Velocity Structure of Bright Points in a Coronal Hole

被引：0

作者：

Kamio, Suguru ^{[1
]}

Hara, Hirohisa ^{[1
]}

Watanabe, Tetsuya ^{[1
]}

Curdt, Werner ^{[2
]}

机构：

[1] Natl Inst Nat Sci, Natl Astron Observ Japan, Hinode Sci Ctr, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan

[2] Max Planck Inst Sonnensyst Forsch MPS, D-37191 Katlenburg Lindau, Germany

来源：

FIRST RESULTS FROM HINODE | 2008年 / 397卷

关键词：

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present the velocity structure of bright points in the corona and in the transition region. This is one of the first results from the coordinated observation with Hinode/EIS and SOHO/SUMER in April 2007. Bright points in the corona are associated with bright patches in the transition region network. The result suggests coronal bright points are rooted in the magnetic field concentration of the network. No clear connection is found between velocities in the corona and the transition region, but observing time difference between EIS and SUMER could be the cause of the dissociation.

引用

页码：35 / +

页数：2

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