Energetic electron heating and chromospheric evaporation during a well-observed compact flare
Energetic electron heating and chromospheric evaporation during a well-observed compact flare
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观察良好的紧凑型耀斑期间的高能电子加热和色球蒸发
DOI：
10.1086/162798
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发表时间：
1985
期刊：
影响因子：
--
通讯作者：
T. A. Gunkler
中科院分区：
文献类型：
--
作者：
R. Canfield;T. A. Gunkler
从太阳极大期使命（SMM）和萨克拉门托峰天文台（SPO），我们观测到了1980年5月7日的致密太阳耀斑，Acton等人（1982）和Simnett（1983）曾对该耀斑进行过研究，X射线和H.的空间、光谱和时间分辨率都很高。阿尔法帽。根据色球耀斑过程的物理模型和从X射线观测中推断出的模型参数，
From the Solar Maximum Mission (SMM) and Sacramento Peak Observatory (SPO) we observed the compact solar flare of 1980 May 7, previously studied by Acton et al. (1982) and Simnett (1983), with spatial, spectral, and temporal resolution in both X-rays and H..cap alpha.. profiles based on physical models of chromospheric flare processes and model parameters inferred from the X-ray observations.