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



ID: 60326.0, MPI für Kernphysik / Interplanetary Dust Physics
Four years of Ulysses dust data: 1996-1999
Authors:Krüger, Harald; Grün, Eberhard; Landgraf, M.; Dermott, S.; Fechtig, Hugo; Gustafson, B. A.; Hamilton, D. P.; Hanner, M. S.; Horányi, M.; Kissel, J.; Lindblad, B. A.; Linkert, Dietmar; Linkert, Gudrun; Mann, I.; McDonnell, J. A. M.; Morfill, G. E.; Polanskey, C.; Schwehm, G.; Srama, Ralf; Zook, H. A.
Language:English
Date of Publication (YYYY-MM-DD):2001-11
Title of Journal:Planetary and Space Science
Journal Abbrev.:Planet. Space Sci.
Volume:49
Issue / Number:13
Start Page:1303
End Page:1324
Copyright:Copyright © 2001 Published by Elsevier Science Ltd. All rights reserved.
Review Status:not specified
Audience:Experts Only
Abstract / Description:The Ulysses spacecraft is orbiting the Sun on a highly inclined ellipse (i=79°, perihelion distance 1.3 AU, aphelion distance 5.4 AU). Between January 1996 and December 1999 the spacecraft was beyond 3 AU from the Sun and crossed the ecliptic plane at aphelion in May 1998. In this 4-yr period 218 dust impacts were recorded with the dust detector on board. We publish and analyse the complete data set of both raw and reduced data for particles with masses 10-16–10-8 g. Together with 1477 dust impacts recorded between launch of Ulysses and the end of 1995 published earlier (Grün et al., Planet. Space Sci. 43 (1995a) 971; Krüger et al., Planet. Space Sci. 47 (1999b) 363), a data set of 1695 dust impacts detected with the Ulysses sensor between October 1990 and December 1999 is now available. The impact rate measured between 1996 and 1999 was relatively constant with about 0.2 impacts per day. The impact direction of the majority of the impacts is compatible with particles of interstellar origin, the rest are most likely interplanetary particles. The observed impact rate is compared with a model for the flux of interstellar dust particles. The flux of particles several micrometres in size is compared with the measurements of the dust instruments on board Pioneer 10 and Pioneer 11 beyond 3 AU (Humes, J. Geophys. Res. 85 (1980) 5841). Between 3 and 5 AU, Pioneer results predict that Ulysses should have seen 5 times more (~10 μm sized) particles than actually detected.
External Publication Status:published
Document Type:Article
Affiliations:MPI für Kernphysik/Group K. Mauersberger/Interplantary Dust Research (E. Grün)
MPI für extraterrestrische Physik
External Affiliations:ESOC, 64293 Darmstadt, Germany, University of Florida, Gainesville, FL 32611, USA, University of Maryland, College Park, MD 20742-2421, USA, Jet Propulsion Laboratory, Pasadena, CA 91109, USA, Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, CO 80309, USA, Lund Observatory, 221 Lund, Sweden, Institut für Planetologie, Universität Münster, 48149 Münster, Germany, Planetary and Space Science Research Institute, The Open University, Milton Keynes, MK7 6AA, UK, ESTEC, 2200 AG Noordwijk, Netherlands, NASA Johnson Space Center, Houston, TX 77058, USA
Identifiers:DOI:10.1016/S0032-0633(01)00054-X
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