P.,et al."Heating and cooling of coronal loops observed by SDO".ASTRONOMY & ASTROPHYSICS 583(2015).