Simulation of non-continuum free jet plume impingement.
Noncontinuum free jet plume impingement simulation, effect of total temperature to model surface temperature ratio, Knudsen number and total enthalpy
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Noncontinuum free jet plume impingement simulation, effect of total temperature to model surface temperature ratio, Knudsen number and total enthalpy
Solid propellant grain design and charge configuration, reviewing dendrite, wagonwheel, star, slotted, conocyl and finocyl grains
Optical depth at under 110 A due to continuous absorption by N, O and Ne ions estimated in high excitation planetary nebulae
Effects of gas rarefaction, compressibility, and turbulence on free stream sphere drag coefficient
Predicting seal leakage rates using modified Hodgon model for rarefied gas viscoseal
Time controllable continuous photon emission from plasma produced by pulsed laser vacuum spark applied to absorption spectroscopy in vacuum UV
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Surface heat transfer rates measured on flat plates in hypervelocity shock tunnel
Aerial and satellite-borne photography of Imperial Valley agricultural land use characteristics
Approximate bridging relations for heat transfer, surface shear and drag in transitional regime between free molecule and continuous flows
Superthermal electrons continuous stream release into interplanetary medium during hectometric solar noise storm activities
Momentum transfer between gas and condensed phase in metallized solid propellant rocket motors, measuring noncontinuum and turbulence effects on sphere drag
The production of cosmic gamma radiation from Compton interactions with low energy photons, bremsstrahlung interactions, cosmic ray induced neutral pion production, and matter-antimatter annihilation is discussed.
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Explore the source record for details and available documents.
Explore the source record for details and available documents.
Explore the source record for details and available documents.
Observations of the variability of the 1.35-cm H2O and 2.2-micron emission from eight late M stars are described. A comparison of the microwave and infrared variations is of interest because the bulk of the stellar energy is radiated in the near-infrared and because at least one theory (Litvak 1969) hypothesizes near-infrared maser pumping via the 2.7-micron H2O vibration-rotation band. Variations at the two wavelengths appear to be correlated and possible explanations for this correlation are discussed.