Some astrophysical instrumentation considerations related to space optical technology
Astrophysical instrumentation considerations related to space optical technology
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Astrophysical instrumentation considerations related to space optical technology
Relativity theory and astrophysics - Conference, Ithaca, July-August 1965, Volume 1, Relativity and cosmology
Relativity theory and astrophysics, Volume 2, Galactic structure
Relativity theory and astrophysics, Volume 3, Stellar structure
Solar, stellar, galactic and extragalactic neutrino astrophysics, discussing observational data on sources, nuclear processes, detection and cosmology
Magnetic field lines of force random walk and astrophysical magnetic fields random fluctuations, noting interplanetary magnetic field and solar photosphere turbulence
Equilibrium generation and maintenance of supraluminous waves with phase velocities in excess of light in collisionless thermal astrophysical plasmas
Smithsonian Astrophysical Observatory satellite observation program, discussing mathematical procedures to transform reduced data in celestial frame to fixed earth plane
Possible applications of continuity equation plasma oscillations to other periodic astrophysical phenomena
High energy astrophysics of cosmic radiation and galaxies
F values for Ti II, Cr II and Fe II by empirical astrophysical line strength analysis, discussing f value determination from stellar growth curve
Plasma acceleration away from rotating magnetized astrophysical objects analyzed and applied to pulsar NP 0532 for magnetic moment and mass loss rate calculations
Nonthermal phenomena of astrophysics in relation to plasma physics, considering planetary and stellar regions, supernova envelopes, interstellar medium, cosmic rays, radio galaxies, etc
Infrared and ultraviolet spectroscopy of solar radiation, astrophysics, and interplanetary diffusion
Internal energy partition function of atom or ion immersed in plasma - astrophysical application
Infrared spectra of molecules and materials of astrophysical interest Quarterly progress report, 15 Jun. - 15 Sep. 1970
Atomic configurations population inversions of astrophysical interest, assuming excitation by electron collisions, solving rate equations for level populations by computer
CH, CD and CH ion excited states decay rates determined from phase shift and frequency data, discussing implications for astrophysics