HARD X-RAY OBSERVATIONS OF HIGH CORONAL REGIONS IN SOLAR FLARES

机译：太阳耀斑高冕区域的硬X射线观察

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Using Hard X-ray data obtained from the Hard X-ray Telescope (HXT) onboard Yohkoh I have studied coronal sources in three limb flares, including one particularly interesting event on April 23 1998. The results for the April flare show: (1) the existence of an extended source located in the high corona (～5000 km), and (2) dominant thermal and other sources do not come from the same looptop region. Preliminary results for the other two flares are also discussed.

机译：使用从Yohkoh上的Hard X-ray Telescope（HXT）获得的Hard X-ray数据，我研究了三个肢体耀斑的日冕来源，包括1998年4月23日的一次特别有趣的事件。4月耀斑的结果显示：（1）高电晕（〜5000 km）处存在扩展的热源，（2）主热源和其他热源都不来自同一环顶区域。还讨论了其他两个耀斑的初步结果。

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《Yohkoh 10th Anniversary Meeting on Multi-Wavelength Observations of Coronal Structure and Dynamics Jan 20-24, 2002 Kona, Hawaii, USA》|2002年|p.407-408|共2页
会议地点 Kona HI(US);Kona HI(US)
作者
J. Sato;
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作者单位

Physics Department, Montana State University, P.O. Box 173840, Bozeman, MT 59717, USA;

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原文格式 PDF
正文语种 eng
中图分类天文学;
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3. An Observational Study on Coronal Hard X-ray Sources in Flares [J] . Wei-Dong B., You-Ping L.I., Wei-Qun G. Chinese Astronomy and Astrophysics . 2012,第3期

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8. Solar Observations during Skylab, April 1973-February 1974. I. Coronal X-Ray Structure. II. Solar Flare Activity [R] . Hanson, J. M., Roelof, E. C., Gold, R. E. 1983

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HARD X-RAY OBSERVATIONS OF HIGH CORONAL REGIONS IN SOLAR FLARES

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