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What is the heliopause? Importance of magnetic reconnection and measurement requirements

hal.structure.identifierLaboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
dc.contributor.authorLAVRAUD, Benoit
dc.contributor.authorOPHER, M.
dc.contributor.authorDIALYNAS, K.
hal.structure.identifierJohns Hopkins University [JHU]
dc.contributor.authorTURNER, D
dc.contributor.authorERIKSSON, S.
hal.structure.identifierJohns Hopkins University [JHU]
dc.contributor.authorPROVORNIKOVA, E.
dc.contributor.authorKORNBLEUTH, M
hal.structure.identifierJohns Hopkins University [JHU]
dc.contributor.authorMOSTAFAVI, P.
hal.structure.identifierInstitut de recherche en astrophysique et planétologie [IRAP]
dc.contributor.authorFEDOROV, A.
dc.contributor.authorRICHARDSON, J
dc.contributor.authorFUSELIER, S
dc.contributor.authorDRAKE, J.
dc.contributor.authorSWISDAK, M.
dc.contributor.authorEUBANKS, M.
dc.contributor.authorCHEN, T
dc.contributor.authorKUCHAREK, H.
hal.structure.identifierJohns Hopkins University [JHU]
dc.contributor.authorKOLLMANN, P.
hal.structure.identifierInstitut de recherche en astrophysique et planétologie [IRAP]
dc.contributor.authorBLANC, M.
hal.structure.identifierInstitut de recherche en astrophysique et planétologie [IRAP]
dc.contributor.authorANDRÉ, N.
hal.structure.identifierInstitut de recherche en astrophysique et planétologie [IRAP]
dc.contributor.authorGÉNOT, V.
dc.contributor.authorWIMMER-SCHWEINGRUBER, R
dc.contributor.authorBARABASH, S.
hal.structure.identifierJohns Hopkins University [JHU]
dc.contributor.authorBRANDT, P.
hal.structure.identifierJohns Hopkins University [JHU]
dc.contributor.authorMCNUTT, R.
dc.date.issued2023
dc.identifier.issn2296-987X
dc.description.abstractEnWe highlight the importance of magnetic reconnection at the heliopause, both as one of the key processes driving the interaction between solar and interstellar media, but also as an element of the definition of the heliopause itself. We highlight the main observations that have fed the current debates on the definition, location and shape of the heliopause. We explain that discriminating between the current interpretations of plasma and magnetic field structures near the heliopause necessitates appropriate measurements which are lacking on Voyager 1 and 2, and describe some of the ensuing requirements for thermal plasma measurements on a future Interstellar Probe. The content of this article was submitted as a white paper contribution to the Decadal Survey for Solar and Space Physics 2024–2033 of the National Academy of Sciences.
dc.language.isoen
dc.publisherFrontiers Media
dc.subject.enHeliosphere
dc.subject.enHeliopause
dc.subject.enSolar wind
dc.subject.enHeliosheath
dc.subject.enInterstellar medium
dc.subject.enMagnetic Reconnection
dc.subject.enInstrumentation
dc.title.enWhat is the heliopause? Importance of magnetic reconnection and measurement requirements
dc.typeArticle de revue
dc.identifier.doi10.3389/fspas.2023.1060618
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Astrophysique stellaire et solaire [astro-ph.SR]
dc.subject.halPhysique [physics]/Physique [physics]/Physique de l'espace [physics.space-ph]
bordeaux.journalFrontiers in Astronomy and Space Sciences
bordeaux.page1060618
bordeaux.volume10
bordeaux.peerReviewedoui
hal.identifierhal-04274010
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-04274010v1
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