FINE MAGNETIC STRUCTURE AND ORIGIN OF COUNTER-STREAMING MASS FLOWS IN A QUIESCENT SOLAR PROMINENCE-Reference-Cited by-同舟云学术

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FINE MAGNETIC STRUCTURE AND ORIGIN OF COUNTER-STREAMING MASS FLOWS IN A QUIESCENT SOLAR PROMINENCE

Published:2015-11-19 Issue:1 Volume:814 Page:L17
ISSN:2041-8213
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Shen Yuandeng,Liu Yu,Liu Ying D.,Chen P. F.,Su Jiangtao,Xu Zhi,Liu Zhong

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.1088/2041-8205/814/1/L17/pdf

Reference51 articles.

1. PATTERNS OF FLOWS IN AN INTERMEDIATE PROMINENCE OBSERVED BYHINODE

2. Coronal Mass Ejection: Initiation, Magnetic Helicity, and Flux Ropes. II. Turbulent Diffusion–driven Evolution

3. Prominence Magnetic Dips in Three-dimensional Sheared Arcades

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