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dc.contributor.authorMann, Ingrid
dc.contributor.authorNouzak, Libor
dc.contributor.authorVaverka, Jakub
dc.contributor.authorAntonsen, Tarjei
dc.contributor.authorFredriksen, Åshild
dc.contributor.authorIssautier, Karine
dc.contributor.authorMalaspina, David
dc.contributor.authorMeyer-Vernet, Nicole
dc.contributor.authorPavlu, Jiri
dc.contributor.authorSternovsky, Zoltan
dc.contributor.authorStude, Joan
dc.contributor.authorYe, Shengyi
dc.contributor.authorZaslavsky, Arnaud
dc.date.accessioned2019-12-30T10:29:32Z
dc.date.available2019-12-30T10:29:32Z
dc.date.issued2019-12-10
dc.description.abstractThe electric and magnetic field instrument suite FIELDS on board the NASA Parker Solar Probe and the radio and plasma waves instrument RPW on the ESA Solar Orbiter mission that explore the inner heliosphere are sensitive to signals generated by dust impacts. Dust impacts have been observed using electric field antennas on spacecraft since the 1980s and the method was recently used with a number of space missions to derive dust fluxes. Here, we consider the details of dust impacts, subsequent development of the impact generated plasma and how it produces the measured signals. We describe empirical approaches to characterise the signals and compare these in a qualitative discussion of laboratory simulations to predict signal shapes for spacecraft measurements in the inner solar system. While the amount of charge production from a dust impact will be higher near the Sun than observed in the interplanetary medium before, the amplitude of pulses is determined by the recovery behaviour that is different near the Sun since it varies with the plasma environment.en_US
dc.identifier.citationMann IB, Nouzak L, Vaverka J, Antonsen T, Fredriksen Å, Issautier K, Malaspina, Meyer-Vernet N, Pavlu J, Sternovsky Z, Stude, Ye S, Zaslavsky A. Dust observations with antenna measurements and its prospects for observations with Parker Solar Probe and Solar Orbiter. Annales Geophysicae. 2019en_US
dc.identifier.cristinIDFRIDAID 1760293
dc.identifier.doihttps://doi.org/10.5194/angeo-37-1121-2019
dc.identifier.issn0992-7689
dc.identifier.issn1432-0576
dc.identifier.urihttps://hdl.handle.net/10037/16994
dc.language.isoengen_US
dc.publisherEuropean Geosciences Unionen_US
dc.relation.journalAnnales Geophysicae
dc.relation.projectIDinfo:eu-repo/grantAgreement/RCN/ROMFORSK/262941/Norway/Cosmic dust in the solar-terrestrial physics: exploring the inner heliosphere//en_US
dc.rights.accessRightsopenAccessen_US
dc.rights.holderCopyright 2019 The Author(s)en_US
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/*
dc.rightsAttribution 4.0 International*
dc.subjectVDP::Mathematics and natural science: 400::Physics: 430::Astrophysics, astronomy: 438en_US
dc.subjectVDP::Matematikk og Naturvitenskap: 400::Fysikk: 430::Astrofysikk, astronomi: 438en_US
dc.titleDust observations with antenna measurements and its prospects for observations with Parker Solar Probe and Solar Orbiteren_US
dc.type.versionpublishedVersionen_US
dc.typeJournal articleen_US
dc.typeTidsskriftartikkelen_US
dc.typePeer revieweden_US


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Attribution 4.0 International
Except where otherwise noted, this item's license is described as Attribution 4.0 International