The Double Structure of the Coronal Streamer Belt

被引：0

作者：

M. V. Eselevich

V. G. Eselevich

机构：

[1] Institute of Solar-Terrestrial Physics,

来源：

Solar Physics | 2006年 / 235卷

关键词：

Physical Process; Streamer Belt; Belt Structure; Coronal Streamer; Double Structure;

D O I：

暂无

中图分类号：

学科分类号：

摘要：

Increasing the effective spatial resolution when analyzing LASCO-C2/SOHO data helped to reveal the existence of double-ray structure in the streamer belt, both in the absence and presence of belt bends. Streamer-belt rays located in the plane of the sky are demonstrated to deviate poleward (north- and southward, respectively, in the N and S hemispheres) at distances R < 4{–}5R⊙ from the Sun center. These new results concerning streamer belt structure are important as the basis for checking a theory claiming to adequately describe physical processes in the corona.

引用

页码：331 / 344

页数：13

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