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Volumn 274, Issue 5292, 1996, Pages 1501-1503

Solar wind magnetic field bending of jovian dust trajectories

Author keywords

[No Author keywords available]

Indexed keywords

ARTICLE; COSMOS; DUST; FORCE; MAGNETIC FIELD; MATHEMATICAL ANALYSIS; MEASUREMENT; PARTICLE SIZE; PRIORITY JOURNAL; SPACE FLIGHT; SUN; VELOCITY; WIND;

EID: 0029806931     PISSN: 00368075     EISSN: None     Source Type: Journal    
DOI: 10.1126/science.274.5292.1501     Document Type: Article
Times cited : (82)

References (17)
  • 1
    • 0027009056 scopus 로고
    • described their observation of the first stream
    • E. Grün et al., Science 257, 1550 (1992) described their observation of the first stream.
    • (1992) Science , vol.257 , pp. 1550
    • Grün, E.1
  • 2
    • 10544255573 scopus 로고
    • described six streams and suggested a jovian source for these streams
    • E. Grün et al., Nature 262, 423 (1993) described six streams and suggested a jovian source for these streams.
    • (1993) Nature , vol.262 , pp. 423
    • Grün, E.1
  • 3
    • 0010810326 scopus 로고
    • found 5 additional streams in the Ulysses' CDD dataset
    • M. Baguhl et al., Planet. Space Sci. 41, 1085 (1994) found 5 additional streams in the Ulysses' CDD dataset.
    • (1994) Planet. Space Sci. , vol.41 , pp. 1085
    • Baguhl, M.1
  • 4
    • 10544244015 scopus 로고    scopus 로고
    • m = 0 when the CDD axis points as close as possible to ecliptic north. Events of digital amplitude higher than 8 are left out of Fig. 1 as they are largely due to impacts by interstellar grains (2, 3) and nearly all occur between streams. This omission highlights the stream data. With 15 impacts in a stream, and considering the 140° fov of the CDD, the true radiant of a monodirectional stream is known, at 95% confidence, to ± 10°. The spacecraft spin axis is coaligned with the high gain antenna, which points toward the Earth. The central axis of the 140° fov CDD is fixed to point at 85° to the Ulysses spin axis
    • m = 0 when the CDD axis points as close as possible to ecliptic north. Events of digital amplitude higher than 8 are left out of Fig. 1 as they are largely due to impacts by interstellar grains (2, 3) and nearly all occur between streams. This omission highlights the stream data. With 15 impacts in a stream, and considering the 140° fov of the CDD, the true radiant of a monodirectional stream is known, at 95% confidence, to ± 10°. The spacecraft spin axis is coaligned with the high gain antenna, which points toward the Earth. The central axis of the 140° fov CDD is fixed to point at 85° to the Ulysses spin axis.
  • 5
    • 3242826579 scopus 로고    scopus 로고
    • E. Grün et al., Nature 381, 395 (1996).
    • (1996) Nature , vol.381 , pp. 395
    • Grün, E.1
  • 6
    • 0029659614 scopus 로고    scopus 로고
    • E. Grün et al., Science 274, 399 (1996).
    • (1996) Science , vol.274 , pp. 399
    • Grün, E.1
  • 7
    • 10544252922 scopus 로고    scopus 로고
    • Gainesville, FL, 14-18 August 1995, B. S. Gustafson and M. S. Hanner, Eds, Astronomical Society of the Pacific, San Francisco
    • A brief description of stream S8 is given in H. A. Zook et al., Proceedings of the 150th Colloquium of the International Astronomical Union, Gainesville, FL, 14-18 August 1995, B. S. Gustafson and M. S. Hanner, Eds, (Astronomical Society of the Pacific, San Francisco, 1996), vol. 104, p. 23.
    • (1996) Proceedings of the 150th Colloquium of the International Astronomical Union , vol.104 , pp. 23
    • Zook, H.A.1
  • 10
    • 0004207414 scopus 로고
    • R. Schwenn and E. Marsch, Eds., Springer-Verlag, New York
    • F. Mariani and F. M. Neubauer, in Physics of the Inner Heliosphere, R. Schwenn and E. Marsch, Eds., (Springer-Verlag, New York, 1990), pp. 99-181.
    • (1990) Physics of the Inner Heliosphere , pp. 99-181
    • Mariani, F.1    Neubauer, F.M.2
  • 16
    • 10544240629 scopus 로고    scopus 로고
    • m for this stream was 24°
    • m for this stream was 24°.
  • 17
    • 10544239820 scopus 로고    scopus 로고
    • We appreciate review comments by M. Cintala, B. Gustafson, and an anonymous reviewer
    • We appreciate review comments by M. Cintala, B. Gustafson, and an anonymous reviewer.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.