Geomagnetic control of diffusion in the upper atmosphere
Physical mechanisms governing atmospheric diffusion and existence of geomagnetic anomaly in ionosphere
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Physical mechanisms governing atmospheric diffusion and existence of geomagnetic anomaly in ionosphere
New geomagnetic field determination using magnetic survey and observatory annual mean data
Dynamic response determination of geomagnetic field boundary in steady solar wind to small initial disturbance from equilibrium configuration
Cosmic noise absorption data on polar cap analyzed for geomagnetic activity
Cosmic ray neutron monitors in geomagnetic field distorted by solar wind
General Fokker-Planck equation for geomagnetically trapped electron distribution as function of longitude, time, energy, and mirror point field intensity
Rapid geoelectric and geomagnetic variations, diurnal and seasonal variations, and polar aurora
Variation vectors of horizontal component of geomagnetic field of earth - geophysics
Geomagnetically trapped particle radiation - protons and electrons
Magnetic field behavior during development and progress of geomagnetic storm noting polar disturbance role
Asymptotic acceptance cone variation of cosmic ray neutron monitors in geomagnetic field distorted by solar wind, noting particle trajectories
Geomagnetic storm development without preceding enhancement of solar plasma pressure, giving typical Sq storm examples
Fokker-Planck equation for geomagnetically trapped electron distribution as function of longitude, time, energy and mirror-point field intensity
IMP-II and OGO-I measurements on plasma characteristics in transition region between solar wind and geomagnetic field
Magnitude of cosmic ray storms and geomagnetic storms as function of central meridian distance of corresponding solar flares
Explorer XIV plasma probe observations during October 7, 1962 geomagnetic disturbance
Geomagnetic field determination based on information gathered from 1940 to 1963
Vertical cut-off rigidities of cosmic ray for more than 300 positions on Earth surface, using sixth degree simulations of quiescent geomagnetic field