TL;DR
This paper reviews the theoretical framework for understanding how cosmic dust interacts with electromagnetic radiation, including absorption, scattering, and reradiation processes, which are crucial for interpreting astronomical observations.
Contribution
It provides a comprehensive theoretical basis for analyzing the optical properties of cosmic dust, essential for astrophysical research.
Findings
Summarizes key optical processes of dust
Provides models for dust-light interactions
Highlights importance for astronomical observations
Abstract
Except in a few cases cosmic dust can be studied in situ or in terrestrial laboratories, essentially all of our information concerning the nature of cosmic dust depends upon its interaction with electromagnetic radiation. This chapter presents the theoretical basis for describing the optical properties of dust -- how it absorbs and scatters starlight and reradiates the absorbed energy at longer wavelengths.
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Taxonomy
TopicsAtmospheric aerosols and clouds