Magnetohydrodynamic waves in the partially ionized solar plasma

dc.contributor.author	Soler, R.
dc.date.accessioned	2024-09-17T11:59:03Z
dc.date.available	2024-09-17T11:59:03Z
dc.identifier.uri	http://hdl.handle.net/11201/166124
dc.description.abstract	<p>[eng] This paper provides a comprehensive review of recent theoretical investigations concerning magnetohydrodynamic (MHD) waves in partially ionized solar plasma. First, we examine the properties of linear MHD waves in a uniform partially ionized plasma and discuss the relevant effects arising from partial ionization. Subsequently, we delve into MHD wave studies in the more intricate settings of the lower solar atmosphere and solar prominences. These investigations involve topics such as MHD waves in magnetic flux tubes, wave excitation, linear and nonlinear mode coupling and wave heating. We outline new challenges that future research should tackle. </p>
dc.format	application/pdf
dc.relation.isformatof	https://doi.org/https://doi.org/10.1098/rsta.2023.0223
dc.relation.ispartof	2024, vol. 382
dc.rights	, 2024
dc.subject.classification	52 - Astronomia. Astrofísica. Investigació espacial. Geodèsia
dc.subject.other	52 - Astronomy. Astrophysics. Space research. Geodesy
dc.title	Magnetohydrodynamic waves in the partially ionized solar plasma
dc.type	info:eu-repo/semantics/article
dc.type	info:eu-repo/semantics/
dc.date.updated	2024-09-17T11:59:04Z
dc.rights.accessRights	info:eu-repo/semantics/openAccess
dc.identifier.doi	https://doi.org/https://doi.org/10.1098/rsta.2023.0223