Microwave, soft and hard X-ray observations of solar flares - A self-consistent model of the flare site

被引：4

作者：

Drago, FC ^{[1
]}

Alissandrakis, CE

Bentley, RD

Philips, AT

机构：

[1] Univ Florence, Dept Astron & Space Sci, I-50121 Florence, Italy

[2] Univ Ioannina, Sect Astrogeophys, GR-45110 Ioannina, Greece

[3] UCL, Mullard Space Sci Lab, Dorking RH5 6NT, Surrey, England

来源：

SOLAR PHYSICS | 1998年 / 182卷 / 02期

关键词：

D O I：

10.1023/A:1005044905663

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

High-resolution microwave observations of several flares performed with the Westerbork Synthesis Radio Telescope (WRST) on 3 and 3 July 1993 are compared with Yuhkoh observations in the soft and hard X-ray domain. Only for one flare, among the six analyzed, was the hard X-ray spectrum between 20 and 200 keV available from the Wide Bragg Spectrometer, supplying the energy spectrum of non-thermal particles responsible for this radiation and for the radio emission. A complete model of this flare is derived which accounts for all available observations in the X-ray and radio wavelengths.

引用

页码：459 / 476

页数：18

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