| 書(shū)目名稱(chēng) | Computational Methods for Astrophysical Fluid Flow |
| 副標(biāo)題 | Saas-Fee Advanced Co |
| 編輯 | R. J. LeVeque,D. Mihalas,E. Müller,O. Steiner,A. G |
| 視頻video | http://file.papertrans.cn/233/232706/232706.mp4 |
| 概述 | This book can be used also as a textbook for scientific modelling in fluid mechanics and astrophysics |
| 叢書(shū)名稱(chēng) | Saas-Fee Advanced Course |
| 圖書(shū)封面 |  |
| 描述 | This book leads directly to the most modern numerical techniques for compressible fluid flow, with special consideration given to astrophysical applications. Emphasis is put on high-resolution shock-capturing finite-volume schemes based on Riemann solvers. The applications of such schemes, in particular the PPM method, are given and include large-scale simulations of supernova explosions by core collapse and thermonuclear burning and astrophysical jets. Parts two and three treat radiation hydrodynamics. The power of adaptive (moving) grids is demonstrated with a number of stellar-physical simulations showing very crispy shock-front structures. |
| 出版日期 | Book 1998 |
| 關(guān)鍵詞 | astronomy; astrophysics; conservation law; dynamics; flow; solution; Supernova |
| 版次 | 1 |
| doi | https://doi.org/10.1007/3-540-31632-9 |
| isbn_softcover | 978-3-642-08412-6 |
| isbn_ebook | 978-3-540-31632-9Series ISSN 1861-7980 Series E-ISSN 1861-8227 |
| issn_series | 1861-7980 |
| copyright | Springer-Verlag Berlin Heidelberg 1998 |
|Archiver|手機(jī)版|小黑屋|
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