Solar and geomagnetic effects on upper atmospheric temperature.
Satellite drag analysis of atmospheric temperatures noting effects of UV, solar radiation and geomagnetic fluctuations
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Satellite drag analysis of atmospheric temperatures noting effects of UV, solar radiation and geomagnetic fluctuations
Dayside distortion of geomagnetic field by solar wind beyond 3.5 earth radii measured and compared with three magnetosphere models
Geomagnetic field boundary observations by Explorer XII
Main geomagnetic field data, discussing data conversion to computer-readable form
Charged particles of extraterrestrial ring current during geomagnetic storms, with Ogo 3 measurements of proton and electron differential energy spectrums
Geomagnetic tail at 1000 earth radii, noting possibility of magnetic force lines connected to earth and tail geometry
Alpha particle proton ratio of geomagnetic field from data from charged-particle telescope on OGO 1 satellite
Reversible betatron acceleration mechanism during geomagnetic storm
Quiet condition solar wind geomagnetic field interaction measurements, discussing solar plasma and bow shock wave generation
Mariner IV flight magnetometer data, determining interplanetary field and geomagnetic variability relationship
Fokker-Planck equation describing distribution of geomagnetically trapped electrons as function of longitude, time, energy and mirror-point field intensity
Numerical program integrating motion equation of charged particles from realistic geomagnetic field model, with trajectory calculations for solar cosmic rays
Growth and decay of geomagnetic storms of April 17-18, 1965 studied using data from 88 ground stations, Explorer XXVI and Vela satellites
Electron precipitation following geomagnetic storm sudden commencement
Solar coronal mass ejections (CMEs) can cause hazadous high-energy particles and geomagnetic storms that, in the more serious instances, can disrupt Earth power grids, communications, and satellites.
Solar wind phenomena leading to different types of geomagnetic activity are discussed.
This paper studies the ionospheric response to major geomagnetic storm of October 18-19, 1995, using the thermosphere-ionosphere electrodynamic general circulation model (TIE-GCM) simulations and the global ionospheric maps (GIM) of total electron content (TEC) observations from the Global Positioning System (GPS) worldwide network.
Two distant ISEE-3 geomagnetic tail passes have been examined to identify all slow-mode shocks present in the data. We find a total of 86 events from 439 plasmasheet/lobe crossings, using five criteria based on relations between the upstream lobe and the downstream plasmasheet magnetic field and plasma measurements. The statistical results of slow-mode shock parameters such as the angle between magnetic field and shock normal, Theta(sub bn), Alfven Mach number along the normal direction, M(sub an), and electron beta, Beta(sub e), are calculated and reported.