Comparison of predictions of an MHD model solar wind flow past the magnetopause with AMPTE/IRM observations on 24 October, 1985

被引:0
作者
机构
来源
Advances in Space Research | / 22卷 / 01期
关键词
D O I
暂无
中图分类号
学科分类号
摘要
引用
收藏
页码:67 / 72
相关论文
共 3 条
  • [1] A comparison of predictions of an MHD model solar wind flow past the magnetopause with AMPTE/IRM observations on 24 October, 1985
    Farrugia, CJ
    Biernat, HK
    Erkaev, NV
    Kistler, LM
    SOLAR-TERRESTRIAL RELATIONS: PREDICTING THE EFFECTS ON THE NEAR- EARTH ENVIRONMENT, 1998, 22 (01): : 67 - 72
  • [2] MHD model of magnetosheath flow: comparison with AMPTE/IRM observations on 24 October, 1985
    Farrugia, CJ
    Biernat, HK
    Erkaev, NV
    Kistler, LM
    Le, G
    Russell, CT
    ANNALES GEOPHYSICAE-ATMOSPHERES HYDROSPHERES AND SPACE SCIENCES, 1998, 16 (05): : 518 - 527
  • [3] MHD model results of solar wind interaction with Mars and comparison with MAVEN plasma observations
    Ma, Y. J.
    Russell, C. T.
    Fang, X.
    Dong, Y.
    Nagy, A. F.
    Toth, G.
    Halekas, J. S.
    Connerney, J. E. P.
    Espley, J. R.
    Mahaffy, P. R.
    Benna, M.
    McFadden, J. P.
    Mitchell, D. L.
    Jakosky, B. M.
    GEOPHYSICAL RESEARCH LETTERS, 2015, 42 (21) : 9113 - 9120