國立高雄大學圖資館 |

語系: 繁體中文

說明(常見問題)

圖資館首頁

登入

回首頁

切換: 標籤 | MARC模式 | ISBD

Magnetoconvection

Proctor, M. R. E.

Magnetoconvection

紀錄類型:	書目-電子資源 : Monograph/item
正題名/作者:	MagnetoconvectionN. O. Weiss, M. R. E. Proctor.
作者:	Weiss, N. O.
其他作者:	Proctor, M. R. E.
出版者:	Cambridge :Cambridge University Press,2014.
面頁冊數:	xi, 397 p. :ill., digital ;24 cm.
標題:	Magnetic fields.
電子資源:	https://doi.org/10.1017/CBO9780511667459
ISBN:	9780511667459$q(electronic bk.)

Magnetoconvection
Weiss, N. O.

Magnetoconvection[electronic resource] /N. O. Weiss, M. R. E. Proctor. - Cambridge :Cambridge University Press,2014. - xi, 397 p. :ill., digital ;24 cm. - Cambridge monographs on mechanics. - Cambridge monographs on mechanics..

Preface -- 1. Introduction -- 2. Basic MHD -- 3. Linearized Boussinesq magnetoconvection -- 4. The nonlinear regime -- 5. 2D Boussinesq magnetoconvection -- 6. 3D Boussinesq magnetoconvection -- 7. Magnetoconvection, rotation and the dynamo -- 8. Compressible magnetoconvection -- 9. Solar and stellar magnetic fields -- Appendix A. The Boussinesq and anelastic approximations -- Appendix B. Chaotic systems -- Appendix C. Double-diffusive convection -- Appendix D. Magnetic buoyancy and the magneto-Boussinesq approximation -- References -- Index.

The last thirty years have seen great leaps forward in the subject of magnetoconvection. Computational techniques can now explain exotic nonlinear behaviour, transition to chaos and the formation of structures that can be observed on the surface of the Sun. Here, two leading experts present the current state of knowledge of the subject. They provide a mathematical and numerical treatment of the interactions between electrically conducting fluids and magnetic fields that lead to the complex structures and rich behaviour observed on the Sun and other stars, as well as in the interiors of planets like the Earth. The authors' combined analytical and computational approach provides a model for the study of a wide range of related problems. The discussion includes bifurcation theory, chaotic behaviour, pattern formation in two and three dimensions, and applications to geomagnetism and to the properties of sunspots and other features at the solar surface.

ISBN: 9780511667459$q(electronic bk.)Subjects--Topical Terms:

203345
Magnetic fields.

LC Class. No.: QC754.2.M3 / W45 2014

Dewey Class. No.: 538.7

Magnetoconvection
LDR:02296nmm a2200265 a 4500 001 560403
003 UkCbUP
005 20151005020621.0
006 m d
007 cr nn 008maaau
008 200113s2014 enk o 1 0 eng d
020 $a 9780511667459$q(electronic bk.)
020 $a 9780521190558$q(paper)
035 $a CR9780511667459
040 $a UkCbUP $b eng $c UkCbUP $d GP
041 0 $a eng
050 4 $a QC754.2.M3 $b W45 2014
082 0 4 $a 538.7 $2 23
090 $a QC754.2.M3 $b W429 2014
100 1 $a Weiss, N. O. $q (Nigel Oscar). $3 844342
245 1 0 $a Magnetoconvection $h [electronic resource] / $c N. O. Weiss, M. R. E. Proctor.
260 $a Cambridge : $b Cambridge University Press, $c 2014.
300 $a xi, 397 p. : $b ill., digital ; $c 24 cm.
490 1 $a Cambridge monographs on mechanics
505 0 $a Preface -- 1. Introduction -- 2. Basic MHD -- 3. Linearized Boussinesq magnetoconvection -- 4. The nonlinear regime -- 5. 2D Boussinesq magnetoconvection -- 6. 3D Boussinesq magnetoconvection -- 7. Magnetoconvection, rotation and the dynamo -- 8. Compressible magnetoconvection -- 9. Solar and stellar magnetic fields -- Appendix A. The Boussinesq and anelastic approximations -- Appendix B. Chaotic systems -- Appendix C. Double-diffusive convection -- Appendix D. Magnetic buoyancy and the magneto-Boussinesq approximation -- References -- Index.
520 $a The last thirty years have seen great leaps forward in the subject of magnetoconvection. Computational techniques can now explain exotic nonlinear behaviour, transition to chaos and the formation of structures that can be observed on the surface of the Sun. Here, two leading experts present the current state of knowledge of the subject. They provide a mathematical and numerical treatment of the interactions between electrically conducting fluids and magnetic fields that lead to the complex structures and rich behaviour observed on the Sun and other stars, as well as in the interiors of planets like the Earth. The authors' combined analytical and computational approach provides a model for the study of a wide range of related problems. The discussion includes bifurcation theory, chaotic behaviour, pattern formation in two and three dimensions, and applications to geomagnetism and to the properties of sunspots and other features at the solar surface.
650 0 $a Magnetic fields. $3 203345
650 0 $a Solar magnetic fields. $3 678231
650 0 $a Geomagnetism. $3 515781
650 0 $a Magnetohydrodynamics. $3 207822
650 0 $a Relativistic fluid dynamics. $3 278254
700 1 $a Proctor, M. R. E. $3 844343
830 0 $a Cambridge monographs on mechanics. $3 844344
856 4 0 $u https://doi.org/10.1017/CBO9780511667459