Non-thermal processes in coronae and beyond

被引：1

作者：

Poppenhaeger, K. ^{[1
]}

Guenther, H. M. ^{[1
]}

Beiersdorfer, P. ^{[2
]}

Brickhouse, N. S. ^{[1
]}

Carter, J. A. ^{[3
]}

Hudson, H. S. ^{[4
]}

Kowalski, A. ^{[5
]}

Lalitha, S. ^{[6
]}

Miceli, M. ^{[7
]}

Wolk, S. J. ^{[1
]}

机构：

[1] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA

[2] Lawrence Livermore Natl Lab, Livermore, CA 94550 USA

[3] Univ Leicester, Dept Phys & Astron, Leicester LE1 7RH, Leics, England

[4] Univ Calif Berkeley, SSL, Berkeley, CA USA

[5] Univ Washington, Dept Astron, Seattle, WA 98195 USA

[6] Hamburger Sternwarte, D-21029 Hamburg, Germany

[7] Univ Palermo, Dipartimento Fis, I-90134 Palermo, Italy

来源：

ASTRONOMISCHE NACHRICHTEN | 2013年 / 334卷 / 1-2期

关键词：

atomic data; methods: laboratory; radiation mechanism: non-thermal; stars: flare; Sun: flares; ATOMIC DATABASE; EMISSION; CHIANTI; PLASMA; IONS;

D O I：

10.1002/asna.201211755

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

This contribution summarizes the splinter session "Non-thermal processes in coronae and beyond" held at the Cool Stars 17 workshop in Barcelona in 2012. It covers new developments in high energy non-thermal effects in the Earth's exosphere, solar and stellar flares, the diffuse emission in star forming regions and reviews the state and the challenges of the underlying atomic databases. (C) 2013 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim

引用

页码：101 / 104

页数：4

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