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The location of the Earth's magnetopause: A comparison of modeled position and in situ Cluster data [PDF]
Journal of Geophysical Research: Space Physics, 2013 Exploiting eight years of magnetic field data from the Cruster mission, we employ an automated magnetopause crossing detection routine to determine the magnetopause location over varying magnetic latitude and local time.
Jim Wild, Nathan A Case
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Magnetopause and Boundary Layer
Space Science Reviews, 2005A brief overview is given of our present knowledge, observational and theoretical, of the structure of the magnetopause and the adjoining plasma boundary layer. Particular attention is given to the relationship between these electromagnetic and plasma structures on the front lobe of the magnetosphere and the magnetic field reconnection process.
de Keyser, J. +8 more
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Planetary and Space Science, 1970
Magnetopause representation by mixing region of plasma streams with different velocities and magnetic fields, assuming hydromagnetic viscosity caused by wave-particle ...
Patrick Cassen, John Szabo
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Magnetopause representation by mixing region of plasma streams with different velocities and magnetic fields, assuming hydromagnetic viscosity caused by wave-particle ...
Patrick Cassen, John Szabo
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Astrophysics and Space Science, 1976
The Magnetosphere-Solar Wind boundary is treated as a tangential discontinuity between collisionless plasma described by C.G.L. equations. An estimate is made, analytically, of the minimum shear speed required to render the interface unstable for propagation in any arbitrary direction.
G. L. Kalra +2 more
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The Magnetosphere-Solar Wind boundary is treated as a tangential discontinuity between collisionless plasma described by C.G.L. equations. An estimate is made, analytically, of the minimum shear speed required to render the interface unstable for propagation in any arbitrary direction.
G. L. Kalra +2 more
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The Structure of the Magnetopause
Planetary and Space Science, 2003Abstract The solar wind is a magnetized flowing plasma that intersects the Earth's magnetosphere at a velocity much greater than that of the compressional fast mode wave that is required to deflect that flow. A bow shock forms that alters the properties of the plasma and slows the flow, enabling continued evolution of the properties of the flow on ...
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Probing the structure of the magnetopause
Science, 2017Magnetospheres The magnetopause is the boundary in space that separates the region dominated by Earth’s magnetic field (the magnetosphere) from the surrounding solar wind. The four spacecraft of NASA’s Magnetospheric Multiscale (MMS) mission have repeatedly flown in formation through the magnetopause, measuring the properties of the plasma and magnetic
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Structure of tangential discontinuities at the magnetopause: the nose of the magnetopause
Journal of Atmospheric and Terrestrial Physics, 1978Abstract Observations show that the magnetopause can sometimes be represented as a tangential discontinuity in the magnetic field. In this paper, we use a theoretical model of steady-state tangential discontinuities to analyze the microscale structure of the nose of the magnetopause.
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Journal of Geophysical Research: Space Physics, 1985
The magnetopause of a symmetric quadrupole embedded in a parallel streaming plasma is calculated by means of the method of the Chapman‐Ferraro problem. The results are discussed with special attention being given to the position of the neutral points for the two symmetric cases of interaction.
M. P. Leubner, K. Zollner
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The magnetopause of a symmetric quadrupole embedded in a parallel streaming plasma is calculated by means of the method of the Chapman‐Ferraro problem. The results are discussed with special attention being given to the position of the neutral points for the two symmetric cases of interaction.
M. P. Leubner, K. Zollner
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On the equilibrium of the magnetopause
Journal of Geophysical Research, 1970The existence of an equilibrium layer between a magnetic field and a field-free stream of cold plasma, moving perpendicularly to the field, was shown many years ago by Ferraro. Recently, Parker treated the interaction of a plasma stream and a magnetic field under somewhat different assumptions.
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