M. Gros et al., AN IMPLICIT INTEGRAL METHOD TO SOLVE SELECTED RADIATIVE-TRANSFER PROBLEMS .4. THE CASE OF SPHERICAL GEOMETRY, The Astrophysical journal, 489(1), 1997, pp. 331-345
In the previous papers of this series, we introduced the implicit inte
gral method (IIM) to solve those radiative transfer (RT) problems in w
hich the source function depends on an integral of the specific intens
ity of the radiation field over directions and frequencies. The IIM re
sts upon a forward-elimination, back-substitution scheme naturally bas
ed on the physics of the RT process, and does not require any matricia
l algorithm. Customary methods to solve RT problems, in which the sour
ce function depends on the aforesaid integral, rest upon matrix algori
thms. In spherical geometry, due to the strong anisotropy of the radia
tion field brought about by the limb curvature, the so-called peaking
effect, the number of directions necessary to describe this anisotropy
is exceedingly high, and consequently the relevant matrices are hard
to handle. The present paper deals with the application of the IIM to
RT problems in spherical geometry, where the distinctive nonmatricial
character of the method can be fully exploited, given the intrinsic hi
gh dimensionality of the problem.