Nonstationary radiative transfer in stellar atmospheres

Details Nonstationary radiative transfer in stellar atmospheres Nonstationary radiative transfer in stellar atmospheres

Apr 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990azh....67..357k&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 67, Mar.-Apr. 1990, p. 357-366. In Russian.

Mathematics

Probability

2

Atmospheric Scattering, Light Scattering, Radiative Transfer, Stellar Atmospheres, Light Curve, Luminous Intensity, Optical Thickness, Time Dependence

Scientific paper

Time-dependent radiative transfer in a one-dimensional homogeneous atmosphere is investigated. It is assumed that photons are mainly in an absorbed state or between successive scatterings. The probability that a photon, originating at a given optical depth, will escape from the atmosphere after multiple scattering over a given period of time is determined for these two cases. The results obtained are used to interpret the brightness variability of flare stars.

Affiliated with

Also associated with

No associations

Rating

Nonstationary radiative transfer in stellar atmospheres 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 Nonstationary radiative transfer in stellar atmospheres, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Nonstationary radiative transfer in stellar atmospheres will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1380406