Results 131 to 140 of about 1,340 (198)
Turbulent dynamo in the terrestrial magnetosheath. [PDF]
Vörös Z +12 more
europepmc +1 more source
Nonlinear spatiotemporal signatures of whistler-mode wave activity around Mercury during six flybys of BepiColombo mission. [PDF]
Ozaki M +10 more
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Universal energy limits of radiation belts in planetary and brown dwarf magnetospheric systems. [PDF]
Turner DL +7 more
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Design of Three-Dimensional Magnetic Probe System for Space Plasma Environment Research Facility (SPERF). [PDF]
Yang J +9 more
europepmc +1 more source
A Novel Determination of the Foreshock ULF Boundary: Statistical Approach. [PDF]
Salohub A +3 more
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Observing Cusp High-Altitude Reconnection and Electrodynamics: The TRACERS Student Rocket. [PDF]
Powers BN +17 more
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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
openaire +3 more sources
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
openaire +1 more source

