Emergence of Magnetic Flux Generated in a Solar Convective Dynamo. I. The Formation of Sunspots and Active Regions, and The Origin of Their Asymmetries-Reference-Cited by-同舟云学术

Emergence of Magnetic Flux Generated in a Solar Convective Dynamo. I. The Formation of Sunspots and Active Regions, and The Origin of Their Asymmetries

Published:2017-09-12 Issue:2 Volume:846 Page:149
ISSN:1538-4357
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Chen Feng^ORCID,Rempel Matthias^ORCID,Fan Yuhong^ORCID

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/846/i=2/a=149/pdf

Reference93 articles.

1. The Magnetic Connection between the Convection Zone and Corona in the Quiet Sun

2. Emergence of magnetic flux from the convection zone into the corona

3. GRAND MINIMA AND EQUATORWARD PROPAGATION IN A CYCLING STELLAR CONVECTIVE DYNAMO

4. The effects of vigorous mixing in a convective model of zonal flow on the ice giants

5. HELIOSEISMOLOGY OF PRE-EMERGING ACTIVE REGIONS. II. AVERAGE EMERGENCE PROPERTIES

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