Radiative Transfer in Circumstellar Dust.
Radiative Transfer in Circumstellar Dust.
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In his second paper Huang (19 69b) argues that the as- sumption that the particles scatter radiation as grey-bodies is valid. He states that in the case of interstellar red- dening blue light is preferentially scattered out of the line of sight, whereas in the case of a circumstellar dust cloud we observe scattered radiation coming in all direc- tions; such that, the amount of radiation of a certain wave- length which is lost in direct transmission along the line of sight is regained due to the... overall scattering process.
For his intermediate case Huang (19 69b) assumes that the radiation field can be broken into two parts - a visual part and an infrared part. He then proceeds to solve the overall transfer problem as though it were two less diffi- cult problems: (1) a nonconservative scattering problem in- volving only the stellar radiation in the visual (the infrared emission of the star is assumed to be negligible) and (2) the problem of an atmosphere in local thermo- dynamical equilibrium for the infrared radiation emitted by the dust, with an energy source, namely, the visual radia- tion absorbed in the nonconservative optical region.
What to read after Radiative Transfer in Circumstellar Dust.?
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To quickly assess the difficulty of the text, read a short excerpt:
In his second paper Huang (19 69b) argues that the as- sumption that the particles scatter radiation as grey-bodies is valid. He states that in the case of interstellar red- dening blue light is preferentially scattered out of the line of sight, whereas in the case of a circumstellar dust cloud we observe scattered radiation coming in all direc- tions; such that, the amount of radiation of a certain wave- length which is lost in direct transmission along the line of sight is regained due to the... overall scattering process.
For his intermediate case Huang (19 69b) assumes that the radiation field can be broken into two parts - a visual part and an infrared part. He then proceeds to solve the overall transfer problem as though it were two less diffi- cult problems: (1) a nonconservative scattering problem in- volving only the stellar radiation in the visual (the infrared emission of the star is assumed to be negligible) and (2) the problem of an atmosphere in local thermo- dynamical equilibrium for the infrared radiation emitted by the dust, with an energy source, namely, the visual radia- tion absorbed in the nonconservative optical region.
What to read after Radiative Transfer in Circumstellar Dust.?
You can find similar books in the "Read Also" column, or choose other free books by Harvel, Christopher Alvin, 1944- to read onlineMoreLess
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