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Computations of ion diffusion coefficients from the Boltzmann-Fokker-Planck equationThe Boltzmann-Fokker-Planck equation is solved with the Chapman-Enskog method of analysis for the velocity distribution functions of helium, carbon, nitrogen, and oxygen. The analysis is a perturbation scheme based on the assumption of a collision-dominated gas, and the calculations are carried out to first order. The elements considered are treated as trace constituents in an electron-proton gas. From the resulting distribution functions, diffusion coefficients are computed which are found to be 20-30% less than those obtained by Chapman and Burgers. In addition, it is shown that the return current of cold electrons needed to maintain quasi-neutrality in a plasma with a temperature gradient contributes a term in the thermal diffusion coefficient omitted erroneously in previous works. This added term resolves the longstanding controversy over the discrepancy between the coefficients of Chapman and Burgers, which are seen to be completely equivalent in the light of this analysis. The viscosity coefficient for an electron-proton gas is also computed and found to be 7% less than that obtained by Braginskii.
Document ID
19810041905
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Roussel-Dupre, R.
(Colorado, University Boulder, Colo.; Hawaii, University, Honolulu, Hawaii, United States)
Date Acquired
August 11, 2013
Publication Date
January 1, 1981
Publication Information
Publication: Astrophysical Journal
Subject Category
Atomic And Molecular Physics
Accession Number
81A26309
Funding Number(s)
CONTRACT_GRANT: NSF GA-31477
CONTRACT_GRANT: NSF ATM-78-22202
CONTRACT_GRANT: NSG-7536
CONTRACT_GRANT: NAS5-22409
Distribution Limits
Public
Copyright
Other

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