Polarization Efficiency and Phase Function Calculated on the Basis of the Mie Theory
スポンサーリンク
概要
- 論文の詳細を見る
The polarization efficiencies for scattering and the efficiency factors for the differential cross-sections are calculated for several interstellar grain models on the basis of the Mie theory. The results for ice, silicate, and graphite grains are presented in the tabular form, which will be convenient for explaining the observations of polarization in reflection nebulae and in the outer part of galaxies, and so on.Interstellar grainsInterstellar scatteringPolarizationRayleigh approximation
- 東北大学の論文
- 1985-06-26
著者
-
Seki M
Tohoku Univ.
-
Seki Munezo
College Of General Education Tohoku University
-
Matsumura Masafumi
Astronomical Institute Faculty Of Science Tohoku University
関連論文
- Spectroscopic Observations of Several Stars Toward the Bok Globule B361
- Polarization Efficiency and Phase Function Calculated on the Basis of the Mie Theory
- Paramagnetic Grain Alignment Associated with Internal Friction and the Polarization Efficiency