Invariant Imbedding and Chandrasekhar's Planetary Problem of Radiative Transfer

Details Invariant Imbedding and Chandrasekhar's Planetary Problem of Radiative Transfer Invariant Imbedding and Chandrasekhar's Planetary Problem of Radiative Transfer

May 1972

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1972ap%26ss..16..241b&link_type=abstract

Astrophysics and Space Science, Volume 16, Issue 2, pp.241-248

Astronomy and Astrophysics

Astrophysics

4

Scientific paper

In connection with Chandrasekhar's planetary problem of radiative transfer the total scattering and the diffuse transmission functions have been discussed by several authors (cf. Chandrasekhar, 1950; van de Hulst, 1948; Sobolev, 1948; Bellman,et al., 1967; Kagiwada and Kalaba, 1971). With the aid of the Bellman-Krein formula for the resolvent kernel of the auxiliary equation governing the source function, we show how the invariant imbedding equations governing the diffuse scattering and transmission functions can readily be obtained. So far as we know, the Cauchy system of the functional equations for the scattering and transmission functions is new and is well-suited for the numerical computation.

Affiliated with

Also associated with

No associations

Rating

Invariant Imbedding and Chandrasekhar's Planetary Problem of Radiative Transfer does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Invariant Imbedding and Chandrasekhar's Planetary Problem of Radiative Transfer, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Invariant Imbedding and Chandrasekhar's Planetary Problem of Radiative Transfer will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1432936