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Transpolar potential saturation: Roles of region 1 current system and solar wind ram pressure
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Zeitschriftentitel: | Journal of Geophysical Research: Space Physics |
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Personen und Körperschaften: | , , |
In: | Journal of Geophysical Research: Space Physics, 107, 2002, A10 |
Format: | E-Article |
Sprache: | Englisch |
veröffentlicht: |
American Geophysical Union (AGU)
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Schlagwörter: |
author_facet |
Siscoe, G. L. Crooker, N. U. Siebert, K. D. Siscoe, G. L. Crooker, N. U. Siebert, K. D. |
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author |
Siscoe, G. L. Crooker, N. U. Siebert, K. D. |
spellingShingle |
Siscoe, G. L. Crooker, N. U. Siebert, K. D. Journal of Geophysical Research: Space Physics Transpolar potential saturation: Roles of region 1 current system and solar wind ram pressure Paleontology Space and Planetary Science Earth and Planetary Sciences (miscellaneous) Atmospheric Science Earth-Surface Processes Geochemistry and Petrology Soil Science Water Science and Technology Ecology Aquatic Science Forestry Oceanography Geophysics |
author_sort |
siscoe, g. l. |
spelling |
Siscoe, G. L. Crooker, N. U. Siebert, K. D. 0148-0227 American Geophysical Union (AGU) Paleontology Space and Planetary Science Earth and Planetary Sciences (miscellaneous) Atmospheric Science Earth-Surface Processes Geochemistry and Petrology Soil Science Water Science and Technology Ecology Aquatic Science Forestry Oceanography Geophysics http://dx.doi.org/10.1029/2001ja009176 <jats:p>MHD simulations give about the same dependence of transpolar potential on solar wind electric field (IEF) as the Hill model of transpolar potential, including saturation and dependence on ram pressure. In the Hill model, feedback of the region 1 current system is presumed to limit the rate of reconnection at the magnetopause thereby causing transpolar potential saturation. MHD simulations add as relevant information that in the saturation domain the region 1 current system usurps the role of the Chapman‐Ferraro current system, which disappears. This means that the region 1 current system takes on the role of providing the current and generating most of the magnetic field in the <jats:bold>J</jats:bold> × <jats:bold>B</jats:bold> force at the magnetopause that balances solar wind ram pressure. Viewed from this perspective, transpolar potential saturation results not from the region 1 current system limiting the rate of reconnection at the magnetopause but instead from ram pressure (more accurately, total solar wind stresses) limiting the total amount of current that can flow in the region 1 current system. Transpolar potential saturation is then the limit on transpolar potential that corresponds to the ram‐pressure limit on total region 1 current.</jats:p> Transpolar potential saturation: Roles of region 1 current system and solar wind ram pressure Journal of Geophysical Research: Space Physics |
doi_str_mv |
10.1029/2001ja009176 |
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Online Free |
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Technik Geologie und Paläontologie Geographie Chemie und Pharmazie Land- und Forstwirtschaft, Gartenbau, Fischereiwirtschaft, Hauswirtschaft Biologie Allgemeine Naturwissenschaft Physik |
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American Geophysical Union (AGU), 2002 |
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American Geophysical Union (AGU), 2002 |
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American Geophysical Union (AGU) |
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Journal of Geophysical Research: Space Physics |
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title |
Transpolar potential saturation: Roles of region 1 current system and solar wind ram pressure |
title_unstemmed |
Transpolar potential saturation: Roles of region 1 current system and solar wind ram pressure |
title_full |
Transpolar potential saturation: Roles of region 1 current system and solar wind ram pressure |
title_fullStr |
Transpolar potential saturation: Roles of region 1 current system and solar wind ram pressure |
title_full_unstemmed |
Transpolar potential saturation: Roles of region 1 current system and solar wind ram pressure |
title_short |
Transpolar potential saturation: Roles of region 1 current system and solar wind ram pressure |
title_sort |
transpolar potential saturation: roles of region 1 current system and solar wind ram pressure |
topic |
Paleontology Space and Planetary Science Earth and Planetary Sciences (miscellaneous) Atmospheric Science Earth-Surface Processes Geochemistry and Petrology Soil Science Water Science and Technology Ecology Aquatic Science Forestry Oceanography Geophysics |
url |
http://dx.doi.org/10.1029/2001ja009176 |
publishDate |
2002 |
physical |
|
description |
<jats:p>MHD simulations give about the same dependence of transpolar potential on solar wind electric field (IEF) as the Hill model of transpolar potential, including saturation and dependence on ram pressure. In the Hill model, feedback of the region 1 current system is presumed to limit the rate of reconnection at the magnetopause thereby causing transpolar potential saturation. MHD simulations add as relevant information that in the saturation domain the region 1 current system usurps the role of the Chapman‐Ferraro current system, which disappears. This means that the region 1 current system takes on the role of providing the current and generating most of the magnetic field in the <jats:bold>J</jats:bold> × <jats:bold>B</jats:bold> force at the magnetopause that balances solar wind ram pressure. Viewed from this perspective, transpolar potential saturation results not from the region 1 current system limiting the rate of reconnection at the magnetopause but instead from ram pressure (more accurately, total solar wind stresses) limiting the total amount of current that can flow in the region 1 current system. Transpolar potential saturation is then the limit on transpolar potential that corresponds to the ram‐pressure limit on total region 1 current.</jats:p> |
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author | Siscoe, G. L., Crooker, N. U., Siebert, K. D. |
author_facet | Siscoe, G. L., Crooker, N. U., Siebert, K. D., Siscoe, G. L., Crooker, N. U., Siebert, K. D. |
author_sort | siscoe, g. l. |
container_issue | A10 |
container_start_page | 0 |
container_title | Journal of Geophysical Research: Space Physics |
container_volume | 107 |
description | <jats:p>MHD simulations give about the same dependence of transpolar potential on solar wind electric field (IEF) as the Hill model of transpolar potential, including saturation and dependence on ram pressure. In the Hill model, feedback of the region 1 current system is presumed to limit the rate of reconnection at the magnetopause thereby causing transpolar potential saturation. MHD simulations add as relevant information that in the saturation domain the region 1 current system usurps the role of the Chapman‐Ferraro current system, which disappears. This means that the region 1 current system takes on the role of providing the current and generating most of the magnetic field in the <jats:bold>J</jats:bold> × <jats:bold>B</jats:bold> force at the magnetopause that balances solar wind ram pressure. Viewed from this perspective, transpolar potential saturation results not from the region 1 current system limiting the rate of reconnection at the magnetopause but instead from ram pressure (more accurately, total solar wind stresses) limiting the total amount of current that can flow in the region 1 current system. Transpolar potential saturation is then the limit on transpolar potential that corresponds to the ram‐pressure limit on total region 1 current.</jats:p> |
doi_str_mv | 10.1029/2001ja009176 |
facet_avail | Online, Free |
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imprint | American Geophysical Union (AGU), 2002 |
imprint_str_mv | American Geophysical Union (AGU), 2002 |
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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publisher | American Geophysical Union (AGU) |
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series | Journal of Geophysical Research: Space Physics |
source_id | 49 |
spelling | Siscoe, G. L. Crooker, N. U. Siebert, K. D. 0148-0227 American Geophysical Union (AGU) Paleontology Space and Planetary Science Earth and Planetary Sciences (miscellaneous) Atmospheric Science Earth-Surface Processes Geochemistry and Petrology Soil Science Water Science and Technology Ecology Aquatic Science Forestry Oceanography Geophysics http://dx.doi.org/10.1029/2001ja009176 <jats:p>MHD simulations give about the same dependence of transpolar potential on solar wind electric field (IEF) as the Hill model of transpolar potential, including saturation and dependence on ram pressure. In the Hill model, feedback of the region 1 current system is presumed to limit the rate of reconnection at the magnetopause thereby causing transpolar potential saturation. MHD simulations add as relevant information that in the saturation domain the region 1 current system usurps the role of the Chapman‐Ferraro current system, which disappears. This means that the region 1 current system takes on the role of providing the current and generating most of the magnetic field in the <jats:bold>J</jats:bold> × <jats:bold>B</jats:bold> force at the magnetopause that balances solar wind ram pressure. Viewed from this perspective, transpolar potential saturation results not from the region 1 current system limiting the rate of reconnection at the magnetopause but instead from ram pressure (more accurately, total solar wind stresses) limiting the total amount of current that can flow in the region 1 current system. Transpolar potential saturation is then the limit on transpolar potential that corresponds to the ram‐pressure limit on total region 1 current.</jats:p> Transpolar potential saturation: Roles of region 1 current system and solar wind ram pressure Journal of Geophysical Research: Space Physics |
spellingShingle | Siscoe, G. L., Crooker, N. U., Siebert, K. D., Journal of Geophysical Research: Space Physics, Transpolar potential saturation: Roles of region 1 current system and solar wind ram pressure, Paleontology, Space and Planetary Science, Earth and Planetary Sciences (miscellaneous), Atmospheric Science, Earth-Surface Processes, Geochemistry and Petrology, Soil Science, Water Science and Technology, Ecology, Aquatic Science, Forestry, Oceanography, Geophysics |
title | Transpolar potential saturation: Roles of region 1 current system and solar wind ram pressure |
title_full | Transpolar potential saturation: Roles of region 1 current system and solar wind ram pressure |
title_fullStr | Transpolar potential saturation: Roles of region 1 current system and solar wind ram pressure |
title_full_unstemmed | Transpolar potential saturation: Roles of region 1 current system and solar wind ram pressure |
title_short | Transpolar potential saturation: Roles of region 1 current system and solar wind ram pressure |
title_sort | transpolar potential saturation: roles of region 1 current system and solar wind ram pressure |
title_unstemmed | Transpolar potential saturation: Roles of region 1 current system and solar wind ram pressure |
topic | Paleontology, Space and Planetary Science, Earth and Planetary Sciences (miscellaneous), Atmospheric Science, Earth-Surface Processes, Geochemistry and Petrology, Soil Science, Water Science and Technology, Ecology, Aquatic Science, Forestry, Oceanography, Geophysics |
url | http://dx.doi.org/10.1029/2001ja009176 |