Observations of galactic and extragalactic sources between 50 and 300 microns
Galactic and extragalactic sources of far IR radiation, discussing spectral distribution and luminosities
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Galactic and extragalactic sources of far IR radiation, discussing spectral distribution and luminosities
Extragalactic LF background radiation spectra, using model for free-free absorption in galactic disk
Mn 53 age measurement of galactic cosmic rays
Galactic magnetic field generation by dynamo process with nonuniform rotation and turbulence in gaseous disk
X ray sources identification and position measurements near galactic center on basis of rocket experiments
Galactic cosmic ray solar modulation in interplanetary medium, discussing spherically symmetric model
Solar and galactic cosmic rays interactions with interplanetary magnetic field 28 January-25 February 1967 based on Explorer 33 and 28 satellite observations
Galactic cosmic rays solar modulation effects on fast neutron flux in atmosphere
Galactic center region far IR map in 75-125 microns spectral interval with 6 minute resolution
Soft galactic X rays role in interstellar grains alignment
OSO 3 satellite observations of diffuse X ray emission from galactic plane, eliminating straight line interpolation of spectrum between 3-10 keV X ray range and 100 MeV energy range
Galactic wind as steady radial perfect gas flow from stars and central gravitating source
Galactic plane X ray scan by NASA small astronomy satellite Uhuru, discussing satellite instrumentation, detector and sensor sensitivity and preliminary measurements
Galactic radio source Sagittarius optically thick component evidence based on flux density measurement
Galactic dynamo generated magnetic field periodic modes based on mathematical model involving cyclonic turbulence and nonuniform rotation of gaseous disk
Galactic cosmic ray transport equation numerical solution for interplanetary region, considering modulation, diffusion, convection and energy loss effects
Line emission in diffuse X ray background at high galactic latitudes, interpreting rocket observations
Galactic nucleus thermal emission due to dirty ice or silicate grains, explaining far IR radiation power output and spectral dependence