Results 131 to 140 of about 1,340 (198)

Turbulent dynamo in the terrestrial magnetosheath. [PDF]

open access: yesNat Commun
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]

open access: yesNat Commun
Ozaki M   +10 more
europepmc   +1 more source

Universal energy limits of radiation belts in planetary and brown dwarf magnetospheric systems. [PDF]

open access: yesSci Adv
Turner DL   +7 more
europepmc   +1 more source

Design of Three-Dimensional Magnetic Probe System for Space Plasma Environment Research Facility (SPERF). [PDF]

open access: yesSensors (Basel)
Yang J   +9 more
europepmc   +1 more source

A Novel Determination of the Foreshock ULF Boundary: Statistical Approach. [PDF]

open access: yesJ Geophys Res Space Phys
Salohub A   +3 more
europepmc   +1 more source

Observing Cusp High-Altitude Reconnection and Electrodynamics: The TRACERS Student Rocket. [PDF]

open access: yesSpace Sci Rev
Powers BN   +17 more
europepmc   +1 more source

Magnetopause Processes

Space Science Reviews, 2005
Not ...
Phan, T. D.   +9 more
openaire   +4 more sources

Magnetopause and Boundary Layer

Space Science Reviews, 2005
A 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

The viscous magnetopause

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
openaire   +1 more source

Stability of the magnetopause

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
openaire   +1 more source

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