RHESSI Level-0 Data

NASA Open Data Portal2026-08-13 收录

太阳耀斑物理

太阳高能成像

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The Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) was a NASA Small Explorer mission launched in 2002 to investigate the physics of solar flares through...

Multipoint study of the rapid filament evolution during a confined C2 flare...

太阳暗条演化

太阳耀斑物理

Aims. This study focuses on the rapid evolution of the solar filament in active region 12975 during a confined C2 flare on 28 March 2022, which finally led to an eruptive M4...

University Corporation for Atmospheric Research50

Beam electrons as a source of H-alpha flare ribbons

太阳耀斑物理

H-alpha耀斑观测

Data for the paperDruett, M. et al. Beam electrons as a source of H-a flare ribbons. Nat. Commun. 8, 15905 doi: 10.1038/ncomms15905 (2017).

Figshare2017-06-13 更新30

The animations described in "X-ray/Radio Quasi-periodic Pulsations Associated with Plasmoids in Solar Flare Current Sheets"

太阳耀斑物理

等离子体动力学

Movie S1: An animation of the AIA 171, 211, and 131 {\AA} images covers the first flare (C3.8). The top panels show a large field of view, while the lower panels display a zoomed-in view of the area o

NIAID Data Ecosystem10

Spectropolarimetric insight into plasma sheet dynamics of a solar flare

太阳耀斑物理

等离子体光谱偏振分析

We examine spectropolarimetric data from the Coronal Multi-channel Polarimeter (CoMP) instrument, acquired during the evolution of the 2017 September 10 X8.2 solar flare on the...

University Corporation for Atmospheric Research30

Are all flare ribbons simply connected to the corona?

太阳耀斑物理

日冕能量传输

We consider the observational basis for the belief that flare ribbons in the chromosphere result from energy transport from the overlying corona. We study ribbons of small...

University Corporation for Atmospheric Research20

RHESSI Level-0 Data

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