Statistics – Computation
Scientific paper
Mar 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.165..119b&link_type=abstract
Astrophysics and Space Science (ISSN 0004-640X), vol. 165, no. 1, March 1990, p. 119-129.
Statistics
Computation
5
Atmospheric Scattering, Computational Astrophysics, Invariance, Novae, Stellar Atmospheres, Integral Equations, Isotropic Media, Laplace Transformation, Stellar Evolution, Time Dependence
Scientific paper
Karanjai and Biswas (1988) derived the time-dependent X- and Y-functions for a homogeneous, plane-parallel, nonemitting, and isotropic atmosphere of finite thickness, using the integral-equation method developed by Rybicki (1971); they then (1989) derived the time-dependent H-, X-, and Y-functions in a homogeneous atmosphere scattering anisotropically with Dirac delta-function type and Heavyside unit-step function type time-dependence incidence. The principle of invariance is presently employed to arrive at expressions for time-dependent X- and Y-functions.
Biswas G.
Karanjai Sitansubimal
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