Computer Science – Numerical Analysis
Scientific paper
Aug 1994
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ap%26ss.218..175o&link_type=abstract
Astrophysics and Space Science, vol. 218, no. 2, p. 175-186
Computer Science
Numerical Analysis
Ambient Temperature, Astronomical Models, Electric Current, Magnetic Flux, Magnetohydrodynamic Flow, Plasma Jets, Temperature Dependence, Asymptotic Methods, Grashof Number, Magnetospheres, Numerical Analysis, Prandtl Number, Reynolds Number
Scientific paper
Numerical solution of the effect of current-carrying jets on the temperature of an astrophysical surrounding is carried out using classical magnetohydrodynamic equations. Under the assumption of small hydrodynamic and magnetic Reynolds numbers and invoking a jet magnetic field intensity Btheta, which confines high pressure jets along the z'-axis, a non-linear equation is generated and solved by asymptotic approximation. It is found that when the field intensity is large, the temperature of the surrounding is small and vice-versa. The problem is of interest in the astrophysical studies of current-carrying jets or magnetised radio jets.
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