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Volumn 286, Issue 5448, 1999, Pages 2319-2320

Deflection of the local interstellar dust flow by solar radiation pressure

Author keywords

[No Author keywords available]

Indexed keywords

GRAPHITE;

EID: 0033579381     PISSN: 00368075     EISSN: None     Source Type: Journal    
DOI: 10.1126/science.286.5448.2319     Document Type: Article
Times cited : (63)

References (38)
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    • note
    • The data sets contain data from 804 days of Ulysses measurements between 2 and 4 AU and 822 days outside 4 AU. Galileo spent 598 days between 2 and 4 AU and 632 days outside 4 AU before it arrived at Jupiter. To compare the 2- to 4-AU and >4-AU mass histograms, we scale the 2- to 4-AU histogram of the Ulysses data by 822/804 and the 2- to 4-AU histogram of the Galileo data by 632/598.
  • 25
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    • note
    • 6 interstellar grains are destroyed by a collision in this region.
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    • J. P. Bradley et al., Science 285, 1716 (1999).
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    • note
    • We thank A. L. Graps for improving the clarity of the text. This work was performed while M.L held a position funded by the program on physics of star formation at the Deutsche Forschungsgemeinschaft. We also thank M. Mischenko for making his T-matrix light scattering code for bispheres available, Y.-I. Xu for calculating scattering by bispheres and larger clusters of spheres using his boundary condition code, and L. Kolokolova for performing the T-matrix light scattering calculations for bispheres. Supported in part by NASA grant NAGS-6378.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.