Astronomy and Astrophysics – Astrophysics
Scientific paper
Jan 1997
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997a%26a...317..630b&link_type=abstract
Astronomy and Astrophysics, v.317, p.630-635
Astronomy and Astrophysics
Astrophysics
14
Radiative Transfer, Methods: Analytical
Scientific paper
Based on the well known solution of the time-independent radiative transfer equation along a ray and on suitable point transformations, general quadrature solutions of the monochromatic transfer equation for plane-parallel, spherically-symmetric and arbitrarily shaped 3D configurations with differential motion are derived for the observer's and the comoving frame. The source function is assumed to be given; however, the scattering case requires only a simple iteration in addition. Since complete Lorentz transformations are used, the velocities are not restricted. It is shown that in many cases the explicit form of the transfer equation - which often is quite complicated - is not required for the determination of the specific intensities.
Baschek Bodo
Efimov G. V.
von Waldenfels W.
Wehrse Rainer
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