プラズマ原子·分子過程の展望 4. 輸送コード 4.1 輻射輸送コード
1999 年 75 巻 10 号 p. 1145-1155
詳細
1999 年 75 巻 10 号 p. 1145-1155
A brief review is given of the physics of radiation transport, a topic that is important in the study of astrophysics, laser-plasmas, divertor-plasmas, etc. In general, we must solve non-local thermodynamic equilibrium processes using an appropriate atomic model. The resultant data related to the spectral emissivity and opacity of partially ionized plasmas are then used to solve the radiation transfer equation. In this note, I briefly overview a variety of ways to carry out such a calculation. In addition, similarities and differences in the physical process between laser-plasmas and divertor-plasmas are briefly described.
