Statistical study of the reconnection rate in solar flares

被引：0

作者：

Isobe, H ^{[1
]}

Morimoto, T ^{[1
]}

Eto, S ^{[1
]}

Narukage, N ^{[1
]}

Shibata, K ^{[1
]}

机构：

[1] Kyoto Univ, Kwasan Observ, Kyoto 6078417, Japan

来源：

MULTI-WAVELENGTH OBSERVATIONS OF CORONAL STRUCTURE AND DYNAMICS | 2002年 / 13卷

关键词：

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Reconnection rate defined by (inflow velocity)/(Alfven velocity) is one of the key parameters for understanding the physics of magnetic reconnection. In this paper we utilize the method for determining the reconnection rate from observational data suggested by Isobe et al. (2002) for 7 solar flares and 2 giant arcades. We have found that the reconnection rate is 0.001-0.2, which is consistent with the fast reconnection model by Petschek.

引用

页码：171 / 172

页数：2

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