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hal.structure.identifierUniversity of Arizona
dc.contributor.authorKLEIN, Kristopher
hal.structure.identifierUniversity of New Hampshire [UNH]
dc.contributor.authorSPENCE, Harlan
hal.structure.identifierPôle Planétologie du LESIA
dc.contributor.authorALEXANDROVA, Olga
hal.structure.identifierUniversity of New Hampshire [UNH]
dc.contributor.authorARGALL, Matthew
hal.structure.identifierInstitute for Advanced Study [Princeton] [IAS]
dc.contributor.authorARZAMASSKIY, Lev
hal.structure.identifierNASA Ames Research Center [ARC]
dc.contributor.authorBOOKBINDER, Jay
hal.structure.identifierUniversity of Arizona
dc.contributor.authorBROEREN, Theodore
hal.structure.identifierUniversity of Chicago
dc.contributor.authorCAPRIOLI, Damiano
dc.contributor.authorCASE, Anthony
hal.structure.identifierUniversity of New Hampshire [UNH]
dc.contributor.authorCHANDRAN, Benjamin
dc.contributor.authorCHEN, Li-Jen
dc.contributor.authorDORS, Ivan
hal.structure.identifierImperial College London
dc.contributor.authorEASTWOOD, Jonathan
hal.structure.identifierUniversity College of London [London] [UCL]
dc.contributor.authorFORSYTH, Colin
dc.contributor.authorGALVIN, Antoinette
hal.structure.identifierInstitut de recherche en astrophysique et planétologie [IRAP]
dc.contributor.authorGENOT, Vincent
dc.contributor.authorHALEKAS, Jasper
dc.contributor.authorHESSE, Michael
dc.contributor.authorHINE, Butler
dc.contributor.authorHORBURY, Tim
dc.contributor.authorJIAN, Lan
dc.contributor.authorKASPER, Justin
hal.structure.identifierLaboratoire de Physique et Chimie de l'Environnement et de l'Espace [LPC2E]
dc.contributor.authorKRETZSCHMAR, Matthieu
dc.contributor.authorKUNZ, Matthew
hal.structure.identifierLaboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
hal.structure.identifierInstitut de recherche en astrophysique et planétologie [IRAP]
dc.contributor.authorLAVRAUD, Benoit
hal.structure.identifierLaboratoire de Physique des Plasmas [LPP]
dc.contributor.authorCONTEL, Olivier Le
hal.structure.identifierUniversity of California [Berkeley] [UC Berkeley]
dc.contributor.authorMALLET, Alfred
hal.structure.identifierUniversity of Delaware [Newark]
dc.contributor.authorMARUCA, Bennett
dc.contributor.authorMATTHAEUS, William
dc.contributor.authorNIEHOF, Jonathan
dc.contributor.authorO'BRIAN, Helen
dc.contributor.authorOWEN, Christopher
hal.structure.identifierLaboratoire de Physique des Plasmas [LPP]
dc.contributor.authorRETINO, Alessandro
hal.structure.identifierUniversity of Cambridge [UK] [CAM]
dc.contributor.authorREYNOLDS, Christopher
hal.structure.identifierAustrian Academy of Sciences [OeAW]
dc.contributor.authorROBERTS, Owen
dc.contributor.authorSCHEKOCHIHIN, Alexander
dc.contributor.authorSKOUG, Ruth
dc.contributor.authorSMITH, Charles
dc.contributor.authorSMITH, Sonya
dc.contributor.authorSTEINBERG, John
dc.contributor.authorSTEVENS, Michael
dc.contributor.authorSZABO, Adam
dc.contributor.authorTENBARGE, Jason
dc.contributor.authorTORBERT, Roy
dc.contributor.authorVASQUEZ, Bernard
dc.contributor.authorVERSCHAREN, Daniel
dc.contributor.authorWHITTLESEY, Phyllis
dc.contributor.authorWICKIZER, Brittany
hal.structure.identifierDepartment of Atmospheric Science [Huntsville]
dc.contributor.authorZANK, Gary
hal.structure.identifierUniversity of Wisconsin-Madison
dc.contributor.authorZWEIBEL, Ellen
dc.date2023
dc.date.issued2023
dc.identifier.issn0038-6308
dc.description.abstractEnHelioSwarm (HS) is a NASA Medium-Class Explorer mission of the Heliophysics Division designed to explore the dynamic three-dimensional mechanisms controlling the physics of plasma turbulence, a ubiquitous process occurring in the heliosphere and in plasmas throughout the universe. This will be accomplished by making simultaneous measurements at nine spacecraft with separations spanning magnetohydrodynamic and sub-ion spatial scales in a variety of near-Earth plasmas. In this paper, we describe the scientific background for the HS investigation, the mission goals and objectives, the observatory reference trajectory and instrumentation implementation before the start of Phase B. Through multipoint, multiscale measurements, HS promises to reveal how energy is transferred across scales and boundaries in plasmas throughout the universe.
dc.language.isoen
dc.publisherSpringer Verlag
dc.subject.enPlasma Physics (physics.plasm-ph)
dc.subject.enSolar and Stellar Astrophysics (astro-ph.SR)
dc.subject.enSpace Physics (physics.space-ph)
dc.subject.enFOS: Physical sciences
dc.title.enHelioSwarm: A Multipoint, Multiscale Mission to Characterize Turbulence
dc.typeArticle de revue
dc.identifier.doi10.48550/arXiv.2306.06537
dc.subject.halPlanète et Univers [physics]
bordeaux.journalSpace Science Reviews
bordeaux.peerReviewedoui
hal.identifierhal-04275202
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-04275202v1
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