Astronomy and Astrophysics – Astrophysics
Scientific paper
Jan 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985a%26a...142..375n&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 142, no. 2, Jan. 1985, p. 375-377.
Astronomy and Astrophysics
Astrophysics
4
Cosmic Plasma, Jet Flow, Magnetohydrodynamics, Plasma Jets, Turbulent Jets, Viscous Flow, Boundary Layers, Brightness Distribution, Dirac Equation, Navier-Stokes Equation, Reynolds Number
Scientific paper
Sets with inhomogeneous turbulent velocity are studied analytically taking account of the magnetic fields, for cases where the fields are parallel to the velocities. It is demonstrated that hydromagnetic flows of self-similar type in constant-pressure environment are equivalent to hydrodynamic jet flows with different velocity and viscosity. Moreover, significant radiation associated with the brightness distribution was observed only inside a jet; the location of the hydromagnetic beam is defined. Finally, it is noted that to maintain a hydrodynamic or hydromagnetic jet a highly directional central source and fluid whose turbulent properties can be described using turbulent viscosity are necessary.
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