SEARCH · Engineering Papers
Search indexed NASA NTRS and DOE OSTI research on propulsion, heat transfer, battery materials and energy systems. Follow report and document links to the original sources.
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Midlatitude total electron content, peak electron concentration and slab thickness variations with time in ionosphere during magnetic storms
Solar wind interaction with magnetosphere, energy dissipation during magnetic storms and magnetic energy conversion in magnetospheric tail
Polar substorm particle event observed with magnetic field and trapped particle detectors on Explorer 26 during April 1965 worldwide magnetic storm
Storm time radiation belt /ring current/, discussing unsolved problems related to belt formation
Auroras and magnetic storms, with historical review of relevant works from eighteenth century to present, noting work of Birkeland
Magnetopause detection by ATS instruments during January 13-14, 1967 magnetic storm, penetration observed within 6.6 earth radii
Changes in upper ionosphere during severe magnetic storms
Correlation between ionospheric electron measurements and transverse magnetic disturbance caused by magnetic storm and aurora
Possible injection of charged particles into zone of trapped radiation during main phase of magnetic storm
Comparison of post magnetic storm nonadiabatic recovery of geomagnetically trapped protons with radial diffusion
Magnetic field data from OGO-2 spacecraft and surface magnetic observatories, noting magnetic storm occurrence and magnetosphere inflation and detection of polar ionospheric currents
VLF emissions intensity and spectra variations compared with energetic electron fluxes variations during magnetosphere storm periods
Magnetic storm time variations of electron concentrations in upper ionosphere near north geomagnetic pole, discussing magnetic time, altitude and latitude dependence
Simultaneous solution of continuity and heat conduction equations for ionospheric electrons, ions and neutral species for studying F region magnetic storm behavior
Geomagnetic storms and Forbush decreases accounted for by interplanetary solar corpuscular streams effects described by interplanetary magnetic field structure, noting independence of flares
Satellite observations of solar proton events with halo structure or energetic storm proton event and SSC, noting similarity in origin
Geomagnetic disturbances and cosmic ray storm of 25-26 May 1967 caused by McMath plage region 8818, noting Forbush decreases and ring current effect
Topside ionosphere response to magnetic storms, using Explorer 22 satellite electron concentration and temperature measurements