Observations of Shock Propagation through Turbulent Plasma in the Solar Corona-Reference-Cited by-同舟云学术

Observations of Shock Propagation through Turbulent Plasma in the Solar Corona

Published:2021-10-26 Issue:1 Volume:921 Page:3
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Carley Eoin P.^ORCID,Cecconi Baptiste^ORCID,Reid Hamish A.^ORCID,Briand Carine^ORCID,Raja K. Sasikumar^ORCID,Masson Sophie^ORCID,Dorovskyy Vladimir^ORCID,Tiburzi Caterina^ORCID,Vilmer Nicole^ORCID,Zucca Pietro^ORCID,Zarka Philippe^ORCID,Tagger Michel^ORCID,Grießmeier Jean-Mathias^ORCID,Corbel Stéphane^ORCID,Theureau Gilles^ORCID,Loh Alan^ORCID,Girard Julien N.^ORCID

Funder

Dublin Institute for Advanced Studies

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.3847/1538-4357/ac1acd/pdf

Reference63 articles.

1. Relationship between Magnetic Power Spectrum and Flare Productivity in Solar Active Regions

2. Fibre structure of decametric type II radio bursts as a manifestation of emission propagation effects in a disturbed near-solar plasma

3. Detection of spike-like structures near the front of type-II bursts

4. Observations of field-aligned density fluctuations in the inner solar wind

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3. Turbulence in Sources of Decimetric Flare Continua;Solar Physics;2023-08

4. Morphology of Solar Type II Bursts Caused by Shock Propagation through Turbulent and Inhomogeneous Coronal Plasma;The Astrophysical Journal;2023-07-01

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