Simulation of Mercury's magnetosheath with a combined hybrid-paraboloid model

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dc.contributor Aalto-yliopisto fi
dc.contributor Aalto University en
dc.contributor.author Parunakian, David
dc.contributor.author Dyadechkin, Sergey
dc.contributor.author Alexeev, Igor
dc.contributor.author Belenkaya, Elena
dc.contributor.author Khodachenko, Maxim
dc.contributor.author Kallio, Esa
dc.contributor.author Alho, Markku
dc.date.accessioned 2017-11-21T13:35:39Z
dc.date.available 2017-11-21T13:35:39Z
dc.date.issued 2017-08-01
dc.identifier.citation Parunakian , D , Dyadechkin , S , Alexeev , I , Belenkaya , E , Khodachenko , M , Kallio , E & Alho , M 2017 , ' Simulation of Mercury's magnetosheath with a combined hybrid-paraboloid model ' Journal of Geophysical Research: Space Physics , vol 122 , no. 8 , pp. 8310-8326 . DOI: 10.1002/2017JA024105 en
dc.identifier.issn 2169-9380
dc.identifier.issn 2169-9402
dc.identifier.other PURE UUID: 3f91a20f-317f-421e-b106-b8733a773a24
dc.identifier.other PURE ITEMURL: https://research.aalto.fi/en/publications/simulation-of-mercurys-magnetosheath-with-a-combined-hybridparaboloid-model(3f91a20f-317f-421e-b106-b8733a773a24).html
dc.identifier.other PURE LINK: http://www.scopus.com/inward/record.url?scp=85029914539&partnerID=8YFLogxK
dc.identifier.other PURE FILEURL: https://research.aalto.fi/files/15729640/Parunakian_et_al_2017_Journal_of_Geophysical_Research_Space_Physics.pdf
dc.identifier.uri https://aaltodoc.aalto.fi/handle/123456789/28782
dc.description.abstract In this paper we introduce a novel approach for modeling planetary magnetospheres that involves a combination of the hybrid model and the paraboloid magnetosphere model (PMM); we further refer to it as the combined hybrid model. While both of these individual models have been successfully applied in the past, their combination enables us both to overcome the traditional difficulties of hybrid models to develop a self-consistent magnetic field and to compensate the lack of plasma simulation in the PMM. We then use this combined model to simulate Mercury's magnetosphere and investigate the geometry and configuration of Mercury's magnetosheath controlled by various conditions in the interplanetary medium. The developed approach provides a unique comprehensive view of Mercury's magnetospheric environment for the first time. Using this setup, we compare the locations of the bow shock and the magnetopause as determined by simulations with the locations predicted by stand-alone PMM runs and also verify the magnetic and dynamic pressure balance at the magnetopause. We also compare the results produced by these simulations with observational data obtained by the magnetometer on board the MErcury Surface, Space ENvironment, GEochemistry, and Ranging (MESSENGER) spacecraft along a dusk-dawn orbit and discuss the signatures of the magnetospheric features that appear in these simulations. Overall, our analysis suggests that combining the semiempirical PMM with a self-consistent global kinetic model creates new modeling possibilities which individual models cannot provide on their own. en
dc.format.extent 17
dc.format.extent 8310-8326
dc.format.mimetype application/pdf
dc.language.iso en en
dc.relation.ispartofseries Journal of Geophysical Research: Space Physics en
dc.relation.ispartofseries Volume 122, issue 8 en
dc.rights openAccess en
dc.subject.other Geophysics en
dc.subject.other Oceanography en
dc.subject.other Forestry en
dc.subject.other Ecology en
dc.subject.other Aquatic Science en
dc.subject.other Water Science and Technology en
dc.subject.other Soil Science en
dc.subject.other Geochemistry and Petrology en
dc.subject.other Earth-Surface Processes en
dc.subject.other Atmospheric Science en
dc.subject.other Earth and Planetary Sciences (miscellaneous) en
dc.subject.other Space and Planetary Science en
dc.subject.other Palaeontology en
dc.subject.other 115 Astronomy and space science en
dc.title Simulation of Mercury's magnetosheath with a combined hybrid-paraboloid model en
dc.type A1 Alkuperäisartikkeli tieteellisessä aikakauslehdessä fi
dc.description.version Peer reviewed en
dc.contributor.department Lomonosov Moscow State University
dc.contributor.department Department of Electronics and Nanoengineering
dc.subject.keyword Hermean magnetosphere
dc.subject.keyword hybrid model
dc.subject.keyword magnetosheath
dc.subject.keyword MESSENGER
dc.subject.keyword semiempirical model
dc.subject.keyword Geophysics
dc.subject.keyword Oceanography
dc.subject.keyword Forestry
dc.subject.keyword Ecology
dc.subject.keyword Aquatic Science
dc.subject.keyword Water Science and Technology
dc.subject.keyword Soil Science
dc.subject.keyword Geochemistry and Petrology
dc.subject.keyword Earth-Surface Processes
dc.subject.keyword Atmospheric Science
dc.subject.keyword Earth and Planetary Sciences (miscellaneous)
dc.subject.keyword Space and Planetary Science
dc.subject.keyword Palaeontology
dc.subject.keyword 115 Astronomy and space science
dc.identifier.urn URN:NBN:fi:aalto-201711217603
dc.identifier.doi 10.1002/2017JA024105
dc.type.version publishedVersion


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