Formation of Solar Magnetic Flux Tubes with Kilogauss Field Strength Induced by Convective Instability-Reference-Cited by-同舟云学术

Formation of Solar Magnetic Flux Tubes with Kilogauss Field Strength Induced by Convective Instability

Published:2008-03-19 Issue:2 Volume:677 Page:L145-L147
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Nagata Shin'ichi,Tsuneta Saku,Suematsu Yoshinori,Ichimoto Kiyoshi,Katsukawa Yukio,Shimizu Toshifumi,Yokoyama Takaaki,Tarbell Theodore D.,Lites Bruce W.,Shine Richard A.,Berger Thomas E.,Title Alan M.,Bellot Rubio Luis R.,Orozco Suárez David

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference24 articles.

1. Observation of Convective Collapse and Upward‐moving Shocks in the Quiet Sun

2. On the Dynamics of Small-Scale Solar Magnetic Elements

3. Convection and magnetic fields in stars

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