中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
THE MORPHOLOGICAL-CHARACTERISTICS AND COOLING MECHANISMS OF THE POST-FLARE LOOP SYSTEM OF APRIL 28, 1980

文献类型:期刊论文

作者LIN, J; ZHANG, Z; WANG, Z; SMARTT, RN
刊名ASTRONOMY & ASTROPHYSICS
出版日期1992
卷号253期号:2页码:557-560
关键词SOLAR FLARE LOOP SYSTEM MORPHOLOGICAL EVOLUTION COOLING MECHANISM
ISSN号0004-6361
英文摘要The morphology and evolution of a post-flare loop system are described in the paper. The observational data show that this loop system is very complex, in which the loops are overlapped and inlaid. The whole loop system is in the relatively stable stage of the main phase, during which the variations of its form with time is slow and the variations of its brightness are also small. A simple method is used to compute the cooling of post-flare loops by radiation, conduction and expansion. The relative importance of radiative, conductive and expansive losses are briefly discussed. Finally, we investigate the most likely resource which permits the loops to stay bright for a long time.
WOS标题词Science & Technology ; Physical Sciences
学科主题天文和天体物理
类目[WOS]Astronomy & Astrophysics
研究领域[WOS]Astronomy & Astrophysics
关键词[WOS]SOLAR-FLARES ; COALESCENCE
收录类别SCI
语种英语
WOS记录号WOS:A1992GY75500031
公开日期2013-02-05
源URL[http://libir.pmo.ac.cn/handle/332002/8552]  
专题紫金山天文台_期刊(老文献)
作者单位1.NANJING UNIV, DEPT ASTRON, NANJING 210008, PEOPLES R CHINA
2.PURPLE MT OBSERV, NANJING 210008, PEOPLES R CHINA
3.NATL SOLAR OBSERV, SUNSPOT, NM 88349 USA
推荐引用方式
GB/T 7714
LIN, J,ZHANG, Z,WANG, Z,et al. THE MORPHOLOGICAL-CHARACTERISTICS AND COOLING MECHANISMS OF THE POST-FLARE LOOP SYSTEM OF APRIL 28, 1980[J]. ASTRONOMY & ASTROPHYSICS,1992,253(2):557-560.
APA LIN, J,ZHANG, Z,WANG, Z,&SMARTT, RN.(1992).THE MORPHOLOGICAL-CHARACTERISTICS AND COOLING MECHANISMS OF THE POST-FLARE LOOP SYSTEM OF APRIL 28, 1980.ASTRONOMY & ASTROPHYSICS,253(2),557-560.
MLA LIN, J,et al."THE MORPHOLOGICAL-CHARACTERISTICS AND COOLING MECHANISMS OF THE POST-FLARE LOOP SYSTEM OF APRIL 28, 1980".ASTRONOMY & ASTROPHYSICS 253.2(1992):557-560.

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来源:紫金山天文台

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