Results 151 to 160 of about 916 (176)
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Cosmic Research, 2008
A possibility of description of the properties of plasma flow in the magnetosheath using the INME hydrodynamical model is considered on the basis of a comparison with experimental data. This model is characterized by a high degree of self-consistency and, in particular, makes it possible to determine positions of the boundaries of the magnetosheath ...
G. N. Zastenker +4 more
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A possibility of description of the properties of plasma flow in the magnetosheath using the INME hydrodynamical model is considered on the basis of a comparison with experimental data. This model is characterized by a high degree of self-consistency and, in particular, makes it possible to determine positions of the boundaries of the magnetosheath ...
G. N. Zastenker +4 more
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Magnetosheath Interaction with the High Latitude Magnetopause
Surveys in Geophysics, 2005We present both statistical and case studies of magnetosheath interaction with the high-latitude magnetopause on the basis of Interball-1 and other ISTP spacecraft data. We discuss those data along with recently published results on the topology of cusp-magnetosheath transition and the roles of nonlinear disturbances in mass and energy transfer across ...
Savin, S. +25 more
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The magnetosheaths of the outer planets
Planetary and Space Science, 2002Abstract This paper provides a review of past work on the magnetosheaths of the outer planets and also provides the most complete look to date at the plasma parameters in these magnetosheaths. We find that proton distributions in the magnetosheaths of Jupiter, Saturn, and Neptune (but not Uranus) are well represented by two Maxwellians with the same ...
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MHD simulations of the magnetosheath
Advances in Space Research, 1994Ideal magnetohydrodynamic (MHD) simulations of the dayside magnetosheath are reported. The calculations show a depletion layer near the magnetopause and a new stagnation flow structure. The stagnation flow appears to be a generalization of the stagnation line for ideal MHD.
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Ion propagation in the magnetosheath
Journal of Geophysical Research: Space Physics, 1984The transport of test ions through the magnetosheath depends upon the macroscopic structure defined by the average magnetic and flow fields, B0 and U, and the fluctuating fields, δE and δB, encountered by the particles. In this paper an approximate model is used to generate the macroscopic configuration: it satisfies the jump conditions at the bow ...
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Sources of magnetosheath waves and turbulence
Advances in Space Research, 1994Abstract In this paper the possible sources of waves and turbulence in the magnetosheath are discussed. In particular, three separate sources resulting in different types of waves are identified. One is the quasi-parallel portion of the bow shock which contains large amplitude magnetosonic waves generated at or upstream of the shock.
N. Omidi, A. O'Farrell, D. Krauss-Varban
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Planetary and Space Science, 2002
Abstract A review is given of the author's two decades of magnetosheath modeling work with John Spreiter Beginning in the early 1970s, a sequence of computational magnetosheath submodels that extended and refined John's basic model were developed and successfully applied to virtually every planet in the solar system including the terrestrial planets ...
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Abstract A review is given of the author's two decades of magnetosheath modeling work with John Spreiter Beginning in the early 1970s, a sequence of computational magnetosheath submodels that extended and refined John's basic model were developed and successfully applied to virtually every planet in the solar system including the terrestrial planets ...
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On the structure of magnetosheath jets
Plasma structures with the enhanced dynamic pressure, density, or speed are often observed in the Earth’s magnetosheath. These structures, known as magnetosheath (MSH) jets, can be detected downstream quasi-perpendicular and quasi-parallel bow shocks.Kostiantyn Grygorov +4 more
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Large‐Scale High‐Speed Jets in Earth's Magnetosheath: Global Hybrid Simulations
Journal of Geophysical Research: Space Physics, 2022Xueyi Wang, Yu Lin, Yufei Hao
exaly

