Effect of magnetic field on heat flow in a polyatomic gas in intermediate pressure range

• Published in: Physica A 1982-01, Vol.111 (3), p.491-512
• Main Authors: Borman, V.D., Krylov, S.Yu, Nikolayev, B.I., Troyan, V.I., Frolov, B.A.
• Format: Article
• Language: English
• ISSN: 0378-4371; 1873-2119
• DOI: 10.1016/0378-4371(82)90047-4

The effect of a magnetic field, B , on heat flow in a gas in an intermediate pressure range has been studied. The ratio of the heat flow changes in the fields B ⊥ ▿T and B ‖ ▿T was found to change nonmonotonically with pressure in N 2 and CO. With the decreasing pressure, a difference is observed between the dependence of heat flow on field orientation and the corresponding angular dependence in the limiting case Kn→0 ( Kn = l/L , l is the mean free path, L is the geometric size). An expression has been obtained for the heat flow in a magnetic field for Kn ≲ 0.1 from the solution of an integral kinetic equation. In particular, it has been shown that the special features of the Senftleben-Beenakker effect observed with the decreasing pressure arise not only due to spherically symmetric molecule-surface interaction, but also to nonspherical scattering on walls.