1983/02/01 by John R. Burke, D. J. Hollenbach · 6 citations
Engineering · Physics and Astronomy · #Spacecraft and Cryogenic Technologies #Solar and Space Plasma Dynamics #Astrophysics and Star Formation Studies #Interstellar medium #Physics #Helium #Hydrogen #Astrophysics #Astrochemistry #Cosmic dust #Cosmic ray #Trapping #Range (aeronautics) #Interstellar cloud #Atomic physics #Galaxy #Materials science
paper · pdf · doi:10.1086/160667
openalex publication_date 1983/02/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/04
The paper develops a numerical model for calculating thermal accommodation coefficients alpha<SUB>T</SUB> and trapping functions f<SUB>t</SUB> for gases incident on solid surfaces. The method is especially designed for astrophysical applications in that it treats economically and with moderate accuracy (+ or - 20%) the dependences of alpha<SUB>T</SUB> and f<SUB>t</SUB> on finite and different surface and gas temperatures for a large number of gas-surface combinations. In particular, the method is applied to the astrophysical combinations of hydrogen and helium gases incident on graphite, silicon, and ice surfaces. Graphs are presented of the dependence of alpha<SUB>T</SUB> and f<SUB>t</SUB> on interstellar gas temperatures in the range of 10 to 10,000 K and grain temperatures in the range 10 to 1000 K, assuming the current estimates of the gas-surface physical parameters such as the composition and the Debye temperature of the grain material, the repulsive range of the surface potential, and the gas-grain adsorption energy.