Thermosphere conditions deduced from satellite observations.
Atmospheric composition data from Explorer XVII SATELLITE, obtaining expression for thermal diffusion factor of He
EXPLORER XVII SATELLITE↗
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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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Intrinsic Magnetic Properties of the Lunar Body
Preliminary analysis of magnetic measurements by Explorer 35 in lunar orbit suggested an upper limit of 4 x 10(exp 20) gauss-cm3 for the magnetic moment of the moon. A more detailed analysis of a larger body of Explorer 35 data from measurements in the earth's magnetic tail has subsequently been performed. Reversal of the ambient tail field by 180deg when the moon and spacecraft traverse the neutral sheet permits a separation of permanent and induced field contributions to the total field observed near the moon. When compared to calculated permanent and induced field effects, the results of this analysis lead to new upper limits of 102' gauss-cm3 on the lunar magnetic moment and 4y on the lunar surface field. Limiting the moment induced in the moon by the magnetotail field permits an upper limit of 1.8 to be set on the bulk relative magnetic permeability of the moon.
Behannon, Kenneth W.↗
The geomagnetic tail - Topology, reconnection and interaction with the moon
Explorer 33 data used to assess geometry and lunar interaction of geomagnetic tail
Colburn, D. S.↗
Velocity axis response of an ion mass spectrometer on a spherical satellite
Velocity axis response of ion mass spectrometer on spherical satellite calculated based on Explorer 32 data
Toner, M. G.↗
Configuration and reconnection of the geomagnetic tail.
Geomagnetic tail configuration and reconnection data from Explorer 33 satellite, noting skewing of field lines
Colburn, D. S.↗
An empirical evaluation of radial diffusion coefficients for electrons of 50-100 kev from L equals 4 to L equals 7.
Radial diffusion coefficients calculated for 50- 100 kev electrons using equilibrium fluxes determined from Explorer 12 data
Kavanagh, L. D., Jr.↗
Photoelectron flux and protonospheric heating during the conjugate point sunrise
Explorer 31 data for photoelectron flux and protonospheric heating during conjugate point sunrise
Maier, E. J. R.↗
Research at the Stanford Center for Radar Astronomy Semiannual status report, 1 Jan. - 30 Jun. 1969
Data reduction and analysis of bistatic radar data from Explorer 35 - bibliographies
Eshleman, V. R.↗
Interaction of the solar wind with the moon
Solar wind interaction with lunar far side and near side surface, and lunar magnetic fields from Explorer 35 data
Ness, N. F.↗
Cosmic ray and solar flare electrons
Cosmic ray electrons and solar flare particles by OGO-E and Explorer 33 data for identifying solar flare electrons
Cline, T. L.↗
Bow shock associated waves observed in the far upstream interplanetary medium.
Earth bow shock waves in far upstream interplanetary medium observed from magnetic data of Explorer 34 satellite
Fairfield, D. H.↗
Ionospheric electron content at midlatitudes near the minimum of the solar cycle.
Ionospheric vertical columnar electron content at midlatitudes near solar cycle minimum based on Faraday rotation data from Explorer 22
Lawrence, R. S.↗
MeV particles in the outer zone - Explorer 12
Explorer 12 data on MeV particles in outer space
Kaufmann, R. L.↗
The midlatitude ionization trough during the rising solar cycle
Midlatitude ionization trough during rising solar cycle using data from Explorer 22
Miller, N. J.↗
Stanford telemetry monitoring experiment on Lunar Explorer 35 Final report
Explorer 35 data analysis including occultation study and antenna pattern interpretation along with electromagnetic property experiments
Ingalls, D. H. H.↗
Observations of the lunar Mach cone
Confirming existance of lunar Mach cones by magnetometer data from Explorer 35
Ness, N. F.↗
Interaction of the solar wind with the moon
Interaction of solar wind with moon, and Explorer 35 data
Ness, N. F.↗
Energy transfer at colliding streams in the solar wind
Measuring energy transfer at colliding streams in solar wind based on data from Explorer 34 and Vela 4B satellites
Bame, S. J.↗