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Volumn 39, Issue 3, 1991, Pages 435-451

Solutions to bi-Maxwellian transport equations for radial solar wind beyond 28 Rs

Author keywords

[No Author keywords available]

Indexed keywords


EID: 33645697301     PISSN: 00320633     EISSN: None     Source Type: Journal    
DOI: 10.1016/0032-0633(91)90005-U     Document Type: Article
Times cited : (15)

References (41)
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    • Barakat1    Schunk2
  • 7
    • 0040102093 scopus 로고
    • Hydrodynamic equations for anisotropic plasmas in magnetic fields, II
    • (1971) Plasma Phys. , vol.13 , pp. 645
    • Chodura1    Pohl2
  • 10
    • 78649981359 scopus 로고
    • Higher order fluid equations for multi-component nonequilibrium stellar (plasma) atmospheres and star clusters II Effects of nonzero relative flow velocities and skewing of velocity distribution functions
    • (1981) The Astrophysical Journal , vol.251 , pp. 297
    • Cuperman1    Weiss2    Dryer3
  • 11
    • 0043049907 scopus 로고
    • Theoretical non-Maxwellian particle velocity distribution functions for spherically symmetric solar wind-like plasma systems and consequences
    • (1983) The Astrophysical Journal , vol.273 , pp. 363
    • Cuperman1    Weiss2    Dryer3
  • 12
    • 84918604708 scopus 로고
    • Theoretical non-Maxwellian particle velocity distribution functions for spherically symmetric solar wind-like plasma systems and consequences II The case of large thermal anisotropy and nine moments description for each species
    • (1987) The Astrophysical Journal , vol.314 , pp. 404
    • Cuperman1    Yatom2    Dryer3    Lewis4
  • 18
    • 33645693934 scopus 로고
    • Solar wind proton velocity distributions: comparison of the bi-Maxwellian based 16-moment expansion with observations
    • (1990) Planet. Space Sci. , vol.38 , pp. 1091
    • Demars1    Schunk2
  • 36
    • 0346581000 scopus 로고
    • Comparison of solutions to the thirteen-moment and standard transport equations for low speed thermal proton flows
    • (1979) Planet. Space Sci. , vol.27 , pp. 433
    • Schunk1    Watkins2


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.