Identification of Pre-flare Processes and Their Possible Role in Driving a Large-scale Flux Rope Eruption with Complex M-class Flare in the Active Region NOAA 12371-Reference-Cited by-同舟云学术

Identification of Pre-flare Processes and Their Possible Role in Driving a Large-scale Flux Rope Eruption with Complex M-class Flare in the Active Region NOAA 12371

Published:2020-02 Issue:2 Volume:295 Page:
ISSN:0038-0938
Container-title:Solar Physics
language:en
Short-container-title:Sol Phys

Author:

Mitra Prabir K.^ORCID,Joshi Bhuwan^ORCID,Prasad Avijeet^ORCID

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://link.springer.com/content/pdf/10.1007/s11207-020-1596-2.pdf

Reference79 articles.

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3. Bi, Y., Yang, J., Jiang, Y., Hong, J., Xu, Z., Qu, Z., Ji, K.: 2017, The photospheric vortex flows during a solar flare. Astrophys. J. Lett.849(2), L35. DOI . ADS .

4. Carmichael, H.: 1964, A process for flares. NASA Spec. Publ.50, 451. ADS .

5. Cheng, X., Ding, M.D.: 2016, Spectroscopic diagnostics of solar magnetic flux ropes using iron forbidden line. Astrophys. J. Lett.823(1), L4. DOI . ADS .

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