UCL Discovery
UCL home » Library Services » Electronic resources » UCL Discovery

Energization of the Ring Current by Substorms

Sandhu, JK; Rae, IJ; Freeman, MP; Forsyth, C; Gkioulidou, M; Reeves, GD; Spence, HE; ... Lam, MM; + view all (2018) Energization of the Ring Current by Substorms. Journal of Geophysical Research: Space Physics 10.1029/2018JA025766. Green open access

[thumbnail of Sandhu_et_al-2018-Journal_of_Geophysical_Research%3A_Space_Physics.pdf]
Preview
Text
Sandhu_et_al-2018-Journal_of_Geophysical_Research%3A_Space_Physics.pdf - Published Version

Download (2MB) | Preview

Abstract

The substorm process releases large amounts of energy into the magnetospheric system, although where the energy is transferred to and how it is partitioned remains an open question. In this study, we address whether the substorm process contributes a significant amount of energy to the ring current. The ring current is a highly variable region, and understanding the energization processes provides valuable insight into how substorm-ring current coupling may contribute to the generation of storm conditions and provide a source of energy for wave driving. In order to quantify the energy input into the ring current during the substorm process, we analyze Radiation Belt Storm Probes Ion Composition Experiment and Helium Oxygen Proton Electron ion flux measurements for H+, O+, and He+. The energy content of the ring current is estimated and binned spatially for L and magnetic local time. The results are combined with an independently derived substorm event list to perform a statistical analysis of variations in the ring current energy content with substorm phase. We show that the ring current energy is significantly higher in the expansion phase compared to the growth phase, with the energy enhancement persisting into the substorm recovery phase. The characteristics of the energy enhancement suggest the injection of energized ions from the tail plasma sheet following substorm onset. The local time variations indicate a loss of energetic H+ions in the afternoon sector, likely due to wave-particle interactions. Overall, we find that the average energy input into the ring current is ∼9% of the previously reported energy released during substorms.

Type: Article
Title: Energization of the Ring Current by Substorms
Open access status: An open access version is available from UCL Discovery
DOI: 10.1029/2018JA025766
Publisher version: https://doi.org/10.1029/2018JA025766
Language: English
Additional information: © 2018. The Authors. This is an open access article under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0/), which permits use, distribution and reproduction in any medium, provided the original work is properly cited.
Keywords: ring current, substorms, magnetosphere, RBSPICE, HOPE, Van Allen Probes
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Space and Climate Physics
URI: https://discovery.ucl.ac.uk/id/eprint/10059968
Downloads since deposit
17Downloads
Download activity - last month
Download activity - last 12 months
Downloads by country - last 12 months

Archive Staff Only

View Item View Item