Dayside Transient Phenomena and Their Impact on the Magnetosphere and Ionosphere

dc.contributorAalto-yliopistofi
dc.contributorAalto Universityen
dc.contributor.authorZhang, Huien_US
dc.contributor.authorZong, Qiugangen_US
dc.contributor.authorConnor, Hyunjuen_US
dc.contributor.authorDelamere, Peteren_US
dc.contributor.authorFacskó, Gáboren_US
dc.contributor.authorHan, Deshengen_US
dc.contributor.authorHasegawa, Hiroshien_US
dc.contributor.authorKallio, Esaen_US
dc.contributor.authorKis, Árpáden_US
dc.contributor.authorLe, Guanen_US
dc.contributor.authorLembège, Bertranden_US
dc.contributor.authorLin, Yuen_US
dc.contributor.authorLiu, Terryen_US
dc.contributor.authorOksavik, Kjellmaren_US
dc.contributor.authorOmidi, Nojanen_US
dc.contributor.authorOtto, Antoniusen_US
dc.contributor.authorRen, Jieen_US
dc.contributor.authorShi, Quanqien_US
dc.contributor.authorSibeck, Daviden_US
dc.contributor.authorYao, Shutaoen_US
dc.contributor.departmentDepartment of Electronics and Nanoengineeringen
dc.contributor.groupauthorEsa Kallio Groupen
dc.contributor.organizationUniversity of Alaska Fairbanksen_US
dc.contributor.organizationPeking Universityen_US
dc.contributor.organizationWigner Research Centre for Physicsen_US
dc.contributor.organizationTongji Universityen_US
dc.contributor.organizationInstitute of Space and Astronautical Scienceen_US
dc.contributor.organizationInstitute of Earth Physics and Space Scienceen_US
dc.contributor.organizationNASA Goddard Space Flight Centeren_US
dc.contributor.organizationLaboratoire Atmosphèresen_US
dc.contributor.organizationAuburn Universityen_US
dc.contributor.organizationUniversity of Bergenen_US
dc.contributor.organizationSolana Scientic Inc.en_US
dc.contributor.organizationShandong Universityen_US
dc.date.accessioned2022-09-07T08:47:53Z
dc.date.available2022-09-07T08:47:53Z
dc.date.issued2022-08en_US
dc.descriptionFunding Information: QGZ acknowledges Major Project of Chinese National Programs for Fundamental Research and Development 2021YFA0718600 and China Space Agency Project D020301. HZ acknowledges NSF AGS-1352669 and NASA grant 80NSSC18K1376. BL thanks the Centre National d’Etudes Spatiales (CNES; grant nos. APR-W-EEXP/10- 01-01-05 and APR-Z-ETP-E-0010/01-01-05) and GENCI Agency (DARI project; grant no. A0050400295) for their support. TZL is supported by the NASA Living With a Star Jack Eddy Postdoctoral Fellowship Program, administered by the Cooperative Programs for the Advancement of Earth System Science (CPAESS) and is partially supported by NSF award AGS-1941012. HKC acknowledges NSF grants, OIA-1920965 and AGS-1928883 and the NASA grants, 80NSSC18K1043, 80NSSC18K1052 and 80NSSC19K0844. Work at GSFC was supported by NASA’s THEMIS, MMS, and SR programs. The work of DH is supported by National Natural Science Foundation of China (42030101). The research of AK and GF has been supported by the Research Centre for Astronomy and Earth Sciences, Eötvös Loránd Research Network. KO is supported by the Research Council of Norway grant 223252. The authors acknowledge the International Space Science Institute-Beijing for supporting the international team “Dayside Transient Phenomena and Their Impact on the Magnetosphere-Ionosphere”. Funding Information: QGZ acknowledges Major Project of Chinese National Programs for Fundamental Research and Development 2021YFA0718600 and China Space Agency Project D020301. HZ acknowledges NSF AGS-1352669 and NASA grant 80NSSC18K1376. BL thanks the Centre National d’Etudes Spatiales (CNES; grant nos. APR-W-EEXP/10- 01-01-05 and APR-Z-ETP-E-0010/01-01-05) and GENCI Agency (DARI project; grant no. A0050400295) for their support. TZL is supported by the NASA Living With a Star Jack Eddy Postdoctoral Fellowship Program, administered by the Cooperative Programs for the Advancement of Earth System Science (CPAESS) and is partially supported by NSF award AGS-1941012. HKC acknowledges NSF grants, OIA-1920965 and AGS-1928883 and the NASA grants, 80NSSC18K1043, 80NSSC18K1052 and 80NSSC19K0844. Work at GSFC was supported by NASA’s THEMIS, MMS, and SR programs. The work of DH is supported by National Natural Science Foundation of China (42030101). The research of AK and GF has been supported by the Research Centre for Astronomy and Earth Sciences, Eötvös Loránd Research Network. KO is supported by the Research Council of Norway grant 223252. The authors acknowledge the International Space Science Institute-Beijing for supporting the international team “Dayside Transient Phenomena and Their Impact on the Magnetosphere-Ionosphere”. Publisher Copyright: © 2022, The Author(s).
dc.description.abstractDayside transients, such as hot flow anomalies, foreshock bubbles, magnetosheath jets, flux transfer events, and surface waves, are frequently observed upstream from the bow shock, in the magnetosheath, and at the magnetopause. They play a significant role in the solar wind-magnetosphere-ionosphere coupling. Foreshock transient phenomena, associated with variations in the solar wind dynamic pressure, deform the magnetopause, and in turn generates field-aligned currents (FACs) connected to the auroral ionosphere. Solar wind dynamic pressure variations and transient phenomena at the dayside magnetopause drive magnetospheric ultra low frequency (ULF) waves, which can play an important role in the dynamics of Earth’s radiation belts. These transient phenomena and their geoeffects have been investigated using coordinated in-situ spacecraft observations, spacecraft-borne imagers, ground-based observations, and numerical simulations. Cluster, THEMIS, Geotail, and MMS multi-mission observations allow us to track the motion and time evolution of transient phenomena at different spatial and temporal scales in detail, whereas ground-based experiments can observe the ionospheric projections of transient magnetopause phenomena such as waves on the magnetopause driven by hot flow anomalies or flux transfer events produced by bursty reconnection across their full longitudinal and latitudinal extent. Magnetohydrodynamics (MHD), hybrid, and particle-in-cell (PIC) simulations are powerful tools to simulate the dayside transient phenomena. This paper provides a comprehensive review of the present understanding of dayside transient phenomena at Earth and other planets, their geoeffects, and outstanding questions.en
dc.description.versionPeer revieweden
dc.format.mimetypeapplication/pdfen_US
dc.identifier.citationZhang, H, Zong, Q, Connor, H, Delamere, P, Facskó, G, Han, D, Hasegawa, H, Kallio, E, Kis, Á, Le, G, Lembège, B, Lin, Y, Liu, T, Oksavik, K, Omidi, N, Otto, A, Ren, J, Shi, Q, Sibeck, D & Yao, S 2022, ' Dayside Transient Phenomena and Their Impact on the Magnetosphere and Ionosphere ', Space Science Reviews, vol. 218, no. 5, 40 . https://doi.org/10.1007/s11214-021-00865-0en
dc.identifier.doi10.1007/s11214-021-00865-0en_US
dc.identifier.issn0038-6308
dc.identifier.issn1572-9672
dc.identifier.otherPURE UUID: abf67466-2385-4694-bfe3-c5c3f7236637en_US
dc.identifier.otherPURE ITEMURL: https://research.aalto.fi/en/publications/abf67466-2385-4694-bfe3-c5c3f7236637en_US
dc.identifier.otherPURE LINK: http://www.scopus.com/inward/record.url?scp=85125386009&partnerID=8YFLogxKen_US
dc.identifier.otherPURE FILEURL: https://research.aalto.fi/files/87226021/Dayside_Transient_Phenomena_and_Their_Impact_on_the_Magnetosphere_and_Ionosphere.pdfen_US
dc.identifier.urihttps://aaltodoc.aalto.fi/handle/123456789/116576
dc.identifier.urnURN:NBN:fi:aalto-202209075386
dc.language.isoenen
dc.publisherSPRINGER
dc.relation.ispartofseriesSpace Science Reviewsen
dc.relation.ispartofseriesVolume 218, issue 5en
dc.rightsopenAccessen
dc.subject.keywordBow shocken_US
dc.subject.keywordFlux transfer eventsen_US
dc.subject.keywordMirror modeen_US
dc.subject.keywordSurface wavesen_US
dc.subject.keywordTransient foreshock phenomenaen_US
dc.subject.keywordUltra-low frequency wavesen_US
dc.titleDayside Transient Phenomena and Their Impact on the Magnetosphere and Ionosphereen
dc.typeA2 Katsausartikkeli tieteellisessä aikakauslehdessäfi
dc.type.versionpublishedVersion
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