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...

Descripción completa

Guardado en:
Detalles Bibliográficos
Autor principal: Van Zele, M.A.
Formato: JOUR
Materias:
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_00393169_v46_n1_p33_VanZele
Aporte de:
id todo:paper_00393169_v46_n1_p33_VanZele
record_format dspace
spelling 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