工程流体力学

solutions to-Fluid-Mechanics-Solutions-Frank-M-White.pdf

王洪伟老师版本的流体力学，很有趣的一本书，没有纯粹的大篇幅公式介绍，更多的结合生活中一些日常现象来阐述流体力学。

计算流体力学基础 与CFD软件应用

This book gives an excellent introduction to fluid dynamics First published in 1967, Professor Batchelor's classic work is still one of the foremost texts on fluid dynamics. His careful presentation of the underlying theories of fluids is still timely and applicable, even in these days of almost limitless computer power. This reissue ensures that a new generation of graduate students experiences the elegance of Professor Batchelor's writing. ... many interesting and important photographs of fluid flows are included in order to help the students who do not have an opportunity of observing flow phenomena in a laboratory. The book also contains exercises at the end of each chapter. In comparison with many currently available books, I find this book by Batchelor especially stimulating and useful for students of applied mathematics and engineering.' L. Debnath, Zentralblatt MATH

吴子牛 计算流体力学基本原理-已打标签 涉及计算流体力学较为规范的内容，包括流体力学的基本原理、流体力学基本方程的计算形式与配套模型、方程的基本理论、构造计算方法的基本原则、计算方法的分析理论和一些实用化计算技术． 本书可供从事计算流体力学的科研、技术人员参考，也可以作为流体力学专业和应用数学专业研究生和本科生的教学参考书．

教材 I DO LIKE CFD，相关计算流体力学领域的教材。

matlab如何敲代码喜怒无常的API Moody API：动态系泊库，用于在OpenFOAM和其他流体力学代码中进行站台保持耦合模拟。 版本2.0 -更新2.0.1-为了简化代码管理，文件结构进行了一些更改。 这样可以在存储库上进行git更新，并简化对开源代码API的更新和更改。 因此，“发行”选项卡将不会在以后的更新和发行版中使用。 重命名为thirdParty-> API，其中包含matlab，fortran和OpenFOAM源。 OpenFOAM API中用于多处理器仿真的错误修正。 post / matlab文件夹已删除。 现在，matlab脚本以及matlab API和shell界面都包含在API / matlab中。 moody-arch.tar.gz包含以下文件夹：etc /，bin /，lib /和include /。 将您的OS版本解压缩到位，所有内容都应像以前一样工作。 为了运行Windows教程，我需要将lib / *中的库复制到bin /中。 肯定有一个更清洁的解决方案...-结束更新- 以下列出了Moody中的更新重点： 莫里森型浸没式刚体。 （点和缸） 新

SPH光滑粒子流体动力学 模拟代码

pdf原版,非扫描. The material in this book is based on lecture notes of a course on astrophysical fluid dynamics which has been given for several years to third-year students at the University of Cambridge. There are several excellent books which cover fluid dynamics from a terrestrial standpoint, but very few provide a full introduction to the concepts and methods used to deal with the highly compressible flows which arise in astrophysical contexts. Our aim with this book is to provide just such an introduction, and we hope that it will also serve as a reference volume for advanced undergraduate and graduate students. Several people have provided input at various stages of the preparation of this book. In particular we thank Jim Pringle, Donald Lynden- Bell and Giuseppe Lodato for their help. We are also grateful to the students who have taken the course at Cambridge for correcting typographical errors in the lecture notes, drawing our attention to parts where the description was less clear than it should have been, and helping us to develop the exercises.