NASA NTRS · 19730035062
Lunar ash flow with heat transfer.
Abstract
The most important heat-transfer process in the ash flow under consideration is heat convection. Besides the four important nondimensional parameters of isothermal ash flow (Pai et al., 1972), we have three additional important nondimensional parameters: the ratio of the specific heat of the gas, the ratio of the specific heat of the solid particles to that of gas, and the Prandtl number. We reexamine the one dimensional steady ash flow discussed by Pai et al. (1972) by including the effects of heat transfer. Numerical results for the pressure, temperature, density of the gas, velocities of gas and solid particles, and volume fraction of solid particles as function of altitude for various values of the Jeffreys number, initial velocity ratio, and two different gas species (steam and hydrogen) are presented.
Keep this discovery
Explore connections, maps & timelines
Pai, S. I., Hsieh, T., O'Keefe, J. A.. 1972-01-01. Lunar ash flow with heat transfer.. https://ntrs.nasa.gov/citations/19730035062
Cite the original work for its findings. Save a collection to share your selection of sources.