| タイトル | Turbulent transport in the solar nebula |
| 本文（外部サイト） | http://hdl.handle.net/2060/19890013458 |
| 著者（英） | Thompson, Kevin W. |
| 著者所属（英） | Stanford Univ. |
| 発行日 | 1989-02-01 |
| 言語 | eng |
| 内容記述 | It is likely that turbulence played a major role in the evolution of the solar nebula, which is the flattened disk of dust and gas out of which our solar system formed. Relevant turbulent processes include the transport of angular momentum, mass, and heat, which were critically important to the formation of the solar system. This research will break ground in the modeling of compressible turbulence and its effects on the evolution of the solar nebula. The computational techniques which were developed should be of interest to researchers studying other astrophysical disk systems (e.g., active galactic nuclei), as well as turbulence modelers outside the astrophysics community. |
| NASA分類 | FLUID MECHANICS AND HEAT TRANSFER |
| レポートNO | 89N22829 |
| 権利 | No Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/142197 |
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