東華大學圖書館 |

語系: 繁體中文

說明(常見問題)

回圖書館首頁

手機版館藏查詢

登入

回首頁

切換: 標籤 | MARC模式 | ISBD

Modern fluid dynamics for physics an...

Regev, Oded.

FindBook

Google Book

Amazon

博客來

Modern fluid dynamics for physics and astrophysics

紀錄類型:	書目-電子資源 : Monograph/item
正題名/作者:	Modern fluid dynamics for physics and astrophysics/ by Oded Regev, Orkan M. Umurhan, Philip A. Yecko.
作者:	Regev, Oded.
其他作者:	Umurhan, Orkan M.
出版者:	New York, NY :Springer New York : : 2016.,
面頁冊數:	xxiii, 680 p. :ill. (some col.), digital ;24 cm.
內容註:	Fundamentals -- Special flows and their properties -- Rotating flows -- Shallow water theory and incompressible waves -- Effects of compressibility sound and shock waves -- Stability and transition -- Rudiments of turbulence -- Equations of magnetohydrodynamics -- Magnetohydrodynamical Phenomena -- Numerical methods and caveats.
Contained By:	Springer eBooks
標題:	Fluid dynamics. -
電子資源:	http://dx.doi.org/10.1007/978-1-4939-3164-4
ISBN:	9781493931644

Modern fluid dynamics for physics and astrophysics
Regev, Oded.

Modern fluid dynamics for physics and astrophysics[electronic resource] /by Oded Regev, Orkan M. Umurhan, Philip A. Yecko. - New York, NY :Springer New York :2016. - xxiii, 680 p. :ill. (some col.), digital ;24 cm. - Graduate texts in physics,1868-4513. - Graduate texts in physics..

Fundamentals -- Special flows and their properties -- Rotating flows -- Shallow water theory and incompressible waves -- Effects of compressibility sound and shock waves -- Stability and transition -- Rudiments of turbulence -- Equations of magnetohydrodynamics -- Magnetohydrodynamical Phenomena -- Numerical methods and caveats.

This book grew out of the need to provide students with a solid introduction to modern fluid dynamics. It offers a broad grounding in the underlying principles and techniques used, with some emphasis on applications in astrophysics and planetary science. The book comprehensively covers recent developments, methods and techniques, including, for example, new ideas on transitions to turbulence (via transiently growing stable linear modes), new approaches to turbulence (which remains the enigma of fluid dynamics), and the use of asymptotic approximation methods, which can give analytical or semi-analytical results and complement fully numerical treatments. The authors also briefly discuss some important considerations to be taken into account when developing a numerical code for computer simulation of fluid flows. Although the text is populated throughout with examples and problems from the field of astrophysics and planetary science, the text is eminently suitable as a general introduction to fluid dynamics. It is assumed that the readers are mathematically equipped with a reasonable knowledge in analysis, including basics of ordinary and partial differential equations and a good command of vector calculus and linear algebra. Each chapter concludes with bibliographical notes in which the authors briefly discuss the chapter's essential literature and give recommendations for further, deeper reading. Included in each chapter are a number of problems, some of them relevant to astrophysics and planetary science. The book is written for advanced undergraduate and graduate students, but will also prove a valuable source of reference for established researchers.

ISBN: 9781493931644

Standard No.: 10.1007/978-1-4939-3164-4doiSubjects--Topical Terms:

545210
Fluid dynamics.

LC Class. No.: TA357

Dewey Class. No.: 620.1064

Modern fluid dynamics for physics and astrophysics
LDR:03077nmm a2200337 a 4500 001 2038364
003 DE-He213
005 20161103114723.0
006 m d
007 cr nn 008maaau
008 161209s2016 nyu s 0 eng d
020 $a 9781493931644 $q (electronic bk.)
020 $a 9781493931637 $q (paper)
024 7 $a 10.1007/978-1-4939-3164-4 $2 doi
035 $a 978-1-4939-3164-4
040 $a GP $c GP
041 0 $a eng
050 4 $a TA357
072 7 $a PGC $2 bicssc
072 7 $a SCI004000 $2 bisacsh
072 7 $a SCI005000 $2 bisacsh
082 0 4 $a 620.1064 $2 23
090 $a TA357 $b .R333 2016
100 1 $a Regev, Oded. $3 2195510
245 1 0 $a Modern fluid dynamics for physics and astrophysics $h [electronic resource] / $c by Oded Regev, Orkan M. Umurhan, Philip A. Yecko.
260 $a New York, NY : $b Springer New York : $b Imprint: Springer, $c 2016.
300 $a xxiii, 680 p. : $b ill. (some col.), digital ; $c 24 cm.
490 1 $a Graduate texts in physics, $x 1868-4513
505 0 $a Fundamentals -- Special flows and their properties -- Rotating flows -- Shallow water theory and incompressible waves -- Effects of compressibility sound and shock waves -- Stability and transition -- Rudiments of turbulence -- Equations of magnetohydrodynamics -- Magnetohydrodynamical Phenomena -- Numerical methods and caveats.
520 $a This book grew out of the need to provide students with a solid introduction to modern fluid dynamics. It offers a broad grounding in the underlying principles and techniques used, with some emphasis on applications in astrophysics and planetary science. The book comprehensively covers recent developments, methods and techniques, including, for example, new ideas on transitions to turbulence (via transiently growing stable linear modes), new approaches to turbulence (which remains the enigma of fluid dynamics), and the use of asymptotic approximation methods, which can give analytical or semi-analytical results and complement fully numerical treatments. The authors also briefly discuss some important considerations to be taken into account when developing a numerical code for computer simulation of fluid flows. Although the text is populated throughout with examples and problems from the field of astrophysics and planetary science, the text is eminently suitable as a general introduction to fluid dynamics. It is assumed that the readers are mathematically equipped with a reasonable knowledge in analysis, including basics of ordinary and partial differential equations and a good command of vector calculus and linear algebra. Each chapter concludes with bibliographical notes in which the authors briefly discuss the chapter's essential literature and give recommendations for further, deeper reading. Included in each chapter are a number of problems, some of them relevant to astrophysics and planetary science. The book is written for advanced undergraduate and graduate students, but will also prove a valuable source of reference for established researchers.
650 0 $a Fluid dynamics. $3 545210
650 1 4 $a Physics. $3 516296
650 2 4 $a Astronomy, Astrophysics and Cosmology. $3 890823
650 2 4 $a Mechanics. $3 525881
650 2 4 $a Theoretical, Mathematical and Computational Physics. $3 1066859
700 1 $a Umurhan, Orkan M. $3 2195511
700 1 $a Yecko, Philip A. $3 2195512
710 2 $a SpringerLink (Online service) $3 836513
773 0 $t Springer eBooks
830 0 $a Graduate texts in physics. $x 1868-4513. $3 1314540
856 4 0 $u http://dx.doi.org/10.1007/978-1-4939-3164-4
950 $a Physics and Astronomy (Springer-11651)