Magnetoconvection:
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 curr...
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| Main Author: | |
|---|---|
| Format: | Electronic eBook |
| Language: | English |
| Published: |
Cambridge
Cambridge University Press
2014
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| Series: | Cambridge monographs on mechanics
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| Subjects: | |
| Online Access: | BSB01 FHN01 Volltext |
| Summary: | 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 |
| Item Description: | Title from publisher's bibliographic system (viewed on 05 Oct 2015) |
| Physical Description: | 1 online resource (xi, 397 pages) |
| ISBN: | 9780511667459 |
| DOI: | 10.1017/CBO9780511667459 |
Staff View
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| 505 | 8 | |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 | 4 | |a Magnetic fields | |
| 650 | 4 | |a Solar magnetic fields | |
| 650 | 4 | |a Geomagnetism | |
| 650 | 4 | |a Magnetohydrodynamics | |
| 650 | 4 | |a Relativistic fluid dynamics | |
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Record in the Search Index
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| author | Weiss, N. O. |
| author_facet | Weiss, N. O. |
| author_role | aut |
| author_sort | Weiss, N. O. |
| author_variant | n o w no now |
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| contents | 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 |
| ctrlnum | (ZDB-20-CBO)CR9780511667459 (OCoLC)897489034 (DE-599)BVBBV043941684 |
| dewey-full | 538/.7 |
| dewey-hundreds | 500 - Natural sciences and mathematics |
| dewey-ones | 538 - Magnetism |
| dewey-raw | 538/.7 |
| dewey-search | 538/.7 |
| dewey-sort | 3538 17 |
| dewey-tens | 530 - Physics |
| discipline | Physik |
| doi_str_mv | 10.1017/CBO9780511667459 |
| format | Electronic eBook |
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| id | DE-604.BV043941684 |
| illustrated | Not Illustrated |
| indexdate | 2024-07-10T07:39:16Z |
| institution | BVB |
| isbn | 9780511667459 |
| language | English |
| oai_aleph_id | oai:aleph.bib-bvb.de:BVB01-029350654 |
| oclc_num | 897489034 |
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| owner | DE-12 DE-92 |
| owner_facet | DE-12 DE-92 |
| physical | 1 online resource (xi, 397 pages) |
| psigel | ZDB-20-CBO ZDB-20-CBO BSB_PDA_CBO ZDB-20-CBO FHN_PDA_CBO |
| publishDate | 2014 |
| publishDateSearch | 2014 |
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| publisher | Cambridge University Press |
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| series2 | Cambridge monographs on mechanics |
| spelling | Weiss, N. O. Verfasser aut Magnetoconvection N.O. Weiss, University of Cambridge, M.R.E. Proctor, University of Cambridge Cambridge Cambridge University Press 2014 1 online resource (xi, 397 pages) txt rdacontent c rdamedia cr rdacarrier Cambridge monographs on mechanics Title from publisher's bibliographic system (viewed on 05 Oct 2015) 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 Magnetic fields Solar magnetic fields Geomagnetism Magnetohydrodynamics Relativistic fluid dynamics Proctor, M. R. E. Sonstige oth Erscheint auch als Druckausgabe 978-0-521-19055-8 https://doi.org/10.1017/CBO9780511667459 Verlag URL des Erstveröffentlichers Volltext |
| spellingShingle | Weiss, N. O. Magnetoconvection 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 Magnetic fields Solar magnetic fields Geomagnetism Magnetohydrodynamics Relativistic fluid dynamics |
| title | Magnetoconvection |
| title_auth | Magnetoconvection |
| title_exact_search | Magnetoconvection |
| title_full | Magnetoconvection N.O. Weiss, University of Cambridge, M.R.E. Proctor, University of Cambridge |
| title_fullStr | Magnetoconvection N.O. Weiss, University of Cambridge, M.R.E. Proctor, University of Cambridge |
| title_full_unstemmed | Magnetoconvection N.O. Weiss, University of Cambridge, M.R.E. Proctor, University of Cambridge |
| title_short | Magnetoconvection |
| title_sort | magnetoconvection |
| topic | Magnetic fields Solar magnetic fields Geomagnetism Magnetohydrodynamics Relativistic fluid dynamics |
| topic_facet | Magnetic fields Solar magnetic fields Geomagnetism Magnetohydrodynamics Relativistic fluid dynamics |
| url | https://doi.org/10.1017/CBO9780511667459 |
| work_keys_str_mv | AT weissno magnetoconvection AT proctormre magnetoconvection |