Energy partition in two solar flare/CME events

被引：214

作者：

Emslie, AG

Kucharek, H

Dennis, BR

Gopalswamy, N

Holman, GD

Share, GH

Vourlidas, A

Forbes, TG

Gallagher, PT

Mason, GM

Metcalf, TR

Mewaldt, RA

Murphy, RJ

Schwartz, RA

Zurbuchen, TH

机构：

[1] Univ Alabama, Dept Phys, Huntsville, AL 35899 USA

[2] Univ New Hampshire, Inst Study Earth Oceans & Space, Durham, NH 03824 USA

[3] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA

[4] USN, Res Lab, Washington, DC 20375 USA

[5] GSI, L 3 Commun, New York, NY USA

[6] Univ Maryland, Dept Phys, College Pk, MD 20742 USA

[7] Lockheed Martin Solar & Astrophys Lab, Dept L9 41, Palo Alto, CA 94304 USA

[8] CALTECH, Downs Lab 220 47, Pasadena, CA 91125 USA

[9] Sci Syst & Applicat Inc, Lanham, MD USA

[10] Univ Michigan, Dept Atmospher Ocean & Space Sci, Ann Arbor, MI 48109 USA

来源：

JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS | 2004年 / 109卷 / A10期

关键词：

solar flares; coronal mass ejections; solar energetic particles; energetics; hard X rays; gamma rays;

D O I：

10.1029/2004JA010571

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Using coordinated observations from instruments on the Advanced Composition Explorer (ACE), the Solar and Heliospheric Observatory (SOHO), and the Ramaty High Energy Solar Spectroscopic Imager (RHESSI), we have evaluated the energetics of two well-observed flare/CME events on 21 April 2002 and 23 July 2002. For each event, we have estimated the energy contents ( and the likely uncertainties) of ( 1) the coronal mass ejection, ( 2) the thermal plasma at the Sun, ( 3) the hard X-ray producing accelerated electrons, ( 4) the gamma-ray producing ions, and ( 5) the solar energetic particles. The results are assimilated and discussed relative to the probable amount of nonpotential magnetic energy available in a large active region.

引用

页数：16

共 55 条

[41] The solar flare 3.8-10 keV X-ray spectrum [J].