PROCEEDINGS OF THE SECOND INTERNATIONAL SYMPOSIUM ON RAREFIED GAS DYNAMICS
Rarefied gas dynamics - molecular beams and surface interactions, free-molecular flow, fluid mechanics, kinetic theory
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Rarefied gas dynamics - molecular beams and surface interactions, free-molecular flow, fluid mechanics, kinetic theory
Rarefied gas dynamics - transition flow in gases of simple, nonreacting, electrically neutral molecules
Rarefied gas dynamics - kinetic theory, solutions of boltzmann equation, molecular beams and surface interactions
Molecular approach to rarefied gas dynamics
Second international symposium on rarefied gas dynamics totaling 40 individually abstracted papers on related topics, edited by l. talbot
The current state of those aspects of rarefied gas dynamics research that appear to be most important to research planned over the next decade is evaluated. These aspects encompass assessments of computational rarefied-gas dynamics (CRGD) that will allows their use as surrogates for experiments, the development of hybris-flowfield computational techniques matching continuum computations with particle computations, and the validation of CRGD through the results of experimental studies of Knudsen layers in simple flows. The design of surfaces for the achievement of stable, low-momentum and thermal accommodation coefficients will be a major priority, together with theorization and experimentation on evaporation and condensation effects close to surfaces.
Rarefied gas dynamics - Conference, Oxford University, July 1966, Volume I
Rarefied gas dynamics - conference, Oxford University, July 1966
Rarefied gas dynamics, Advances in applied mechanics - International Symposium, University of Toronto, July 1964
Rarefied gas dynamics - International Symposium, Institute for Aerospace Studies, University of Toronto, July 1964, Volume 1
Rarefied gas dynamics - Conference, Cambridge, Mass., July 1968, Volume 2
Rarefied gas dynamics - Conference, Cambridge, Mass., July 1968, Volume 1
Monte Carlo method, and radiant heat transfer to analyze impact pressure probes
When the conditions of flow are rarefied and hypersonic, a more suitable alternative to the use of the Navier-Stokes equations for developing a numerical solution is the Direct Simulation Monte Carlo method (DSMC), a method of simulation which employs a large number of particles in modeling a rarefied gas. The performance of a parallel DSMC code developed for the Intel iPSC/860 Touchstone Gamma prototype computer is studied and the scaleup is found to be very nearly over the range of 16-128 processors.
Conference on transition flow, surface interactions, kinetic theory, molecular beams, internal flow, and rarified plasmas and shock structures
Recent studies in the theory of rarefied gases (kinetic theory, shock structure, molecular forces and interactions, evaporation and condensation, expansions and jets, flow past bodies, gas-solid interactions) are presented along with descriptions of numerous experiments in these areas. Some of the topics covered include: singular limits of solutions of Boltzmann's equations, the Boltzmann and Klimontovich formalisms with reference to turbulent resolution, higher-order kinetic theory for the Lorentz gas, intermolecular potentials from shock structure experiments, cooling of particles in aerosol beams, hypersonic-subsonic transition in spherically symmetric expanding flows, absolute velocity measurements in a rarefied gas flow by an ion time-of-flight technique, the product distribution of gas-solid reactions from absolute rate theory, and relaxation of a gas with internal degrees of freedom. Individual items are announced in this issue.
Interplanetary space provides simultaneously the best vacuum available to man and, because of the solar wind, a tenuous and unsteady high-speed outflow of predominantly hydrogen gas from the sun, a remarkable variety of rarefied gasdynamics phenomena to observe. This paper provides a review of these phenomena, and of the way in which the present level of understanding has been achieved.
Interplanetary space provides simultaneously the best vacuum available to man and, because of the solar wind, a tenuous and unsteady high-speed outflow of predominantly hydrogen gas from the sun, a remarkable variety of rarefied gasdynamics phenomena, to observe. A review is provided of these phenomena, and of the way in which the present level of understanding has been achieved.