Radiative Transfer in a Translucent Cloud Illuminated by an Extended Background Source
Abstract
We discuss the radiative transfer theory for translucent clouds illuminated by an extended background source. First, we derive a rigorous solution based on the assumption that multiple scatterings produce an isotropic flux. Then we derive a more manageable analytic approximation showing that it nicely matches the results of the rigorous approach. To validate our model, we compare our predictions with accurate laboratory measurements for various types of wellcharacterized grains, including purely dielectric and strongly absorbing materials representative of astronomical icy and metallic grains, respectively, finding excellent agreement without the need to add free parameters. We use our model to explore the behavior of an astrophysical cloud illuminated by a diffuse source with dust grains having parameters typical of the classic ISM grains of Draine and Lee and protoplanetary disks, with an application to the dark silhouette disk 114–426 in Orion Nebula. We find that the scattering term modifies the transmitted radiation, both in terms of intensity (extinction) and shape (reddening) of the spectral distribution. In particular, for small optical thickness, our results show that scattering makes reddening almost negligible at visible wavelengths. Once the optical thickness increases enough and the probability of scattering events becomes close to or larger thanmore »
 Authors:
 Università degli Studi dell’Insubria Dept. of Science and High Technology Via Valleggio, 11, I22100 Como (Italy)
 Universitá degli Studi di Milano Dept. of Physics Via Celoria 16, I20133 Milano (Italy)
 Space Telescope Science Institute Baltimore, MD 21218 (United States)
 Publication Date:
 OSTI Identifier:
 22663642
 Resource Type:
 Journal Article
 Resource Relation:
 Journal Name: Astrophysical Journal; Journal Volume: 840; Journal Issue: 1; Other Information: Country of input: International Atomic Energy Agency (IAEA)
 Country of Publication:
 United States
 Language:
 English
 Subject:
 79 ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; ABSORPTION; APPROXIMATIONS; ASTROPHYSICS; DIELECTRIC MATERIALS; DISTRIBUTION; DUSTS; FORECASTING; MULTIPLE SCATTERING; NEBULAE; PROTOPLANETS; RADIANT HEAT TRANSFER; REFRACTIVE INDEX; THICKNESS; WAVELENGTHS
Citation Formats
Biganzoli, Davide, Potenza, Marco A. C., and Robberto, Massimo, Email: robberto@stsci.edu. Radiative Transfer in a Translucent Cloud Illuminated by an Extended Background Source. United States: N. p., 2017.
Web. doi:10.3847/15384357/AA6BF9.
Biganzoli, Davide, Potenza, Marco A. C., & Robberto, Massimo, Email: robberto@stsci.edu. Radiative Transfer in a Translucent Cloud Illuminated by an Extended Background Source. United States. doi:10.3847/15384357/AA6BF9.
Biganzoli, Davide, Potenza, Marco A. C., and Robberto, Massimo, Email: robberto@stsci.edu. Mon .
"Radiative Transfer in a Translucent Cloud Illuminated by an Extended Background Source". United States.
doi:10.3847/15384357/AA6BF9.
@article{osti_22663642,
title = {Radiative Transfer in a Translucent Cloud Illuminated by an Extended Background Source},
author = {Biganzoli, Davide and Potenza, Marco A. C. and Robberto, Massimo, Email: robberto@stsci.edu},
abstractNote = {We discuss the radiative transfer theory for translucent clouds illuminated by an extended background source. First, we derive a rigorous solution based on the assumption that multiple scatterings produce an isotropic flux. Then we derive a more manageable analytic approximation showing that it nicely matches the results of the rigorous approach. To validate our model, we compare our predictions with accurate laboratory measurements for various types of wellcharacterized grains, including purely dielectric and strongly absorbing materials representative of astronomical icy and metallic grains, respectively, finding excellent agreement without the need to add free parameters. We use our model to explore the behavior of an astrophysical cloud illuminated by a diffuse source with dust grains having parameters typical of the classic ISM grains of Draine and Lee and protoplanetary disks, with an application to the dark silhouette disk 114–426 in Orion Nebula. We find that the scattering term modifies the transmitted radiation, both in terms of intensity (extinction) and shape (reddening) of the spectral distribution. In particular, for small optical thickness, our results show that scattering makes reddening almost negligible at visible wavelengths. Once the optical thickness increases enough and the probability of scattering events becomes close to or larger than 1, reddening becomes present but is appreciably modified with respect to the standard expression for lineofsight absorption. Moreover, variations of the grain refractive index, in particular the amount of absorption, also play an important role in changing the shape of the spectral transmission curve, with dielectric grains showing the minimum amount of reddening.},
doi = {10.3847/15384357/AA6BF9},
journal = {Astrophysical Journal},
number = 1,
volume = 840,
place = {United States},
year = {Mon May 01 00:00:00 EDT 2017},
month = {Mon May 01 00:00:00 EDT 2017}
}

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