Published September 1990
| Version v1
Journal article
A model for the optical properties of porous grains
Description
A numerical method, based on an integral representation of Maxwell's equations, is used to calculate scattering properties of model porous aggregates of small particles. It is shown that increasing porosity can lead to enhanced absorption and emission of radiation and a lower albedo. One application is to show how strongly the 9.7-micron emission feature of a piece of astronomical silicate matter depends on its porosity. The integral method is compared with the well-known coupled dipole approach for the case of a solid sphere. The validity of the Maxwell-Garnett effective medium theory is shown for certain cases where the individual particles in the aggregate satisfy the Rayleigh size conditions. 27 refs
Additional details
Publishing Information
- Journal Title
- Astrophysical Journal
- Journal Volume
- 361
- Series
- Astrophys. J.
- Journal Page Range
- 251-259
- ISSN
- 0004-637X
- CODEN
- ASJOA
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 22014381
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ABSORPTION SPECTRA; ALBEDO; COMETS; INFRARED SPECTRA; INTERSTELLAR GRAINS; INTERSTELLAR SPACE; MAXWELL EQUATIONS; NUMERICAL SOLUTION; OPTICAL PROPERTIES; POROSITY; RADIATION TRANSPORT; SCATTERING; SILICATES
- Descriptors DEC
- DIFFERENTIAL EQUATIONS; EQUATIONS; OXYGEN COMPOUNDS; PARTIAL DIFFERENTIAL EQUATIONS; PARTICLES; PHYSICAL PROPERTIES; SILICON COMPOUNDS; SPACE; SPECTRA