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Volumn 104, Issue A7, 1999, Pages 14437-14451

Numerical simulation of Alfvénic turbulence in the solar wind

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[No Author keywords available]

Indexed keywords


EID: 3843137630     PISSN: None     EISSN: 21699402     Source Type: Journal    
DOI: None     Document Type: Article
Times cited : (35)

References (16)
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  • 2
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  • 3
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  • 5
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    • Boris, J. P., D.L. Book, Flux corrected transport I: SHASTA A fluid transport algorithm that works, J. Comput. Phys., 11, 38, 1973.
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  • 6
    • 1842838006 scopus 로고
    • Origin of low cross-helicity regions in the inner solar wind
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  • 7
    • 0040321816 scopus 로고
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  • 8
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    • Burlaga, L.F.1    Ogilvie, K.W.2
  • 9
    • 0000218037 scopus 로고
    • A model for the three-dimensional magnetic field correlation spectra of low-frequency solar wind fluctuations during Alfvénic periods
    • Carbone, V., F. Malara, and P. Veltri, A model for the three-dimensional magnetic field correlation spectra of low-frequency solar wind fluctuations during Alfvénic periods, J. Geophys. Res., 100, 1763, 1995.
    • (1995) J. Geophys. Res. , vol.100 , pp. 1763
    • Carbone, V.1    Malara, F.2    Veltri, P.3
  • 10
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  • 11
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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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    • Coleman, P.J.1
  • 12
    • 5244330104 scopus 로고    scopus 로고
    • Solwnd: A 3D compressible MHD code for Solar Wind studies, version 1.0: Cartesian coordinates
    • NASA Goddard Space Flight Cent., Greenbelt, Md.
    • Deane, A., solwnd: A 3D compressible MHD code for Solar Wind studies, version 1.0: Cartesian coordinates, Tech. Rep. CR 4725, NASA Goddard Space Flight Cent., Greenbelt, Md., 1996.
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    • Deane, A.1
  • 13
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  • 14
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  • 15
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  • 16
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    • Evolution of turbulent magnetic fluctuation power with heliospheric distance
    • Zank, G.P., W.H. Matthaeus, and C.W. Smith, Evolution of turbulent magnetic fluctuation power with heliospheric distance, J. Geophys. Res., 101, 17,093, 1996.
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    • Zank, G.P.1    Matthaeus, W.H.2    Smith, C.W.3


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.