Astrophysical Phenomena and Radiocarbon
Astronophysical phenomena studied by determination of radiocarbon content in specimens of known age
Kocharov, G. YE.↗
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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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Field theory and astrophysical processes.
Stellar plasma energy loss due to neutrino emission resulting from electromagnetic interaction between plasma and photon
Chiu, H.-Y.↗
Astrophysical evidence for the direct electron- neutrino weak interaction.
Plasma neutrino process of Adams, Ruderman and Woo dependent on direct electron-neutrino interaction and connected with stellar evolution
Chin, C.-W.↗
Satellite orbit analysis at Smithsonian Astrophysical Observatory.
Orbital analysis precision improvement requiring second order oblateness and lunar, air drag and tesseral harmonics perturbations
Gaposchkin, E. M.↗
The precise reduction of Baker-Nunn films at the Smithsonian Astrophysical Observatory.
Computer programs to reduce Baker-Nunn films and maintain time records
Haefner, R. R.↗
Origin of solar wind and its astrophysical aspects
Origin of solar wind, and relation to corona, solar magnetic field, and geomagnetic variations during years of low solar activity
Mustel, E. R.↗
Cosmic-ray electrons and related astrophysical problems
Cosmic distribution of high energy electrons and thermal photons
Ramaty, R.↗
Astrophysical and Geophysical Variations in C 14 Production
Production rate of carbon 14 based on atmospheric neutron measurements and cosmic ray ionization monitor records
Lingenfelter, Richard E.↗
Technical aspects of satellite tracking on IBM computers at Smithsonian Astrophysical Observatory in Cambridge, Massachusetts
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Rossoni, J. P.↗
Introduction to experimental techniques of high-energy astrophysics
Measurements of cosmic rays and high energy extraterrestrial particles
Oegelman, H.↗
Infrared spectra of molecules and materials of astrophysical interest Quarterly progress report, 15 Sep. - 15 Dec. 1970
Vibrational spectra of molecules and solid materials from 4000 to 33 cm in Jovian atmosphere
Durig, J. R.↗
Infrared spectra of molecules and materials of astrophysical interest Quarterly progress report, 15 Dec. 1970 - 15 Mar. 1971
Vibrational spectra of molecules expected in Jovian atmosphere
Durig, J. R.↗
The generation of magnetic fields in astrophysical bodies. II - The galactic field
Galactic magnetic field generation by dynamo process with nonuniform rotation and turbulence in gaseous disk
Parker, E. N.↗
The generation of magnetic fields in astrophysical bodies. III - Turbulent diffusion of fields and efficient dynamos
Galaxy gaseous disk as low mode dynamo, calculating turbulent diffusion coefficient for passive magnetic fields
Parker, E. N.↗
The generation of magnetic fields in astrophysical bodies. IV - The solar and terrestrial dynamos
Earth and sun magnetic field production models as function of dynamo states, discussing solar field effects on terrestrial space environment
Parker, E. N.↗
Magnetic fields in astrophysics
Terrestrial, solar and galactic magnetic fields, discussing generation by combined nonuniform rotation and cyclonic turbulence based on dynamo equation
Parker, E. N.↗