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A happy ending for SADs
被引:0
|作者:
Seaton, Daniel B.
[1
,2
]
机构:
[1] Univ Colorado, Cooperat Inst Res Environm Sci, Boulder, CO 80309 USA
[2] Southwest Res Inst, Boulder, CO 80302 USA
关键词:
RECONNECTION;
D O I:
10.1038/s41550-022-01607-0
中图分类号:
P1 [天文学];
学科分类号:
0704 ;
摘要:
Supra-arcade downflows (SADs) are dark, turbulent flows that appear in the Sun's corona during a solar flare, which have defied explanation for over two decades. A three-dimensional simulation can finally explain the origins of these plasma downflows.
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页码:299 / 301
页数:3
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