THE MORPHOLOGICAL-CHARACTERISTICS AND COOLING MECHANISMS OF THE POST-FLARE LOOP SYSTEM OF APRIL 28, 1980 | |
LIN, J; ZHANG, Z![]() ![]() | |
刊名 | ASTRONOMY & ASTROPHYSICS
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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. |
学科主题 | 天文和天体物理 |
WOS标题词 | Science & Technology ; Physical Sciences |
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 |
内容类型 | 期刊论文 |
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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