Multiple regions of shock-accelerated particles during a solar coronal mass ejection

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http://hdl.handle.net/10138/326624

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Morosan , D E , Carley , E P , Hayes , L A , Murray , S A , Zucca , P , Fallows , R A , McCauley , J , Kilpua , E K J , Mann , G , Vocks , C & Gallagher , P T 2019 , ' Multiple regions of shock-accelerated particles during a solar coronal mass ejection ' , Nature Astronomy , vol. 3 , no. 5 , pp. 452-461 . https://doi.org/10.1038/s41550-019-0689-z

Title: Multiple regions of shock-accelerated particles during a solar coronal mass ejection
Author: Morosan, Diana E.; Carley, Eoin P.; Hayes, Laura A.; Murray, Sophie A.; Zucca, Pietro; Fallows, Richard A.; McCauley, Joe; Kilpua, Emilia K. J.; Mann, Gottfried; Vocks, Christian; Gallagher, Peter T.
Contributor organization: Space Physics Research Group
Particle Physics and Astrophysics
Department of Physics
Date: 2019-05
Language: eng
Number of pages: 10
Belongs to series: Nature Astronomy
ISSN: 2397-3366
DOI: https://doi.org/10.1038/s41550-019-0689-z
URI: http://hdl.handle.net/10138/326624
Abstract: The Sun is an active star that can launch large eruptions of magnetized plasma into the heliosphere, known as corona! mass ejections (CMEs). These can drive shocks that accelerate particles to high energies, often resulting in radio emission at low frequencies (
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115 Astronomy, Space science
Peer reviewed: Yes
Rights: unspecified
Usage restriction: openAccess
Self-archived version: acceptedVersion


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