Study of ribbon separation and magnetic reconnection rates

Document Type

Conference Proceeding

Publication Date

8-1-2012

Abstract

We study the correlation between the speed of two-ribbon separation and the magnetic flux density during the 2001 April 10 solar flare. A weak negative correlation is found between the ribbon separation speed (Vr ) and the longitudinal magnetic flux density (Bz ). In addition, we estimate the magnetic reconnection rate (Erec ). Along the flare ribbons, Erec fluctuates in the small range except near the HXR source. The localized enhancement of the reconnection rate corresponds to the position of the HXR source. © International Astronomical Union 2013.

Identifier

84880555295 (Scopus)

ISBN

[9781107033832]

Publication Title

Proceedings of the International Astronomical Union

External Full Text Location

https://doi.org/10.1017/S1743921313003323

e-ISSN

17439221

ISSN

17439213

First Page

585

Last Page

586

Issue

S294

Volume

8

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