The radiative transfer through an astronomical region populated by stochastic clumps is studied by means of functional analytical techniques. Random density fluctuations of the background medium are described by a finite number of parameters. In the framework, each realization of the statistics corresponds to a possible configuration of a real clumpy region, as it is possible to infer from observations.
Radiative transfer in a stochastic universe. I - Observation-related statistics / C. Cecchi Pestellini; L. Barletti. - In: NEW ASTRONOMY. - ISSN 1384-1076. - STAMPA. - 6(3):(2001), pp. 151-163. [10.1016/S1384-1076(01)00046-X]
Radiative transfer in a stochastic universe. I - Observation-related statistics.
CECCHI PESTELLINI, CESARE;BARLETTI, LUIGI
2001
Abstract
The radiative transfer through an astronomical region populated by stochastic clumps is studied by means of functional analytical techniques. Random density fluctuations of the background medium are described by a finite number of parameters. In the framework, each realization of the statistics corresponds to a possible configuration of a real clumpy region, as it is possible to infer from observations.
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