Contributions to the ring current energy during geomagnetic storms
The purpose of this research was to study the complexity of the energization of the ring current during a geomagnetic storm, produced during southern Bz(IMF) by the injection of plasma sheet ions, accelerated by enhanced convective electric fields. This model assumes that the plasma sheet is continu...
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Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_00393169_v46_n1_p33_VanZele |
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todo:paper_00393169_v46_n1_p33_VanZele2023-10-03T14:49:36Z Contributions to the ring current energy during geomagnetic storms Van Zele, M.A. Ring current Solar wind-magnetosphere coupling geomagnetic storm magnetosphere solar wind The purpose of this research was to study the complexity of the energization of the ring current during a geomagnetic storm, produced during southern Bz(IMF) by the injection of plasma sheet ions, accelerated by enhanced convective electric fields. This model assumes that the plasma sheet is continuously populated by H+ from the sun and the ionosphere, and sporadically by ionospheric O+, making the ring current a coupled system whose energy can hardly be expressed analytically. When Bz(IMF) turns north, the ring current becomes uncoupled, and the energy decays exponentially if the storm is weak, or can be expressed as a combination of exponentials during strong storms representing the quick decay of O+ and the slower decay of H+, as has been shown. Fil:Van Zele, M.A. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_00393169_v46_n1_p33_VanZele |
institution |
Universidad de Buenos Aires |
institution_str |
I-28 |
repository_str |
R-134 |
collection |
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) |
topic |
Ring current Solar wind-magnetosphere coupling geomagnetic storm magnetosphere solar wind |
spellingShingle |
Ring current Solar wind-magnetosphere coupling geomagnetic storm magnetosphere solar wind Van Zele, M.A. Contributions to the ring current energy during geomagnetic storms |
topic_facet |
Ring current Solar wind-magnetosphere coupling geomagnetic storm magnetosphere solar wind |
description |
The purpose of this research was to study the complexity of the energization of the ring current during a geomagnetic storm, produced during southern Bz(IMF) by the injection of plasma sheet ions, accelerated by enhanced convective electric fields. This model assumes that the plasma sheet is continuously populated by H+ from the sun and the ionosphere, and sporadically by ionospheric O+, making the ring current a coupled system whose energy can hardly be expressed analytically. When Bz(IMF) turns north, the ring current becomes uncoupled, and the energy decays exponentially if the storm is weak, or can be expressed as a combination of exponentials during strong storms representing the quick decay of O+ and the slower decay of H+, as has been shown. |
format |
JOUR |
author |
Van Zele, M.A. |
author_facet |
Van Zele, M.A. |
author_sort |
Van Zele, M.A. |
title |
Contributions to the ring current energy during geomagnetic storms |
title_short |
Contributions to the ring current energy during geomagnetic storms |
title_full |
Contributions to the ring current energy during geomagnetic storms |
title_fullStr |
Contributions to the ring current energy during geomagnetic storms |
title_full_unstemmed |
Contributions to the ring current energy during geomagnetic storms |
title_sort |
contributions to the ring current energy during geomagnetic storms |
url |
http://hdl.handle.net/20.500.12110/paper_00393169_v46_n1_p33_VanZele |
work_keys_str_mv |
AT vanzelema contributionstotheringcurrentenergyduringgeomagneticstorms |
_version_ |
1807320452068016128 |