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    A new parameter to define interplanetary coronal mass ejections

    Russell, C.T. / Shinde, A.A. / Jian, L. | Elsevier | 2005
    of the magnetic pressure and plasma kinetic or thermal pressure. It provides a vehicle for classifying the nature of the ICME encounter and ...

    A Simple Test of the Induced Nature of the Martian Tail

    Russell, C.T. | Online Contents | 1995

    Bow shock motion with two-point observations: Prognoz 7, 8 and ISEE 1, 2; Prognoz 10 and IMP 8

    Zastenker, G.N. / Russell, C.T. / Bridge, H.S. et al. | Elsevier | 1989
    allow us to estimate the nature and velocity of bow shock motion. We have studied this motion with Prognoz 7, 8, 10, ISEE 1, 2 and IMP ...

    Flows and obstacles in the solar wind

    Russell, C.T. / Jian, L. | Elsevier | 2007
    disturbances. Because of their complementary nature we discuss both the disturbances that arise within the solar wind due to the stream structure and ...

    Global hybrid simulations of solar wind interaction with Mercury: Magnetosperic boundaries

    Omidi, N. / Blanco-Cano, X. / Russell, C.T. et al. | Elsevier | 2005
    Dp=64, to examine the nature of the boundaries and discontinuities at the hermean magnetosphere ...

    Interplanetary magnetic field enhancements: Evidence for solar wind dust trail interactions

    Russell, C.T. | Elsevier | 1989
    mode instability. This is further evidence for the comet-like nature of the October 22, 1980 disturbance. ...

    Magnetic flux ropes in the Venus ionosphere: In situ observations of force-free structures?

    Elphic, R.C. / Luhmann, J.G. / Russell, C.T. et al. | Elsevier | 1981
    under a variety of conditions in nature. Filamentary helical magnetic structures are observed to be associated with prominences and flares in ...

    On the nature of ULF waves upstream of planetary bow shocks

    Hoppe, M. / Russell, C.T. | Elsevier | 1981

    Simultaneous observation of upstream waves with ISEE and AMPTE

    Russell, C.T. / Luhmann, J.G. / Elphic, R.C. et al. | Elsevier | 1986
    are most similar at high frequencies and least similar at low frequencies. The position dependent nature of the upstream waves indicates that ...

    The Venus ashen light: Results of the 1988 observing campaign

    Phillips, J.L. / Russell, C.T. | Elsevier | 1992
    weakening the argument that the emissions are auroral in nature. ...

    The visual appearance of comets under varying solar wind conditions

    Russell, C.T. / Guan, L. / Luhmann, J.G. et al. | Elsevier | 1989
    fluid calculations, it is possible to separate the solar wind and cometary ions using the divergenceless nature of the solar wind ions. We then ...