Solar flare physics enlivened by TRACE and RHESSI

被引：6

作者：

Aschwanden, Markus J. ^{[1
]}

机构：

[1] Lockheed Martin Adv Technol Ctr, Solar & Astrophys Lab, Org ADBS, Palo Alto, CA 94304 USA

来源：

JOURNAL OF ASTROPHYSICS AND ASTRONOMY | 2008年 / 29卷 / 1-2期

关键词：

solar flares; particle acceleration; hard X-rays;

D O I：

10.1007/s12036-008-0015-0

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The Transition Region and Coronal Explorer (TRACE) gave us the highest EUV spatial resolution and the Ramaty High Energy Solar Spectrometric Imager (RHESSI) gave us the highest hard X-ray and gamma-ray spectral resolution to study solar flares. We review a number of recent highlights obtained from both missions that either enhance or challenge our physical understanding of solar flares, such as: 1. Multi-thermal Diagnostic of 6.7 and 8.0 keV Fe and Ni lines, 2. Multi-thermal Conduction Cooling Delays, 3. Chromospheric Altitude of Hard X-Ray Emission, 4. Evidence for Dipolar Reconnection Current Sheets, 5. Footpoint Motion and Reconnection Rate, 6. Evidence for Tripolar Magnetic Reconnection, 7. Displaced Electron and Ion Acceleration Sources.

引用

页码：115 / 124

页数：10

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