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Sökning: WFRF:(Espley J.) > (2020) > Mars' Ionospheric I...

LIBRIS Formathandbok  (Information om MARC21)
FältnamnIndikatorerMetadata
00004125naa a2200445 4500
001oai:DiVA.org:umu-173841
003SwePub
008200803s2020 | |||||||||||000 ||eng|
009oai:DiVA.org:uu-414323
0247 a https://urn.kb.se/resolve?urn=urn:nbn:se:umu:diva-1738412 URI
0247 a https://doi.org/10.1029/2019JA0273442 DOI
0247 a https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-4143232 URI
040 a (SwePub)umud (SwePub)uu
041 a engb eng
042 9 SwePub
072 7a ref2 swepub-contenttype
072 7a art2 swepub-publicationtype
1001 a Sanchez-Cano, Beatrizu Univ Leicester, Dept Phys & Astron, Radio & Space Plasma Phys Grp, Leicester, Leics, England.4 aut
2451 0a Mars' Ionospheric Interaction With Comet C/2013 A1 Siding Spring's Coma at Their Closest Approach as Seen by Mars Express
264 1b American Geophysical Union (AGU),c 2020
338 a print2 rdacarrier
520 a On 19 October 2014, Mars experienced a close encounter with Comet C/2013 A1 Siding Spring. Using data from the Mars Advanced Radar for Subsurface and Ionosphere Sounding (MARSIS) on board Mars Express (MEX), we assess the interaction of the Martian ionosphere with the comet's coma and possibly magnetic tail during the orbit of their closest approach. The topside ionospheric electron density profile is evaluated from the altitude of the peak density of the ionosphere up to the MEX altitude. We find complex and rapid variability in the ionospheric profile along the MEX orbit, not seen even after the impact of a large coronal mass ejection. Before closest approach, large electron density reductions predominate, which could be caused either by comet water damping or comet magnetic field interactions. After closest approach, a substantial electron density rise predominates. Moreover, several extra topside layers are visible along the whole orbit at different altitudes, which could be related to different processes as we discuss.
650 7a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe
650 7a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng
7001 a Lester, Marku Univ Leicester, Dept Phys & Astron, Radio & Space Plasma Phys Grp, Leicester, Leics, England.4 aut
7001 a Witasse, Olivieru European Space Agcy, ESTEC Sci Support Off, Noordwijk, Netherlands.4 aut
7001 a Morgan, David D.u Univ Iowa, Dept Phys & Astron, Iowa City, IA 52242 USA.4 aut
7001 a Opgenoorth, Hermann J.u Umeå universitet,Institutionen för fysik,Radio and Space Plasma Physics Group, Department of Physics and Astronomy, University of Leicester, Leicester, UK,Univ Leicester, Dept Phys & Astron, Radio & Space Plasma Phys Grp, Leicester, Leics, England.;Umea Univ, Dept Phys, Umea, Sweden.4 aut0 (Swepub:umu)heop0005
7001 a Andrews, David J.u Uppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen4 aut0 (Swepub:uu)davan153
7001 a Blelly, Pierre-Louisu Inst Rech Astrophys & Planetol IRAP, Toulouse, France.4 aut
7001 a Cowley, Stanley W. H.u Univ Leicester, Dept Phys & Astron, Radio & Space Plasma Phys Grp, Leicester, Leics, England.4 aut
7001 a Kopf, Andrew J.u Univ Iowa, Dept Phys & Astron, Iowa City, IA 52242 USA.4 aut
7001 a Leblanc, Francoisu Sorbonne Univ, CNRS, UVSQ, LATMOS, Paris, France.4 aut
7001 a Espley, Jared R.u NASA, Goddard Space Flight Ctr, Greenbelt, MD USA.4 aut
7001 a Cardesin-Moinelo, Alejandrou European Space Agcy, ESAC, Madrid, Spain.4 aut
7102 a Univ Leicester, Dept Phys & Astron, Radio & Space Plasma Phys Grp, Leicester, Leics, England.b European Space Agcy, ESTEC Sci Support Off, Noordwijk, Netherlands.4 org
7730 t Journal of Geophysical Research - Space Physicsd : American Geophysical Union (AGU)g 125:1q 125:1x 2169-9380x 2169-9402
8564 8u https://urn.kb.se/resolve?urn=urn:nbn:se:umu:diva-173841
8564 8u https://doi.org/10.1029/2019JA027344
8564 8u https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-414323

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