Possible applications of the continuity- equation plasma oscillation to pulsars and other periodic astrophysical phenomena
Possible applications of continuity equation plasma oscillations to other periodic astrophysical phenomena
Roth, J. R.↗
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Current problems of high energy astrophysics
High energy astrophysics of cosmic radiation and galaxies
Oegelmann, H. B.↗
Astrophysical determination of f-values for TiII, CrII, FeII.
F values for Ti II, Cr II and Fe II by empirical astrophysical line strength analysis, discussing f value determination from stellar growth curve
Aller, L. H.↗
Hydromagnetic plasma acceleration by rapidly rotating astrophysical objects.
Plasma acceleration away from rotating magnetized astrophysical objects analyzed and applied to pulsar NP 0532 for magnetic moment and mass loss rate calculations
Michel, F. C.↗
Nonthermal phenomena of astrophysics and their relation to plasma physics.
Nonthermal phenomena of astrophysics in relation to plasma physics, considering planetary and stellar regions, supernova envelopes, interstellar medium, cosmic rays, radio galaxies, etc
Cameron, A. G. W.↗
Astrophysics and astronomy
Infrared and ultraviolet spectroscopy of solar radiation, astrophysics, and interplanetary diffusion
Source record↗
Calculations of astrophysical partition functions
Internal energy partition function of atom or ion immersed in plasma - astrophysical application
Hagyard, M. J.↗
Infrared spectra of molecules and materials of astrophysical interest Quarterly progress report, 15 jun. - 15 sep. 1970
Infrared spectra of molecules and materials of astrophysical interest Quarterly progress report, 15 Jun. - 15 Sep. 1970
Durig, J. R.↗
Population inversions in ions of astrophysical interest
Atomic configurations population inversions of astrophysical interest, assuming excitation by electron collisions, solving rate equations for level populations by computer
Smith, H. A.↗
Probabilities for radiation and predissociation. II - The excited states of CH, CD, and CH/plus/, and some astrophysical implications
CH, CD and CH ion excited states decay rates determined from phase shift and frequency data, discussing implications for astrophysics
Hesser, J. E.↗
Astrophysical determination of the coupling constant for the electron-neutrino weak interaction
Electron-neutrino weak interaction and beat decay coupling constants found nearly equal, describing astrophysical tests based on white dwarf stars luminosity intervals
Stothers, R. B.↗
Astrophysical implications of the continuity equation plasma oscillation
Continuity equation plasma oscillation, discussing ion current waveform flowing from discharge and implications for periodic astrophysical phenomena
Roth, J. R.↗
Astrophysical exclusion of photon-neutrino weak coupling
Photon-neutrino coupling theory of weak interactions, noting exclusion by astrophysical data for white dwarfs
Stothers, R. B.↗
The generation of magnetic fields in astrophysical bodies. V - Behavior at large dynamo numbers
Astrophysical objects magnetic field generation, examining behavior at large dynamo numbers
Parker, E. N.↗
Intense magnetic fields in astrophysics
Intense magnetic fields in astrophysics, emphasizing flux conservation law and quantum effects
Canuto, V.↗
Critical review of ultraviolet photoabsorption cross sections for molecules of astrophysical and aeronomic interest
Astrophysical and aeronomic UV molecular photoabsorption cross sections, discussing experimental techniques and associated systematic and random errors
Hudson, R. D.↗
High energy astronomy or astrophysics and properties of the interplanetary plasma
The research activities related to high energy astrophysics and interplanetary plasma are reported. The experimental work in the following areas are described: (1) balloon-and rocket-borne cosmic X-ray, (2) X-ray spectroscopy, and (3) OSO-3 gamma ray experiment. Plasma studies in the interplanetary region, magnetosphere, and geomagnetic tail are included.
Source record↗
Charged-particle transport in turbulent astrophysical plasmas
The effect of electromagnetic fluctuations, or plasma turbulence, on the motion of the individual particles in a plasma is investigated. Two alternative methods are used to find a general equation governing the time-evolution of a distribution of charged particles subject to both an external force field and the random fields of the fluctuations. It is found that, for the high-temperature, low-density plasmas frequently encountered in the study of astrophysics, the presence of even a small amount of turbulence can have a very important effect on the behavior of the plasma. Two problems in which turbulence plays an important role are treated.
Newman, C. E., Jr.↗