Coronal heating, spicules, and Solar-B

被引：0

作者：

Moore, RL ^{[1
]}

Falconer, DA ^{[1
]}

Porter, JG ^{[1
]}

Hathaway, DI ^{[1
]}

Yamauchi, Y ^{[1
]}

Rabin, DM ^{[1
]}

机构：

[1] NASA, George C Marshall Space Flight Ctr, Huntsville, AL 35812 USA

来源：

Solar-B Mission and the Forefront of Solar Physics, Proceedings | 2004年 / 325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 summarize certain observations of coronal luminosity, network magnetic flux, spicules, and macrospicules. These observations together imply that in quiet regions that are not influenced by active regions the coronal heating comes from magnetic activity in the edges of the network flux, possibly from explosions of sheared core fields around granule-sized inclusions of opposite-polarity flux. This scenario can be tested by Solar-B.

引用

页码：283 / 288

页数：6

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