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Field line resonances in discretized magnetospheric models: an artifact study
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Zeitschriftentitel: | Annales Geophysicae |
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Personen und Körperschaften: | , , , |
In: | Annales Geophysicae, 15, 1997, 6, S. 614-624 |
Format: | E-Article |
Sprache: | Englisch |
veröffentlicht: |
Copernicus GmbH
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Schlagwörter: |
author_facet |
Stellmacher, M. Glassmeier, K.-H. Lysak, R. L. Kivelson, M. G. Stellmacher, M. Glassmeier, K.-H. Lysak, R. L. Kivelson, M. G. |
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author |
Stellmacher, M. Glassmeier, K.-H. Lysak, R. L. Kivelson, M. G. |
spellingShingle |
Stellmacher, M. Glassmeier, K.-H. Lysak, R. L. Kivelson, M. G. Annales Geophysicae Field line resonances in discretized magnetospheric models: an artifact study Space and Planetary Science Earth and Planetary Sciences (miscellaneous) Atmospheric Science Geology Astronomy and Astrophysics |
author_sort |
stellmacher, m. |
spelling |
Stellmacher, M. Glassmeier, K.-H. Lysak, R. L. Kivelson, M. G. 1432-0576 Copernicus GmbH Space and Planetary Science Earth and Planetary Sciences (miscellaneous) Atmospheric Science Geology Astronomy and Astrophysics http://dx.doi.org/10.1007/s00585-997-0614-0 <jats:p>Abstract. For more than two decades numerical models of the Earth's magnetosphere have been used successfully to study magnetospheric dynamic features such as the excitation of ULF pulsations and the mechanism of field line resonance. However, numerical formulations simplify important properties of the real system. For instance the Alfvén continuum becomes discrete because of a finite grid size. This discretization can be a possible source of numerical artefacts. Therefore a careful interpretation of any observed features is required. Examples of such artefacts are presented using results from a three dimensional dipole model of the magnetosphere, including an inhomogeneous distribution of the Alfvén velocity. </jats:p> Field line resonances in discretized magnetospheric models: an artifact study Annales Geophysicae |
doi_str_mv |
10.1007/s00585-997-0614-0 |
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Physik Technik Geologie und Paläontologie Geographie |
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Copernicus GmbH, 1997 |
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Copernicus GmbH, 1997 |
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1997 |
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Copernicus GmbH |
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Annales Geophysicae |
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49 |
title |
Field line resonances in discretized magnetospheric models: an artifact study |
title_unstemmed |
Field line resonances in discretized magnetospheric models: an artifact study |
title_full |
Field line resonances in discretized magnetospheric models: an artifact study |
title_fullStr |
Field line resonances in discretized magnetospheric models: an artifact study |
title_full_unstemmed |
Field line resonances in discretized magnetospheric models: an artifact study |
title_short |
Field line resonances in discretized magnetospheric models: an artifact study |
title_sort |
field line resonances in discretized magnetospheric models: an artifact study |
topic |
Space and Planetary Science Earth and Planetary Sciences (miscellaneous) Atmospheric Science Geology Astronomy and Astrophysics |
url |
http://dx.doi.org/10.1007/s00585-997-0614-0 |
publishDate |
1997 |
physical |
614-624 |
description |
<jats:p>Abstract. For more than two decades numerical models of the Earth's magnetosphere have been used successfully to study magnetospheric dynamic features such as the excitation of ULF pulsations and the mechanism of field line resonance. However, numerical formulations simplify important properties of the real system. For instance the Alfvén continuum becomes discrete because of a finite grid size. This discretization can be a possible source of numerical artefacts. Therefore a careful interpretation of any observed features is required. Examples of such artefacts are presented using results from a three dimensional dipole model of the magnetosphere, including an inhomogeneous distribution of the Alfvén velocity.
</jats:p> |
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author | Stellmacher, M., Glassmeier, K.-H., Lysak, R. L., Kivelson, M. G. |
author_facet | Stellmacher, M., Glassmeier, K.-H., Lysak, R. L., Kivelson, M. G., Stellmacher, M., Glassmeier, K.-H., Lysak, R. L., Kivelson, M. G. |
author_sort | stellmacher, m. |
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container_start_page | 614 |
container_title | Annales Geophysicae |
container_volume | 15 |
description | <jats:p>Abstract. For more than two decades numerical models of the Earth's magnetosphere have been used successfully to study magnetospheric dynamic features such as the excitation of ULF pulsations and the mechanism of field line resonance. However, numerical formulations simplify important properties of the real system. For instance the Alfvén continuum becomes discrete because of a finite grid size. This discretization can be a possible source of numerical artefacts. Therefore a careful interpretation of any observed features is required. Examples of such artefacts are presented using results from a three dimensional dipole model of the magnetosphere, including an inhomogeneous distribution of the Alfvén velocity. </jats:p> |
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id | ai-49-aHR0cDovL2R4LmRvaS5vcmcvMTAuMTAwNy9zMDA1ODUtOTk3LTA2MTQtMA |
imprint | Copernicus GmbH, 1997 |
imprint_str_mv | Copernicus GmbH, 1997 |
institution | DE-Gla1, DE-Zi4, DE-15, DE-Pl11, DE-Rs1, DE-105, DE-14, DE-Ch1, DE-L229, DE-D275, DE-Bn3, DE-Brt1, DE-Zwi2, DE-D161 |
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physical | 614-624 |
publishDate | 1997 |
publishDateSort | 1997 |
publisher | Copernicus GmbH |
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recordtype | ai |
series | Annales Geophysicae |
source_id | 49 |
spelling | Stellmacher, M. Glassmeier, K.-H. Lysak, R. L. Kivelson, M. G. 1432-0576 Copernicus GmbH Space and Planetary Science Earth and Planetary Sciences (miscellaneous) Atmospheric Science Geology Astronomy and Astrophysics http://dx.doi.org/10.1007/s00585-997-0614-0 <jats:p>Abstract. For more than two decades numerical models of the Earth's magnetosphere have been used successfully to study magnetospheric dynamic features such as the excitation of ULF pulsations and the mechanism of field line resonance. However, numerical formulations simplify important properties of the real system. For instance the Alfvén continuum becomes discrete because of a finite grid size. This discretization can be a possible source of numerical artefacts. Therefore a careful interpretation of any observed features is required. Examples of such artefacts are presented using results from a three dimensional dipole model of the magnetosphere, including an inhomogeneous distribution of the Alfvén velocity. </jats:p> Field line resonances in discretized magnetospheric models: an artifact study Annales Geophysicae |
spellingShingle | Stellmacher, M., Glassmeier, K.-H., Lysak, R. L., Kivelson, M. G., Annales Geophysicae, Field line resonances in discretized magnetospheric models: an artifact study, Space and Planetary Science, Earth and Planetary Sciences (miscellaneous), Atmospheric Science, Geology, Astronomy and Astrophysics |
title | Field line resonances in discretized magnetospheric models: an artifact study |
title_full | Field line resonances in discretized magnetospheric models: an artifact study |
title_fullStr | Field line resonances in discretized magnetospheric models: an artifact study |
title_full_unstemmed | Field line resonances in discretized magnetospheric models: an artifact study |
title_short | Field line resonances in discretized magnetospheric models: an artifact study |
title_sort | field line resonances in discretized magnetospheric models: an artifact study |
title_unstemmed | Field line resonances in discretized magnetospheric models: an artifact study |
topic | Space and Planetary Science, Earth and Planetary Sciences (miscellaneous), Atmospheric Science, Geology, Astronomy and Astrophysics |
url | http://dx.doi.org/10.1007/s00585-997-0614-0 |