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Dynamo action and the nearly axisymmetric magnetic field of Saturn
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Zeitschriftentitel: | Geophysical Research Letters |
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Personen und Körperschaften: | |
In: | Geophysical Research Letters, 27, 2000, 18, S. 2889-2892 |
Format: | E-Article |
Sprache: | Englisch |
veröffentlicht: |
American Geophysical Union (AGU)
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Schlagwörter: |
author_facet |
Love, J. J. Love, J. J. |
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author |
Love, J. J. |
spellingShingle |
Love, J. J. Geophysical Research Letters Dynamo action and the nearly axisymmetric magnetic field of Saturn General Earth and Planetary Sciences Geophysics |
author_sort |
love, j. j. |
spelling |
Love, J. J. 0094-8276 1944-8007 American Geophysical Union (AGU) General Earth and Planetary Sciences Geophysics http://dx.doi.org/10.1029/1999gl008466 <jats:p>We examine kinematic dynamo action in an electrically conducting spherical body of fluid with an overlying shell of differential rotation. It is thought that such flow types could explain the nearly axisymmetric magnetic field of Saturn. Although we find that an outer layer of differential rotation can ‘axisymmetrize’ the exterior magnetic field, surprisingly, sometimes it does not, giving magnetic fields that have no axisymmetric ingredients.</jats:p> Dynamo action and the nearly axisymmetric magnetic field of Saturn Geophysical Research Letters |
doi_str_mv |
10.1029/1999gl008466 |
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Physik Geologie und Paläontologie Geographie |
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American Geophysical Union (AGU), 2000 |
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American Geophysical Union (AGU), 2000 |
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0094-8276 1944-8007 |
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2000 |
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American Geophysical Union (AGU) |
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Geophysical Research Letters |
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49 |
title |
Dynamo action and the nearly axisymmetric magnetic field of Saturn |
title_unstemmed |
Dynamo action and the nearly axisymmetric magnetic field of Saturn |
title_full |
Dynamo action and the nearly axisymmetric magnetic field of Saturn |
title_fullStr |
Dynamo action and the nearly axisymmetric magnetic field of Saturn |
title_full_unstemmed |
Dynamo action and the nearly axisymmetric magnetic field of Saturn |
title_short |
Dynamo action and the nearly axisymmetric magnetic field of Saturn |
title_sort |
dynamo action and the nearly axisymmetric magnetic field of saturn |
topic |
General Earth and Planetary Sciences Geophysics |
url |
http://dx.doi.org/10.1029/1999gl008466 |
publishDate |
2000 |
physical |
2889-2892 |
description |
<jats:p>We examine kinematic dynamo action in an electrically conducting spherical body of fluid with an overlying shell of differential rotation. It is thought that such flow types could explain the nearly axisymmetric magnetic field of Saturn. Although we find that an outer layer of differential rotation can ‘axisymmetrize’ the exterior magnetic field, surprisingly, sometimes it does not, giving magnetic fields that have no axisymmetric ingredients.</jats:p> |
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author | Love, J. J. |
author_facet | Love, J. J., Love, J. J. |
author_sort | love, j. j. |
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container_title | Geophysical Research Letters |
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description | <jats:p>We examine kinematic dynamo action in an electrically conducting spherical body of fluid with an overlying shell of differential rotation. It is thought that such flow types could explain the nearly axisymmetric magnetic field of Saturn. Although we find that an outer layer of differential rotation can ‘axisymmetrize’ the exterior magnetic field, surprisingly, sometimes it does not, giving magnetic fields that have no axisymmetric ingredients.</jats:p> |
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physical | 2889-2892 |
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publisher | American Geophysical Union (AGU) |
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series | Geophysical Research Letters |
source_id | 49 |
spelling | Love, J. J. 0094-8276 1944-8007 American Geophysical Union (AGU) General Earth and Planetary Sciences Geophysics http://dx.doi.org/10.1029/1999gl008466 <jats:p>We examine kinematic dynamo action in an electrically conducting spherical body of fluid with an overlying shell of differential rotation. It is thought that such flow types could explain the nearly axisymmetric magnetic field of Saturn. Although we find that an outer layer of differential rotation can ‘axisymmetrize’ the exterior magnetic field, surprisingly, sometimes it does not, giving magnetic fields that have no axisymmetric ingredients.</jats:p> Dynamo action and the nearly axisymmetric magnetic field of Saturn Geophysical Research Letters |
spellingShingle | Love, J. J., Geophysical Research Letters, Dynamo action and the nearly axisymmetric magnetic field of Saturn, General Earth and Planetary Sciences, Geophysics |
title | Dynamo action and the nearly axisymmetric magnetic field of Saturn |
title_full | Dynamo action and the nearly axisymmetric magnetic field of Saturn |
title_fullStr | Dynamo action and the nearly axisymmetric magnetic field of Saturn |
title_full_unstemmed | Dynamo action and the nearly axisymmetric magnetic field of Saturn |
title_short | Dynamo action and the nearly axisymmetric magnetic field of Saturn |
title_sort | dynamo action and the nearly axisymmetric magnetic field of saturn |
title_unstemmed | Dynamo action and the nearly axisymmetric magnetic field of Saturn |
topic | General Earth and Planetary Sciences, Geophysics |
url | http://dx.doi.org/10.1029/1999gl008466 |