Journal article Open Access

Discovery of Jovian dust streams and interstellar grains by the Ulysses spacecraft

Grün, E.; Zook, H. A.; Baguhl, M.; Balogh, A.; Bame, S. J.; Fechtig, H.; Forsyth, R.; Manner, M. S.; Horanyi, M.; Kissel, J.; Lindblad, B.-A.; Linkert, D.; Linkert, G.; Mann, I.; McDonnell, J. A. M.; Morfill, G. E.; Phillips, J. L.; Polanskey, C.; Schwehm, G.; Siddique, N.; Staubach, P.; Svestka, J.; Taylor, A.


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  <identifier identifierType="URL">https://zenodo.org/record/1233143</identifier>
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      <creatorName>Grün, E.</creatorName>
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      <creatorName>Zook, H. A.</creatorName>
      <givenName>H. A.</givenName>
      <familyName>Zook</familyName>
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      <creatorName>Baguhl, M.</creatorName>
      <givenName>M.</givenName>
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      <creatorName>Balogh, A.</creatorName>
      <givenName>A.</givenName>
      <familyName>Balogh</familyName>
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      <creatorName>Bame, S. J.</creatorName>
      <givenName>S. J.</givenName>
      <familyName>Bame</familyName>
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      <creatorName>Fechtig, H.</creatorName>
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      <creatorName>Forsyth, R.</creatorName>
      <givenName>R.</givenName>
      <familyName>Forsyth</familyName>
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      <creatorName>Manner, M. S.</creatorName>
      <givenName>M. S.</givenName>
      <familyName>Manner</familyName>
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      <creatorName>Horanyi, M.</creatorName>
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      <creatorName>Kissel, J.</creatorName>
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      <creatorName>Lindblad, B.-A.</creatorName>
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      <creatorName>Linkert, D.</creatorName>
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      <creatorName>Linkert, G.</creatorName>
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      <creatorName>Mann, I.</creatorName>
      <givenName>I.</givenName>
      <familyName>Mann</familyName>
    </creator>
    <creator>
      <creatorName>McDonnell, J. A. M.</creatorName>
      <givenName>J. A. M.</givenName>
      <familyName>McDonnell</familyName>
    </creator>
    <creator>
      <creatorName>Morfill, G. E.</creatorName>
      <givenName>G. E.</givenName>
      <familyName>Morfill</familyName>
    </creator>
    <creator>
      <creatorName>Phillips, J. L.</creatorName>
      <givenName>J. L.</givenName>
      <familyName>Phillips</familyName>
    </creator>
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      <creatorName>Polanskey, C.</creatorName>
      <givenName>C.</givenName>
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      <creatorName>Schwehm, G.</creatorName>
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      <creatorName>Siddique, N.</creatorName>
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      <creatorName>Staubach, P.</creatorName>
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      <creatorName>Svestka, J.</creatorName>
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    </creator>
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      <creatorName>Taylor, A.</creatorName>
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      <familyName>Taylor</familyName>
    </creator>
  </creators>
  <titles>
    <title>Discovery of Jovian dust streams and interstellar grains by the Ulysses spacecraft</title>
  </titles>
  <publisher>Zenodo</publisher>
  <publicationYear>1993</publicationYear>
  <dates>
    <date dateType="Issued">1993-04-01</date>
  </dates>
  <resourceType resourceTypeGeneral="JournalArticle"/>
  <alternateIdentifiers>
    <alternateIdentifier alternateIdentifierType="url">https://zenodo.org/record/1233143</alternateIdentifier>
  </alternateIdentifiers>
  <relatedIdentifiers>
    <relatedIdentifier relatedIdentifierType="DOI" relationType="IsIdenticalTo">10.1038/362428a0</relatedIdentifier>
  </relatedIdentifiers>
  <rightsList>
    <rights rightsURI="https://creativecommons.org/publicdomain/zero/1.0/legalcode">Creative Commons Zero v1.0 Universal</rights>
    <rights rightsURI="info:eu-repo/semantics/openAccess">Open Access</rights>
  </rightsList>
  <descriptions>
    <description descriptionType="Abstract">ON 8 February 1992, the Ulysses spacecraft flew by Jupiter at a distance of 5.4 AU from the Sun. During the encounter, the spacecraft was deflected into a new orbit, inclined at about 80° to the ecliptic plane, which will ultimately lead Ulysses over the polar regions of the Sun1. Within 1 AU from Jupiter, the onboard dust detector2 recorded periodic bursts of submicrometre dust particles, with durations ranging from several hours to two days, and occurring at approximately monthly intervals (28 ± 3 days). These particles arrived at Ulysses in collimated streams radiating from close to the line-of-sight direction to Jupiter, suggesting a jovian origin for the periodic bursts. Ulysses also detected a flux of micrometre-sized dust particles moving in high-velocity ( =26 km s-1) retrograde orbits (opposite to the motion of the planets); we identify these grains as being of interstellar origin.</description>
  </descriptions>
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