The Flare on December 13, 2006 and the Standard Solar Flare Model

被引：0
|
作者：
Shibasaki, Kiyoto [1 ]
机构：
[1] Natl Inst Nat Sci, Natl Astron Observ Japan, Nobeyama Solar Radio Observ, Minamisa Ku, Minamimaki, Nagano 3841305, Japan
来源：
HINODE-3: THE 3RD HINODE SCIENCE MEETING | 2012年 / 454卷
关键词：
HINODE MISSION; TELESCOPE; NOBEYAMA; EMISSION; SHEAR;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The solar flare on December 13, 2006 was well observed by Hinode, Nobeyama Radioheliograph and other instruments. In this work, these observations are used to test applicability of the standard solar flare model. This flare contains various elements (Neupert effect, two ribbons, cusp structure, etc.) which are expected from the standard model. Each element is tested whether it really supports the model or not using high cadence multi-wavelength datasets. It is shown that these elements do not necessarily support the model.
引用
收藏
页码：315 / 320
页数：6
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