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Volumn 308, Issue 5724, 2005, Pages 992-995

Titan's magnetic field signature during the first Cassini encounter

Author keywords

[No Author keywords available]

Indexed keywords

EXTRATERRESTRIAL ATMOSPHERES; MAGNETIC FIELDS; MATHEMATICAL MODELS; SATELLITES; SPACE APPLICATIONS; SPACECRAFT;

EID: 20844445961     PISSN: 00368075     EISSN: None     Source Type: Journal    
DOI: 10.1126/science.1109763     Document Type: Article
Times cited : (116)

References (28)
  • 1
    • 0001904929 scopus 로고
    • T. Gehrels, M. S. Matthews, Eds. Univ. of Ariz. Press, Tucson, AZ
    • A. W. Schardt et al., Saturn, T. Gehrels, M. S. Matthews, Eds. (Univ. of Ariz. Press, Tucson, AZ, 1984), pp. 417-459.
    • (1984) Saturn , pp. 417-459
    • Schardt, A.W.1
  • 2
    • 18644382903 scopus 로고    scopus 로고
    • note
    • This velocity was measured by Voyager 1 (3). Ideal corotation would imply a velocity of 200 km/s in Titan's restframe.
  • 3
    • 0001405511 scopus 로고
    • T. Gehrels, M. S. Matthews, Eds. Univ. of Ariz. Press, Tucson, AZ
    • F. M. Neubauer, D. A. Gurnett, J. D. Scudder, R. E. Hartle, Saturn, T. Gehrels, M. S. Matthews, Eds. (Univ. of Ariz. Press, Tucson, AZ, 1984), pp. 760-787.
    • (1984) Saturn , pp. 760-787
    • Neubauer, F.M.1    Gurnett, D.A.2    Scudder, J.D.3    Hartle, R.E.4
  • 4
    • 18644367207 scopus 로고    scopus 로고
    • note
    • Plasma-β: ratio of thermal and magnetic pressure.
  • 6
    • 18644381408 scopus 로고    scopus 로고
    • note
    • Space Craft Event Time (SCET) in the universal time frame (UTC). All times given here are in this time frame.
  • 8
    • 18644374268 scopus 로고    scopus 로고
    • note
    • The coordinate system used is the Titan interaction system (TIIS) defined in Fig. 1.
  • 11
    • 18644376100 scopus 로고    scopus 로고
    • thesis, Institut für Geophysik und Meteorologie, University of Cologne, Germany
    • H. Backes, thesis, Institut für Geophysik und Meteorologie, University of Cologne, Germany (2004).
    • (2004)
    • Backes, H.1
  • 12
    • 18644370480 scopus 로고    scopus 로고
    • note
    • Several models have been developed to explain Titan's interaction with the saturnian plasma (20, 21, 23-27), which all differ in certain respects.
  • 15
    • 2142803437 scopus 로고    scopus 로고
    • Materials and methods are available as supporting material on Science Online.
    • Science Online
  • 16
    • 18644367961 scopus 로고    scopus 로고
    • note
    • A: CA time, 26 October 2004, 15:30:05 UTC; CA altitude, 1174 km; 5LT = 10.6; solar declination, -23.23°; angle between ideal corotation direction and Sun-Titan line, 109.2°; flyby through northern tail.
  • 19
  • 22
    • 18644382531 scopus 로고    scopus 로고
    • note
    • The layer between the northern and the southern lobe can have two configurations: In the first, the magnetic field is at a minimum. In this case, it is called a "neutral sheet." In the second, the magnetic field rotates continuously from the field direction in the northern lobe to the field direction in the southern lobe, while the field magnitude is constant. In this case, the expression "neutral sheet" is not appropriate and we call it "polarity reversal layer" instead.
  • 28
    • 18644365275 scopus 로고    scopus 로고
    • note
    • We acknowledge the superb work done by the technical and data processing staff of the MAG team. H.B., F.M.N., and A.W. are supported by the DLR (Germany). M.K.D., C.B., C.S.A., and N. Achilleos are supported by PPARC (UK). N. André is supported by CNES (France). This research was performed while G.H.J. held a National Research Council Research Associateship at the Jet Propulsion Laboratory (JPL). The research at the University of California, Los Angeles, was supported by NASA under a grant administered by JPL.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.