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Volumn 307, Issue 5713, 2005, Pages 1266-1270

Cassini magnetometer observations during Saturn orbit insertion

Author keywords

[No Author keywords available]

Indexed keywords

CYCLOTRON RADIATION; ION ACOUSTIC WAVES; MAGNETIC FIELDS; MAGNETOMETERS; ORBITS; SPACECRAFT;

EID: 20044367812     PISSN: 00368075     EISSN: None     Source Type: Journal    
DOI: 10.1126/science.1106098     Document Type: Article
Times cited : (195)

References (26)
  • 3
    • 14544280351 scopus 로고    scopus 로고
    • note
    • International Astronomical Union standard definition of the Saturn equatorial body radius.
  • 5
    • 14544307603 scopus 로고    scopus 로고
    • note
    • The ratio δB/B0 is the enhancement of the overshoot magnetic field normalized by the magnetosheath field strength away from the overshoot.
  • 7
    • 0001230590 scopus 로고
    • N. F. Ness et al., Science 212, 211 (1981).
    • (1981) Science , vol.212 , pp. 211
    • Ness, N.F.1
  • 8
    • 0038015313 scopus 로고
    • N. F. Ness et al., Science 215, 558 (1982).
    • (1982) Science , vol.215 , pp. 558
    • Ness, N.F.1
  • 20
    • 14544275651 scopus 로고    scopus 로고
    • note
    • The dayside of the magnetopause is approximately ellipsoidal, but this is not the case in the tail, which is nearly circular in cross section. To accurately approximate the shape of the magnetopause, the tailward half of an ellipsoid is replaced with a cylinder; thus, the boundary is a composite surface composed of a hemi-ellipsoid and a cylinder. The join between these two surfaces is at the semi-minor axis of the prolate ellipsoid (nose portion).
  • 24
    • 14544291194 scopus 로고    scopus 로고
    • note
    • The KSM (Kronocentric Solar Magnetospheric) coordinate system has Saturn at the origin, with the +X axis directed toward the Sun; Z defined such that Saturn's rotation and magnetic axis lies in the XZ plane (with +2 pointing close to northward), and Y lying in Saturn's rotational and magnetic equatorial plane.
  • 25
    • 14544295535 scopus 로고    scopus 로고
    • note
    • The reference for the SPV model is (13); for the Z3 model, (14); and the GD model, (15).
  • 26
    • 14544296756 scopus 로고    scopus 로고
    • note
    • We wish to acknowledge the Cassini Project and operations team from the Jet Propulsion Laboratory, as well as the many people at our home institutions for their design, engineering, and software support over many years on behalf of this investigation. The contributions to the MAG team have been supported by the Particle Physics and Astronomy Research Council in the UK, Deutsches Zentrum für Luft-und Raumfahrt in Germany, and NASA in the U.S.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.