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Four years of Ulysses dust data: 1996-1999

Krüger, H.; Grün, E.; Landgraf, M.; Dermott, S.; Fechtig, H.; Gustafson, B. A.; Hamilton, D. P.; Hanner, M. S.; Horányi, M. and Kissel, J., et al. (2001) In Planetary and Space Science 49(13). p.1303-1324
Abstract
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 AUfrom the Sun and crossed the ecliptic plane at aphelion in May /1998. Inthis 4-yr period 218 dust impacts were recorded with the dust detectoron board. We publish and analyse the complete data set of both raw andreduced data for particles with masses10<SUP>-16</SUP>-10<SUP>-8</SUP>g. Together with 1477 dust impactsrecorded between launch of Ulysses and the end of /1995 publishedearlier (Grün et al., Planet. Space Sci. 43 (/1995a) 971;Krüger et al., Planet. Space Sci. 47 (/1999b) 363), a data set of1695 dust impacts... (More)
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 AUfrom the Sun and crossed the ecliptic plane at aphelion in May /1998. Inthis 4-yr period 218 dust impacts were recorded with the dust detectoron board. We publish and analyse the complete data set of both raw andreduced data for particles with masses10<SUP>-16</SUP>-10<SUP>-8</SUP>g. Together with 1477 dust impactsrecorded between launch of Ulysses and the end of /1995 publishedearlier (Grün et al., Planet. Space Sci. 43 (/1995a) 971;Krüger et al., Planet. Space Sci. 47 (/1999b) 363), a data set of1695 dust impacts detected with the Ulysses sensor between October /1990and December /1999 is now available. The impact rate measured between1996 and 1999 was relatively constant with about 0.2 impacts per day.The impact direction of the majority of the impacts is compatible withparticles of interstellar origin, the rest are most likelyinterplanetary particles. The observed impact rate is compared with amodel for the flux of interstellar dust particles. The flux of particlesseveral micrometres in size is compared with the measurements of thedust instruments on board Pioneer 10 and Pioneer 11 beyond 3 AU (Humes,J. Geophys. Res. 85 /(1980) 5841). Between 3 and 5 AU, Pioneer resultspredict that Ulysses should have seen 5 times more (~10mum sized)particles than actually detected. (Less)
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published
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Planetary and Space Science
volume
49
issue
13
pages
1303 - 1324
publisher
Elsevier
external identifiers
  • Scopus:0142090813
ISSN
1873-5088
DOI
10.1016/S0032-0633(01)00054-X
language
English
LU publication?
yes
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c83be549-bf12-4d3e-9cd4-c55c2442354b (old id 130080)
date added to LUP
2007-07-13 13:49:22
date last changed
2016-10-13 04:44:40
@misc{c83be549-bf12-4d3e-9cd4-c55c2442354b,
  abstract     = {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 AUfrom the Sun and crossed the ecliptic plane at aphelion in May /1998. Inthis 4-yr period 218 dust impacts were recorded with the dust detectoron board. We publish and analyse the complete data set of both raw andreduced data for particles with masses10&lt;SUP&gt;-16&lt;/SUP&gt;-10&lt;SUP&gt;-8&lt;/SUP&gt;g. Together with 1477 dust impactsrecorded between launch of Ulysses and the end of /1995 publishedearlier (Grün et al., Planet. Space Sci. 43 (/1995a) 971;Krüger et al., Planet. Space Sci. 47 (/1999b) 363), a data set of1695 dust impacts detected with the Ulysses sensor between October /1990and December /1999 is now available. The impact rate measured between1996 and 1999 was relatively constant with about 0.2 impacts per day.The impact direction of the majority of the impacts is compatible withparticles of interstellar origin, the rest are most likelyinterplanetary particles. The observed impact rate is compared with amodel for the flux of interstellar dust particles. The flux of particlesseveral micrometres in size is compared with the measurements of thedust instruments on board Pioneer 10 and Pioneer 11 beyond 3 AU (Humes,J. Geophys. Res. 85 /(1980) 5841). Between 3 and 5 AU, Pioneer resultspredict that Ulysses should have seen 5 times more (~10mum sized)particles than actually detected.},
  author       = {Krüger, H. and Grün, E. and Landgraf, M. and Dermott, S. and Fechtig, H. and Gustafson, B. A. and Hamilton, D. P. and Hanner, M. S. and Horányi, M. and Kissel, J. and Lindblad, Bertil Anders and Linkert, D. and Linkert, G. and Mann, I. and McDonnell, J. A. M. and Morfill, G. E. and Polanskey, C. and Schwehm, G. and Srama, R. and Zook, H. A.},
  issn         = {1873-5088},
  language     = {eng},
  number       = {13},
  pages        = {1303--1324},
  publisher    = {ARRAY(0x92c3ac8)},
  series       = {Planetary and Space Science},
  title        = {Four years of Ulysses dust data: 1996-1999},
  url          = {http://dx.doi.org/10.1016/S0032-0633(01)00054-X},
  volume       = {49},
  year         = {2001},
}