Shock wave structure in recombining low-density plasmas.
Shock wave structure in recombining low density plasma flow, noting electron density and temperature distributions
Christiansen, W. H.↗
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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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Perturbations of the interplanetary magnetic field by the lunar wake.
Interplanetary magnetic field perturbations by lunar wake using plasma flow model
Behannon, K. W.↗
The magnetospheric radiation belt and tail plasma sheet.
Magnetospheric radiation belt and tail plasma sheet, discussing plasma flow from tail, particles release and single model
Piddington, J. H.↗
The polar wind and the terrestrial helium budget.
Helium isotopes escape mechanism from earth atmosphere related to polar wind ionospheric plasma flow from earth
Axford, W. I.↗
Two-dimensional Chapman-Ferraro problem with neutral sheet. II - The interior field.
Chapman-Ferraro approximation for magnetic interior field line configuration in plasma flow around two dimensional dipole, allowing for tail formation and neutral sheet
Atkinson, G.↗
The effect of finite Larmor radius on the perturbation flow mixing of a collisionless plasma
Finite Larmor radius effects on collisionless plasma perturbation flow mixing in velocity distribution functions
Morioka, S.↗
MHD boundary layers with non-equilibrium ionization and finite rates Quarterly report, 1 Mar. - 1 Jun. 1969
Boundary layer over segmented electrode wall in MHD channel when nonequilibrium plasma flows
Reshotko, E.↗
Pulsed electromagnetic gas acceleration Semiannual progress report, 1 Jul. - 31 Dec. 1969
Exhaust velocities of arc plasma flow in pulsed electromagnetic gas accelerator
Clark, K. E.↗
Plasma velocity measurements by Abel-unfolding of Doppler shifts
Cylindrical axial plasma flow fields velocity radial dependence measurement by double-wedge spectroscopy using Abel unfolding of Doppler shifts
Ahlborn, B.↗
Ac electric and magnetic fields and collisionless shock structures
Satellite plasma diagnostics for electric and magnetic fields and fine structure of collisionless shocks in solar wind plasma flows and interplanetary shocks
Fredricks, R. W.↗
Stream-tube analysis used to calculate electron concentration in the presence of accelerating and evaporating water droplets
Determining electron concentration in flowing plasma in presence of accelerating and evaporating water droplets
Bushnell, D. M.↗
Antenna performance in the presence of a turbulent plasma
Antenna radiation patterns and electron density profiles in turbulent plasma flow
Chown, J. B.↗
Several comments concerning a recently proposed magnetospheric model
Magnetospheric model for dynamic plasma flows in polar magnetosphere
Frank, L. A.↗
Applications Technology Satellite /ATS-1/ Suprathermal Ion Detector experiment /SID/ data reduction and analysis Final report, 6 Dec. 1966 - 30 Mar. 1970
Data analysis on ATS-1 Suprathermal Ion Detector /SID/ measurements of low energy plasma flow in magnetopause boundary
Freeman, J. W., Jr.↗
Field line motion during geomagnetic storms
Field line motion accompaning rapid plasma flow during geomagnetic storms
Konradi, A.↗
Magnetospheric electric field properties deduced from simultaneous balloon flights
Magnetospheric electric fields properties via simultaneous balloon flights between plasmapause and polar cap, indicating fields and bulk plasma flow turbulence
Manka, R. H.↗
Time-dependent plasmapause motion
Time dependent plasmapause motion after increase and decrease in magnetic activity based on analytical model of plasma flow
Grebowsky, J. M.↗
A study of waves in the earth's bow shock
The perturbation vectors of waves up and downstream from the region of maximum compression in the bow shock were examined on OGO-5 under particularly steady solar wind conditions. The polarization of the upstream waves was RH, circular and of the downstream waves LH, elliptical in the spacecraft frame. By observing that the polarization of the waves remained unchanged as the shock motion swept the wave structure back and forth across the satellite three times in eight minutes, it was found that the waves were not stationary in the shock frame. A study of the methods of determining the shock normal indicates that the normal estimated from a shock model should be superior to one based upon magnetic coplanarity. The propagation vectors of the waves examined did not coincide with the shock model normal, the average magnetic field, or the plasma flow velocity. However, the major axis of the polarization ellipse of the downstream wave was nearly parallel to the upstream propagation vector.
Holzer, R. E.↗