FRiED : A Novel Three-dimensional Model of Coronal Mass Ejections

Show simple item record Isavnin, A. 2017-05-10T07:48:02Z 2017-05-10T07:48:02Z 2016
dc.identifier.citation Isavnin , A 2016 , ' FRiED : A Novel Three-dimensional Model of Coronal Mass Ejections ' , Astrophysical Journal , vol. 833 , no. 2 , 265 .
dc.identifier.other PURE: 79207810
dc.identifier.other PURE UUID: cae4165b-4259-46f5-b101-149fb85e0149
dc.identifier.other Bibtex: urn:b308d2a763d4dbe8e65f213de5d10203
dc.identifier.other Scopus: 85007591724
dc.identifier.other WOS: 000391169600142
dc.identifier.other ORCID: /0000-0002-7178-627X/work/29993955
dc.description.abstract We present a novel three-dimensional (3D) model of coronal mass ejections (CMEs) that unifies all key evolutionary aspects of CMEs and encapsulates their 3D magnetic field configuration. This fully analytic model is capable of reproducing the global geometrical shape of a CME with all major deformations taken into account, i.e., deflection, rotation, expansion, “pancaking,” front flattening, and rotational skew. Encapsulation of 3D magnetic structure allows the model to reproduce in-situ measurements of magnetic field for trajectories of spacecraft-CME encounters of any degree of complexity. As such, the model can be used single-handedly for the consistent analysis of both remote and in-situ observations of CMEs at any heliocentric distance. We demonstrate the latter by successfully applying the model for the analysis of two CMEs. en
dc.format.extent 10
dc.language.iso eng
dc.relation.ispartof Astrophysical Journal
dc.rights unspecified
dc.rights.uri info:eu-repo/semantics/openAccess
dc.subject 114 Physical sciences
dc.title FRiED : A Novel Three-dimensional Model of Coronal Mass Ejections en
dc.type Article
dc.contributor.organization Department of Physics
dc.description.reviewstatus Peer reviewed
dc.relation.issn 0004-637X
dc.rights.accesslevel openAccess
dc.type.version publishedVersion

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