Photoelectron heating efficiency in the ionosphere.
Photoelectron heating efficiency in ionosphere, using Thomson scatter data
Engineering topics
Publications and source records attributed to Hanson, W. B..
Photoelectron heating efficiency in ionosphere, using Thomson scatter data
Planetary atmospheres data in 1967 for Venus, Mercury, Mars, Jupiter, Earth, and Moon
Sodium distribution in upper atmosphere investigated in terms of photoionization lifetime, eddy diffusion and scale height
Continuity equation for electrons in F-2 layer obtained for region near geomagnetic equator at noon including photoionization, recombination, drift, etc
Atomic-to-molecular oxygen concentrations ratio values in upper atmosphere used to determine strength of turbulent mixing in atmosphere, noting definition of turbopause height
Ambipolar diffusion parameter calculation by Quinn and Nisbet found erroneous for night F layer
Eddy diffusion and oxygen transport in lower thermosphere
Ionization transport effect on equatorial F region, using numerical solution of steady state continuity equation
Nike-Apache meteorological rocket for investigation of neutral composition of upper atmosphere
Nighttime F layer maintained by hydrogen ions providing source of oxygen ions through charge exchange or by upward drift of ionization
Nighttime F layer maintenance - protonosphere ion source and effective recombination coefficient
Proton diffusion processes in exosphere, noting importance in determining ion scale height above f-2 peak
Lateral flow and other effects contributing to the diurnal variation of the amount of atomic hydrogen in the exosphere
Calculation of atomic hydrogen distribution in interplanetary space based on solar wind measurements
Solar wind distribution of neutral interplanetary hydrogen by interaction with solar protons
Diurnal variation of hydrogen concentration in exosphere
Energy loss processes for fast electrons, electron heating efficiency, heat input to the electron gas, effect of thermal coupling, and electron thermal conductivity above the f2 peak