Geomagnetically trapped alpha particles
Geomagnetically trapped alpha particles from Injun IV satellite measurements
SEARCH · Search NASA
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.
Quote a phrase for an exact phrase match. Source license links do not imply unrestricted reuse.
Geomagnetically trapped alpha particles from Injun IV satellite measurements
Source mechanisms responsible for generating geomagnetic micropulsations
Response of geomagnetic activity index to interplanetary magnetic field
Comparison between diurnal geomagnetic field and cosmic ray intensity variations
Energetic electron precipitation and 5 to 40 second geomagnetic micropulsations relation to auroral substorms
Geomagnetic and auroral storms provide information on interaction of solar plasma flows and magnetosphere
Interplanetary magnetic field and plasma effect on geomagnetic activity during quiet sun conditions
IMP-I satellite measurements of neutral sheet in geomagnetic tail noting dimensions, motion and parameters of sheet
Magnetosheath field, geomagnetic activity index, magnetopause stability and interplanetary magnetic field influence on magnetospheric phenomena
Growth rate along whistler path for waves propagating at angle to geomagnetic field
Energy spectrum of primary cosmic ray alpha particles measured by nuclear photographic emulsion, estimating geomagnetic cut-off energies
Geomagnetic and solar control of ionization at 1000 km determined from electron density data obtained from Alouette satellite
Satellite measurement of upper atmospheric density variations due to geomagnetic disturbances, correlating time delay with geographic latitude
IMP-II and OGO-I measurements on plasma characteristics in transition region between solar wind and geomagnetic field
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