Current Sheet and Reconnection Inflow-Outflow Observations During Solar Eruptions

被引：0

作者：

Savage, Sabrina L. ^{[1
]}

Holman, Gordon ^{[1
]}

Reeves, Katharine K. ^{[2
]}

Seaton, Daniel B. ^{[3
]}

McKenzie, David E. ^{[4
]}

Su, Yang ^{[1
,5
]}

机构：

[1] NASA, Goddard Space Flight Ctr, Oak Ridge Associated Univ, 8800 Greenbelt Rd,Code 671, Greenbelt, MD 20771 USA

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

[3] SIDC, Royal Observ Belgium, B-1180 Brussels, Belgium

[4] Montana State Univ, Dept Phys, Bozeman, MT 59717 USA

[5] Catholic Univ Amer, Dept Phys, Washington, DC 20064 USA

来源：

FIFTH HINODE SCIENCE MEETING: EXPLORING THE ACTIVE SUN | 2012年 / 456卷

关键词：

SUPRA-ARCADE DOWNFLOWS; CORONAL MASS EJECTIONS; MAGNETIC RECONNECTION; QUANTITATIVE EXAMINATION; PATCHY RECONNECTION; FLARES; MODEL;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Magnetic reconnection is widely accepted as being associated with energy release during solar flares; however, observations of it have been indirect and/or incomplete. Using the suite of instruments available spanning wavelength space, we provide observations and measurements of both the inputs and outputs predicted from reconnection in the form of inflows preceding outflows (i.e. supra-arcade downflows, supra-arcade downflowing loops, upflows, and disconnection events). We also present evidence for current sheets through which reconnection is expected to occur and discuss current sheet motion during flare progression.

引用

页码：169 / +

页数：2

共 37 条

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