Loss-cone instability modulation due to a magnetohydrodynamic sausage mode oscillation in the solar corona

Magnetohydrodynamic (MHD) waves and plasma instabilities can be studied during solar flares. Here the authors show evidence for an MHD sausage mode oscillation periodically triggering electron acceleration at a magnetic null point in the solar corona, indicating MHD oscillations in plasma can indire...

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Autores principales:	Eoin P. Carley, Laura A. Hayes, Sophie A. Murray, Diana E. Morosan, Warren Shelley, Nicole Vilmer, Peter T. Gallagher
Formato:	article
Lenguaje:	EN
Publicado:	Nature Portfolio 2019
Materias:	Science Q
Acceso en línea:	https://doaj.org/article/9c969785775d49cf8ae452955fd3945e
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spelling	oai:doaj.org-article:9c969785775d49cf8ae452955fd3945e2021-12-02T14:40:18ZLoss-cone instability modulation due to a magnetohydrodynamic sausage mode oscillation in the solar corona10.1038/s41467-019-10204-12041-1723https://doaj.org/article/9c969785775d49cf8ae452955fd3945e2019-05-01T00:00:00Zhttps://doi.org/10.1038/s41467-019-10204-1https://doaj.org/toc/2041-1723Magnetohydrodynamic (MHD) waves and plasma instabilities can be studied during solar flares. Here the authors show evidence for an MHD sausage mode oscillation periodically triggering electron acceleration at a magnetic null point in the solar corona, indicating MHD oscillations in plasma can indirectly lead to loss-cone instability modulation.Eoin P. CarleyLaura A. HayesSophie A. MurrayDiana E. MorosanWarren ShelleyNicole VilmerPeter T. GallagherNature PortfolioarticleScienceQENNature Communications, Vol 10, Iss 1, Pp 1-12 (2019)
institution	DOAJ
collection	DOAJ
language	EN
topic	Science Q
spellingShingle	Science Q Eoin P. Carley Laura A. Hayes Sophie A. Murray Diana E. Morosan Warren Shelley Nicole Vilmer Peter T. Gallagher Loss-cone instability modulation due to a magnetohydrodynamic sausage mode oscillation in the solar corona
description	Magnetohydrodynamic (MHD) waves and plasma instabilities can be studied during solar flares. Here the authors show evidence for an MHD sausage mode oscillation periodically triggering electron acceleration at a magnetic null point in the solar corona, indicating MHD oscillations in plasma can indirectly lead to loss-cone instability modulation.
format	article
author	Eoin P. Carley Laura A. Hayes Sophie A. Murray Diana E. Morosan Warren Shelley Nicole Vilmer Peter T. Gallagher
author_facet	Eoin P. Carley Laura A. Hayes Sophie A. Murray Diana E. Morosan Warren Shelley Nicole Vilmer Peter T. Gallagher
author_sort	Eoin P. Carley
title	Loss-cone instability modulation due to a magnetohydrodynamic sausage mode oscillation in the solar corona
title_short	Loss-cone instability modulation due to a magnetohydrodynamic sausage mode oscillation in the solar corona
title_full	Loss-cone instability modulation due to a magnetohydrodynamic sausage mode oscillation in the solar corona
title_fullStr	Loss-cone instability modulation due to a magnetohydrodynamic sausage mode oscillation in the solar corona
title_full_unstemmed	Loss-cone instability modulation due to a magnetohydrodynamic sausage mode oscillation in the solar corona
title_sort	loss-cone instability modulation due to a magnetohydrodynamic sausage mode oscillation in the solar corona
publisher	Nature Portfolio
publishDate	2019
url	https://doaj.org/article/9c969785775d49cf8ae452955fd3945e
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Loss-cone instability modulation due to a magnetohydrodynamic sausage mode oscillation in the solar corona

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