CHARACTERISTICS OF THE PHOTOSPHERIC MAGNETIC FIELD ASSOCIATED WITH SOLAR FLARE INITIATION-Reference-Cited by-同舟云学术

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CHARACTERISTICS OF THE PHOTOSPHERIC MAGNETIC FIELD ASSOCIATED WITH SOLAR FLARE INITIATION

Published:2014-04-16 Issue:1 Volume:786 Page:72
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Yang Ya-Hui^ORCID,Chen P. F.^ORCID,Hsieh Min-Shiu,Wu S. T.^ORCID,He Han,Tsai Tsung-Che

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/786/i=1/a=72/pdf

Reference72 articles.

Cited by 17 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Desaturated EUV Flare Ribbons in an X-class Flare;The Astrophysical Journal;2021-03-01

2. Magnetohydrodynamic Simulation of Magnetic Null-point Reconnections and Coronal Dimmings during the X2.1 Flare in NOAA AR 11283;The Astrophysical Journal;2020-11-10

3. Chirality and magnetic configuration associated with two-ribbon solar flares: AR 10930 versus AR 11158;Advances in Space Research;2020-06

4. Electric Current Evolution at the Footpoints of Solar Eruptions;The Astrophysical Journal;2020-05-20

5. Comparison analysis of current helicity inferred from several solar vector magnetographs;SCIENTIA SINICA Physica, Mechanica & Astronomica;2019-10-23

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