Hydromagnetic Ekman layer on convective heat generating fluid in slip flow regime

Details Hydromagnetic Ekman layer on convective heat generating fluid in slip flow regime Hydromagnetic Ekman layer on convective heat generating fluid in slip flow regime

Jun 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.168..103r&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 168, no. 1, June 1990, p. 103-109.

Astronomy and Astrophysics

Astrophysics

Convective Heat Transfer, Ekman Layer, Magnetohydrodynamic Flow, Rotating Fluids, Slip Flow, Cyclotron Frequency, Hall Effect, Magnetic Flux, Rarefied Gas Dynamics

Scientific paper

The velocity and temperature distributions for a free convective
heat-generating rarefied gas in a rotating frame of reference are
analyzed for the case when a strong magnetic field is imposed in a plane
which makes an angle alpha with the normal to the plate. The effects of
Hall current, heat source parameter, and rarefaction are examined.

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