Radioactive debris over Fairbanks, Alaska, on February 18, 1965.
Radioactive debris over Fairbanks, Alaska, on February 18, 1965, investigating bremsstrahlung X-rays in auroral zone
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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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Radioactive debris over Fairbanks, Alaska, on February 18, 1965, investigating bremsstrahlung X-rays in auroral zone
Printouts and graphs of rocket winds, radiosonde observations and/or thermodynamics of February 1966 firings of Meteorological Rocket Network
Time history and energy spectra of solar proton flare on February 5, 1965
Solar energetic particle intensities obtained with Mariner IV and Injun IV during 5-12 February 1965 cosmic ray event
Solar particle event of February 1965 observation with Mariner IV and Injun IV showing 70 degrees heliocentric longitudinal distribution in interplanetary space
The objective of this test program was to determine the behavior of gas-saturated water and nitrogen tetroxide under various flow and pressure drop conditions. A second part of the test program is to be conducted at a later time to determine the rate of gas diffusion into propellants. The test program was conducted by the Fluid Systems Test Section of the Thermochemical Test Branch for the Auxiliary Propulsion and Pyrotechnics Branch, Propulsion and Power Division. Testing was accomplished at the Fluid Systems Test Facility during the period from February 2, 1966, to May 3, 1966.
Solar particle observations from 24 January to 24 February 1967 correlated with solar flare activity
Heliocentric longitude intensity profiles of protons associated with solar flare of 5 February 1965, discussing data from Mariner 4 and IMP 2
Coronal condensation spectra during 4 February 1962 total eclipse, determining abundances, ionization equilibria, electron densities, etc, from Fe and Ca XV lines analysis
Interplanetary magnetic field measurements by Pioneer 8 during 25 February 1969 solar activity, discussing geomagnetic storms, cosmic rays, shock fronts and ionospheric disturbances
Solar and galactic cosmic rays interactions with interplanetary magnetic field 28 January-25 February 1967 based on Explorer 33 and 28 satellite observations
Meteorological observations and instrumentation - Conference, Washington, D.C., February 1969
This index is intended to serve as a ready reference tool for the names, places and events that comprise the history of John F. Kennedy Space Center. The period covered is December 1962 through February 1972. The arrangement is alphabetical by subject; under each subject, entries are arranged alphabetically by title. To facilitate use, cross references and scope notes have been provided.
The solar particle events of 18 November 1968, 25 February 1969, and 30 March 1969 were studied using data from the detector system aboard the lunar orbiting satellite Explorer 35. Protons, alpha particles, and Z or = 3 nuclei were registered in the solid state detector of the system. Interplanetary propagation, particle anisotropy, and the intensity ratios of protons to alpha particles and of alpha particles to C, N, and O nuclei above a common specific energy of 0.5 MeV/nucleon were studied. Diffusion coefficients and decay constants for the three events are given, as well as magnitudes and directions of anisotropies.
The earth's bow shock exhibited a clean laminar profile at low Mach number as it crossed and recrossed Ogo 5, Heos 1, and Explorer 33 on February 12, 1969. The approximate 120 earth radii distance between Heos and Explorer during one set of crossings indicated the abrupt character of the laminar shock 'front' and the absence of magnetosheath turbulence both in the dayside hemisphere above the ecliptic and in the flank of the shock 75 earth radii behind the earth and below the ecliptic. The abruptness of the shock and coplanarity of the loci of Ogo and Heos with the local shock normal permit the most reliable estimates yet obtained of shock velocities along the normal. These mean velocities ranged from 11 to at least 100 km/sec over distances of 2-7 earth radii.
Observations were made of the total lunar eclipse on February 10, 1971 at a wavelength of 3.1 mm at the Millimeter Wave Observatory of the University of Texas at Austin. Eclipse cooling curves obtained for Copernicus, Mare Serenitatis, and a mountainous region indicate maximum temperature decreases of 6.77%, 6.37%, and 7.51%, respectively. Cooling rates of about 6 K/hour were measured. The normalized solar insolation has also been calculated for each region.
This special bibliography lists 322 reports, articles, and other documents introduced into the NASA scientific and technical information system in February 1973.
Documentation of data acquired from the Nimbus 4 Meteorological Satellite for the period from 1 January to 28 February 1971 is provided. Included are the types of data available, anomalies in the data, geographic location, and time notations.