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Volumn 103, Issue A2, 1998, Pages 2085-2097

The radial and latitudinal dependence of the cosmic ray diffusion tensor in the heliosphere

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[No Author keywords available]

Indexed keywords


EID: 0000577509     PISSN: None     EISSN: 21699402     Source Type: Journal    
DOI: None     Document Type: Article
Times cited : (146)

References (12)
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    • Bieber, J. W., W. Wanner, and W. H. Matthaeus, Dominant two-dimensional solar wind turbulence with implications for cosmic ray transport, J. Geophys. Res., 101, 2511, 1996.
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    • Bieber, J.W.1    Wanner, W.2    Matthaeus, W.H.3
  • 7
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    • Radial variations of large-scale magnetohydrodynamic fluctuations in the solar wind
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    • Burlaga, L.F.1    Goldstein, M.L.2
  • 8
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    • Turbulence, viscosity and dissipation in the solar wind plasma
    • Coleman, P.J., Turbulence, viscosity and dissipation in the solar wind plasma, Astrophys. J., 153, 371, 1968.
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  • 9
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    • Distance to the solar wind termination shock and the source flux of anomalous cosmic rays during 1986-1988
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    • Cummings, A.C.1    Stone, E.G.2    Webber, W.R.3
  • 10
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    • The interactions of energetic particles with the solar wind
    • edited by C.F. Kennel, L.J. Lanzerotti, and E.N. Parker, North-Holland, Amsterdam
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  • 11
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    • Cosmic ray streaming perpendicular to the mean magnetic field
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  • 12
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    • Transport and turbulence modeling of solar wind fluctuations
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    • Zhou, Y.1    Matthaeus, W.H.2


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.