Large solar flares and coronal mass ejections: Their manifestations in the chromosphere

被引：0

作者：

V. I. Sidorov

S. A. Yazev

机构：

[1] Irkutsk State University,Astronomical Observatory

[2] Russian Academy of Sciences,Institute of Solar

来源：

Geomagnetism and Aeronomy | 2009年 / 49卷

关键词：

Flare; Coronal Mass Ejection; Solar Flare; Current Layer; Coronal Magnetic Field;

D O I：

暂无

中图分类号：

学科分类号：

摘要：

A phenomenological model of a united (solar flare-coronal mass ejection (CME)) event is briefly described. The model is based on the analysis of the images of the development of some events in various spectral ranges. A modified classification of the chomospheric manifestations of the event is proposed. A phenomenological model describing phenomena in the process of the development of intense solar flare-CME events in the activity complexes on the Sun is briefly presented. The model is based on the analysis of the observation data for some major flares (May 16, 1981, October 19, 2001, July 23, 2002).

引用

页码：1076 / 1079

页数：3

共 11 条

[1]

Dulk G. A.(1978)Coronal Magnetic Fields Solar Phys. 57 279-295

[2]

McLean D. J.(2004)Acceleration and Heating Processes in a Collapsing Magnetic Trap Astron. Astrophys. 419 1159-1168

[3]

Karlicky M.(2001)3D Coronal Structures and Their Evolutions Measured by Stereoscopy, Consequences for Space Wather and the Stereo Mission Space Sci. Rev. 97 51-54

[4]

Kosugi T.(2004)Magnetic Field, Hα, and RHESSI Observation of the July 23, 2002 Gamma-Ray Flare Ap. J. 605 546-553

[5]

Portier-Fozzani F.(2008)Coronal Magnetic Arcs Usp. Fiz. Nauk 178 1165-1204

[6]

Inhester B.(undefined)undefined undefined undefined undefined-undefined

[7]

Yurchyshyn V. H.(undefined)undefined undefined undefined undefined-undefined

[8]

Wang V.(undefined)undefined undefined undefined undefined-undefined

[9]

Abramenko V. V.(undefined)undefined undefined undefined undefined-undefined

[10]

Zaitsev A. V.(undefined)undefined undefined undefined undefined-undefined

← 1 2 →