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          Institute: MPI für Kernphysik     Collection: Interplanetary Dust Physics     Display Documents



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ID: 246975.0, MPI für Kernphysik / Interplanetary Dust Physics
In-Situ Monitoring of Interstellar Dust in the Inner Solar System
Authors:Altobelli, Nicolas; Kempf, Sascha; Krüger, Harald; Landgraf, Markus; Srama, Ralf; Grün, Eberhard
Language:English
Publisher:American Institute of Physics
Place of Publication:Melville
Date of Publication (YYYY-MM-DD):2005
Title of Proceedings:The Spectral Energy Distributions of Gas-Rich Galaxies: Confronting Models with Data
Start Page:149
End Page:152
Title of Series:AIP Conference Proceedings
Volume (in Series):761
Physical Description:XVII, 465 S. : Ill., graph. Darst.
Name of Conference/Meeting:The Spectral Energy Distributions of Gas-Rich Galaxies: Confronting Models with Data
Place of Conference/Meeting:Heidelberg
(Start) Date of Conference/Meeting
 (YYYY-MM-DD):
2004-10-04
End Date of Conference/Meeting 
 (YYYY-MM-DD):
2004-10-08
Review Status:not specified
Audience:Experts Only
Abstract / Description:We present in this paper new interstellar dust data obtained in the inner solar system by the dust instruments on-board the Cassini, Galileo and Helios spacecraft. While the Ulysses dust instrument provided an in-situ monitoring of the interstellar dust stream at high ecliptic latitude between 3 AU and 5 AU, the new data cover an heliocentric distance range between 0.3 AU and 3 AU in the ecliptic plane. Furthermore, the data provide evidence of the interstellar dust stream alteration in the inner solar system, caused by radiation pressure forces and gravitation focusing.
External Publication Status:published
Document Type:Conference-Paper
Affiliations:MPI für Kernphysik/Group K. Mauersberger/Interplantary Dust Research (E. Grün)
Identifiers:URL:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bi...
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