NASA IRIS Home Page
English
United States, Denver
University of Oslo Virtual Solar Observatory Level
数据描述
IRIS is a NASA small explorer mission developed and operated by LMSAL with mission operations executed at NASA Ames Research Center and major contributions to downlink communications funded by ESA and the Norwegian Space Centre.
iris.lmsal.com
IP: 166.21.241.141
加载中...
相关论文
3Observation of super-Alfvénic slippage of reconnecting magnetic field lines on the Sun
Juraj Lörinčík•Jaroslav Dudík•Alberto Sainz Dalda•Guillaume Aulanier•Vanessa Polito等 6 人
Nature Astronomy
2024
•2024/10/18
•00 p.1-10
Slipping motions of magnetic field lines are a distinct signature of three-dimensional magnetic reconnection, a fundamental process driving solar and stellar flares. While being a key prediction of numerical experiments, the rapid super-Alfvénic field line slippage driven by the ‘slip-running’ recon...
Astrophysical magnetic fieldsAstrophysical plasmasSolar physics
10.1038/S41550-024-02396-4
ISSN:2397-3366
Multi-viewpoint observation of a failed prominence eruption on the Sun
Tingyu Gou•Katharine K. Reeves•Peter R. Young•Astrid M. Veronig•Xingyao Chen等 8 人
Nature Astronomy
2026
•2026/5/20
•00 p.1-12
Solar eruptions are sudden ejections of coronal mass and magnetic fields accompanied by intense energy release. The eruptive structure does not always erupt successfully: it sometimes fails to escape the Sun after initiation. The failure of an eruption, however, provides an invaluable opportunity fo...
Astrophysical plasmasSolar physics
10.1038/S41550-026-02872-Z
ISSN:2397-3366
Complete replacement of magnetic flux in a flux rope during a coronal mass ejection
Gou Tingyu•Liu Rui•Veronig Astrid M.•Zhuang Bin•Li Ting等 8 人
Nature Astronomy
2023
•2023/5/4
•00 p.1-10
Solar coronal mass ejections are the most energetic events in the Solar System. In their standard formation model, a magnetic flux rope builds up into a coronal mass ejection through magnetic reconnection that continually converts overlying, untwisted magnetic flux into twisted flux enveloping the p...
Solar physics
10.1038/S41550-023-01966-2
ISSN:2397-3366