The geomagnetic tail.
Satellite observations of geomagnetic tail in magnetosphere near midnight meridian plane, discussing formation, shape, plasma sheet and models
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Satellite observations of geomagnetic tail in magnetosphere near midnight meridian plane, discussing formation, shape, plasma sheet and models
Particle fluxes in outer radiation belt and unstable radiation zone of outer geomagnetic field, discussing electron diffusion into magnetosphere and magnetic disturbances
Magnetosphere model for plasma pressure by solar wind, discussing plasma drift from neutral sheet into geomagnetic tail
Relativistic electron confinement within geomagnetic tail neutral sheet measured by Pioneer 7 deep space probe, confirming kinetic energy observations of IMP 1 satellite
Geomagnetic field westward drift related to earth core rotation from calculating drift at earth surface and at core
Interplanetary magnetic fields from Explorer 33 magnetometer relationship to surface geomagnetic variations emphasizing unified view
Geomagnetic storms and Forbush decreases accounted for by interplanetary solar corpuscular streams effects described by interplanetary magnetic field structure, noting independence of flares
Geomagnetic field model /POGO/ to confirm eccentric dipole westward velocity secular decrease predicted by day length changes
Geomagnetic disturbances and cosmic ray storm of 25-26 May 1967 caused by McMath plage region 8818, noting Forbush decreases and ring current effect
Geomagnetically trapped protons and alpha particles, analyzing OGO 4 data
Low energy particle fluxes in geomagnetic tail, and plasma sheet relation to auroral oval
Geomagnetic survey data reduction results by polar orbiters OGO-2 and OGO-4
Automatic digitized system for processing of geomagnetic data
Drift of noninteracting charged particles in simple geomagnetic field
Configuration of geomagnetic field to determine solar wind-earth interaction
Very low frequency electromagnetic hiss propagation along geomagnetic field in earth magnetosphere
Configuration of geomagnetic tail during substorms
Computer program for transforming spherical harmonic coefficients to geomagnetic dipole coordinates