Radial Evolution of Magnetic Field Fluctuations in an Interplanetary Coronal Mass Ejection Sheath

Show simple item record

dc.contributor.author Good, S. W.
dc.contributor.author Ala-Lahti, M.
dc.contributor.author Palmerio, E.
dc.contributor.author Kilpua, E. K. J.
dc.contributor.author Osmane, A.
dc.date.accessioned 2021-04-20T21:52:51Z
dc.date.available 2021-12-18T03:45:52Z
dc.date.issued 2020-04
dc.identifier.citation Good , S W , Ala-Lahti , M , Palmerio , E , Kilpua , E K J & Osmane , A 2020 , ' Radial Evolution of Magnetic Field Fluctuations in an Interplanetary Coronal Mass Ejection Sheath ' , Astrophysical Journal , vol. 893 , no. 2 , 110 . https://doi.org/10.3847/1538-4357/ab7fa2
dc.identifier.other PURE: 137140764
dc.identifier.other PURE UUID: 8ecd27c6-d2b7-4ad7-bde0-10038955cd06
dc.identifier.other WOS: 000529238000001
dc.identifier.other ORCID: /0000-0002-4489-8073/work/74069487
dc.identifier.other ORCID: /0000-0001-6590-3479/work/74070645
dc.identifier.other ORCID: /0000-0002-4921-4208/work/74070730
dc.identifier.other ORCID: /0000-0001-9574-339X/work/74070800
dc.identifier.uri http://hdl.handle.net/10138/329216
dc.description.abstract The sheaths of compressed solar wind that precede interplanetary coronal mass ejections (ICMEs) commonly display large-amplitude magnetic field fluctuations. As ICMEs propagate radially from the Sun, the properties of these fluctuations may evolve significantly. We have analyzed magnetic field fluctuations in an ICME sheath observed by MESSENGER at 0.47 au and subsequently by STEREO-B at 1.08 au while the spacecraft were close to radial alignment. Radial changes in fluctuation amplitude, compressibility, inertial-range spectral slope, permutation entropy, Jensen-Shannon complexity, and planar structuring are characterized. These changes are discussed in relation to the evolving turbulent properties of the upstream solar wind, the shock bounding the front of the sheath changing from a quasi-parallel to quasi-perpendicular geometry, and the development of complex structures in the sheath plasma. 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 Solar wind
dc.subject Interplanetary magnetic fields
dc.subject Interplanetary turbulence
dc.subject SOLAR-WIND TURBULENCE
dc.subject DRIVEN
dc.subject WAVES
dc.subject EARTH
dc.subject 115 Astronomy, Space science
dc.title Radial Evolution of Magnetic Field Fluctuations in an Interplanetary Coronal Mass Ejection Sheath en
dc.type Article
dc.contributor.organization Particle Physics and Astrophysics
dc.contributor.organization Space Physics Research Group
dc.contributor.organization Department of Physics
dc.description.reviewstatus Peer reviewed
dc.relation.doi https://doi.org/10.3847/1538-4357/ab7fa2
dc.relation.issn 0004-637X
dc.rights.accesslevel openAccess
dc.type.version acceptedVersion

Files in this item

Total number of downloads: Loading...

Files Size Format View
2003.05760_1.pdf 2.850Mb PDF View/Open

This item appears in the following Collection(s)

Show simple item record