The automatic processing and analysis of solar image sequences

被引：1
|
作者：
Persiantsev I.G. [1 ]
Ryazanov A.Yu. [1 ]
Shugai Ju.S. [1 ]
机构：
[1] Skobel'tsyn Institute of Nuclear Physics, Moscow State University, Vorob'evy gory, Moscow
来源：
Pattern Recognition and Image Analysis | 2006年 / 16卷 / 1期
关键词：
Solar Wind; Coronal Hole; Geomagnetic Storm; Solar Wind Velocity; Central Meridian;
D O I：
10.1134/S1054661806010093
中图分类号：
学科分类号：
摘要：
An algorithm for the analysis of sequential images of the Sun is presented and tested with the imagery obtained by the SOHO satellite. In the context of space weather monitoring, it is interesting to reveal the sources of fast solar wind on the surface of the Sun. Examples of such sources are coronal holes, which may cause a fast flow of solar wind when crossing the central meridian of the Sun. The proposed algorithm determines the area and location of coronal holes. The calculated dynamics of the hole areas and of the observed solar wind velocity are compared from August 1 to December 31, 2003. © Pleiades Publishing, Inc., 2006.
引用
收藏
页码：30 / 32
页数：2
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