Solar and geomagnetic effects on upper atmospheric temperature
Solar extreme ultraviolet and corpuscular radiation effects on upper atmospheric temperature
ULTRAVIOLET RADIATION↗
SEARCH · Search NASA
Results for “Geomagnetic”
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.
A note on the effect of re-entrant albedo electrons on the measurements of high energy electrons made at geomagnetic latitudes less than or equal to 40 deg
Return of high energy splash albedo electrons to earth investigated under limitations of Stormer theory
ATMOSPHERIC ENTRY↗
Orbital flux integrations within the subsynchronous regions of the geomagnetic cavity, part I
Computer code for calculating omnidirectional vehicle encountered trapped particle fluxes
PARTICLE FLUX↗
Adiabatic motion of outer-zone particles in a model of the geoelectric and geomagnetic fields.
Charged particle motions calculated in model of earth magnetosphere including magnetic and electric field
ATMOSPHERIC ELECTRIC FIELD↗
The solar wind velocity and its correlation with geomagnetic, solar and cosmic ray activity
Explore the source record for details and available documents.
Neugebauer, M.↗
The response of the upper atmospheric temperature to changes in solar EUV radiation and geomagnetic activity
Solar radiation and magnetic effects on upper atmospheric neutral temperatures derived from satellite drag
Chandra, S.↗
Simultaneous measurements on three satellites and the observation of the geomagnetic tail at 1000 R sub E
Comparison of simultaneous magnetic field measurements by Pioneer 7, Explorer 28, and Explorer 33 satellites
Fairfield, D. H.↗
Contraction of the plasmasphere during geomagnetically disturbed periods.
Plasmasphere behavior during solar flare events compared with satellite data from storm-time and plasmapause
Brinton, H. C.↗
Albedo neutron source for high-energy protons trapped in the geomagnetic field.
Absolute intensity measurement of cosmic ray neutrons in atmosphere, obtaining albedo leakage neutron flux near solar minimum
Intriligator, D. S.↗
Pearl-type geomagnetic oscillations.
Sudden commencement of magnetic storm initiating magnetoacoustic oscillations of magnetosphere boundary leading to pearl type micropulsations
Sen, A. K.↗
Simultaneous measurements on three satellites and the observation of the geomagnetic tail at 1000 R sub E.
Simultaneous magnetic field measurements in interplanetary medium in front of earth and in magnetosheath at various earth radii, using satellites
Fairfield, D. H.↗
On the structure of the geomagnetic field at great distances from earth
Solar wind and current sheet considered in determining shape of magnetosphere boundary and calculation of magnetic field lines
Antonova, A. E.↗
Ionospheric and magnetic observations at 1000 kilometers during the geomagnetic storm and aurora of 25-26 May 1967
Correlation between ionospheric electron measurements and transverse magnetic disturbance caused by magnetic storm and aurora
Brace, L. H.↗
Flux and energy spectrum of cosmic-ray electrons at 42 deg north geomagnetic latitude in October 1967.
Cosmic ray electron flux and energy spectrum from balloon data obtained at Palestine, Texas, monitoring proton flux periodically
Frye, G. M., Jr.↗
Interplanetary field and geomagnetic variations a unified view
Explore the source record for details and available documents.
Colburn, D. S.↗
Cosmic-ray positrons and negatrons of energies 10 to 250 MeV at 85 deg geomagnetic latitude
Balloon measurements of cosmic ray positron and negatron intensities near North Pole
Cline, T. L.↗
VLF measurements of the Poynting flux along the geomagnetic field with the Injun 5 satellite
Poynting flux direction for proton whistlers determined from Injun 5 observations, obtaining data on source region and propagation in ionosphere
Gurnett, D. A.↗
Identification and relative abundances of C, N, and O nuclei trapped in the geomagnetic field
C, N and O nuclei abundances in radiation belt near geometric equator, using data obtained by OGO-5 satellite in 1968
Mogro-Campero, A.↗