Quasi-Periodic Pulsations in Solar and Stellar Flares: A Review of Underpinning Physical Mechanisms and Their Predicted Observational Signatures-Reference-Cited by-同舟云学术

Quasi-Periodic Pulsations in Solar and Stellar Flares: A Review of Underpinning Physical Mechanisms and Their Predicted Observational Signatures

Published:2021-07-19 Issue:5 Volume:217 Page:
ISSN:0038-6308
Container-title:Space Science Reviews
language:en
Short-container-title:Space Sci Rev

Author:

Zimovets I. V.^ORCID,McLaughlin J. A.^ORCID,Srivastava A. K.^ORCID,Kolotkov D. Y.^ORCID,Kuznetsov A. A.^ORCID,Kupriyanova E. G.^ORCID,Cho I.-H.^ORCID,Inglis A. R.^ORCID,Reale F.^ORCID,Pascoe D. J.^ORCID,Tian H.,Yuan D.^ORCID,Li D.^ORCID,Zhang Q. M.

Funder

budgetary funding of Basic Research program

UK Science and Technology Facilities Council

budgetary funding of Basic Research program II.16

National Natural Science Foundation of China

Shenzhen Technology Project

National Research Foundation of Korea

Korea Astronomy and Space Science Institute

European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme

Internal Funds KU Leuven

Russian Science Foundation

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://link.springer.com/content/pdf/10.1007/s11214-021-00840-9.pdf

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5. S. Anfinogentov, V.M. Nakariakov, Motion magnification in coronal seismology. Sol. Phys. 291(11), 3251–3267 (2016). https://doi.org/10.1007/s11207-016-1013-z. arXiv:1611.01790

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