The Emergence of Magnetic Field into Stellar Atmospheres

Bibcode
2004Ap&SS.292..587M
DOI
10.1023/B:ASTR.0000045065.79067.a1
Moreno-Insertis, F.
Bibliographical reference

Astrophysics and Space Science, v. 292, Issue 1, p. 587-597 (2004).

Advertised on:
8
2004
Journal
Astrophysics and Space Science
Number of authors
1
IAC number of authors
1
Citations
4
Refereed citations
3
Description
The magnetic activity in the atmosphere of the Sun, possibly of most other magnetically active late-type stars, is a consequence of the emergence of magnetic flux from the stellar interior. Research in this field has to consider the rise of magnetized plasma from the depths of the convective envelope through the stellar surface and out across the corona. In the present review, a number of key questions, difficulties and results are discussed.
Type
Non-refereed
Stellar atmospheres

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