dc.contributor.author
Baalmann, L. R.
dc.contributor.author
Janisch, T.
dc.contributor.author
Hunziker, S.
dc.contributor.author
Strub, Peter
dc.contributor.author
Krüger, H.
dc.contributor.author
Hofstetter, K.
dc.contributor.author
Sieber, M.
dc.contributor.author
Sterken, V. J.
dc.date.accessioned
2025-08-26T07:15:44Z
dc.date.available
2025-08-26T07:15:44Z
dc.identifier.uri
https://refubium.fu-berlin.de/handle/fub188/48864
dc.identifier.uri
http://dx.doi.org/10.17169/refubium-48587
dc.description.abstract
Interstellar dust (ISD) enters the heliosphere from the direction of its nose. It is first modulated by the heliosheath and then the inner heliosphere before it is measured by the dust detectors on board of spacecraft, for example on Ulysses. Various criteria exist to distinguish ISD from the dust of other sources, and different methods exist to determine the particle masses and impact speeds from the measurements.
en
dc.format.extent
31 Seiten
dc.rights.uri
https://creativecommons.org/licenses/by/4.0/
dc.subject
Sun: heliosphere
en
dc.subject
interplanetary medium
en
dc.subject
ISM: general
en
dc.subject.ddc
500 Naturwissenschaften und Mathematik::520 Astronomie::520 Astronomie und zugeordnete Wissenschaften
dc.title
Interstellar dust measured in situ by Ulysses: New aspects of the particle size distribution and its modulation by the heliosheath
dc.type
Wissenschaftlicher Artikel
dcterms.bibliographicCitation.articlenumber
A138
dcterms.bibliographicCitation.doi
10.1051/0004-6361/202453532
dcterms.bibliographicCitation.journaltitle
Astronomy & Astrophysics
dcterms.bibliographicCitation.volume
698
dcterms.bibliographicCitation.url
https://doi.org/10.1051/0004-6361/202453532
refubium.affiliation
Geowissenschaften
refubium.affiliation.other
Institut für Geologische Wissenschaften / Fachrichtung Planetologie und Fernerkundung
refubium.resourceType.isindependentpub
no
dcterms.accessRights.openaire
open access
dcterms.isPartOf.eissn
1432-0746
refubium.resourceType.provider
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