Solar flares: observations vs simulations

被引:0
|
作者
da Costa, Fatima Rubio [1 ]
Zuccarello, Francesca [1 ]
Labrosse, Nicolas
Fletcher, Lyndsay
Prosecky, Tomas
Kasparova, Jana
机构
[1] Dipartimento Fis & Astron, I-95123 Catania, Italy
来源
ADVANCES IN PLASMA ASTROPHYSICS | 2011年 / 274期
关键词
Methods: numerical; radiative transfer; Sun: atmosphere; Sun: flares;
D O I
10.1017/S1743921311006880
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In order to study the properties of faint, moderate and bright flares, we simulate the conditions of the solar atmosphere using a radiative hydrodynamic model (Abbett & Hawley, 1999). A constant beam of non-thermal electrons is injected at the apex of a 1D coronal loop and heating from thermal soft X-ray emission is included. We compare the results with some observational data in Ly-alpha (using TRACE 1216 and 1600 angstrom data and estimating the "pure" Ly-alpha emission) and in H alpha (data taken with a Multichannel Flare Spectrograph, at the Ondrejov Observatory).
引用
收藏
页码:182 / 184
页数:3
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