Simulation study of near-Earth space disturbances: 1. magnetic storms
Abstract A magnetic storm is the world-wide geomagnetic disturbance taking place in near-Earth space environment, lasting for a few days. Geomagnetic fields can be depressed by ~ 1% on the ground for large magnetic storms. The prime cause of the long-lasting, world-wide geomagnetic disturbance is th...
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doaj-45bbfbeff2464589b1a1dc5c072c5bd52020-11-25T02:56:53ZengSpringerOpenProgress in Earth and Planetary Science2197-42842019-02-016112010.1186/s40645-019-0264-3Simulation study of near-Earth space disturbances: 1. magnetic stormsYusuke Ebihara0Research Institute for Sustainable Humanosphere, Kyoto UniversityAbstract A magnetic storm is the world-wide geomagnetic disturbance taking place in near-Earth space environment, lasting for a few days. Geomagnetic fields can be depressed by ~ 1% on the ground for large magnetic storms. The prime cause of the long-lasting, world-wide geomagnetic disturbance is the development of the ring current that surrounds the Earth. The ring current is an electric current carried by charged particles. Thus, the growth and decay of the ring current correspond to accumulation and loss of the ring current particles, respectively. The ring current is strong enough to modulate near-Earth space environment, and leads to many observable effects. In this sense, the ring current can be regarded as an important mediator in the near-Earth space environment. Here, the dynamics and structure of the ring current and its active role are briefly reviewed on the basis of numerical simulation results.http://link.springer.com/article/10.1186/s40645-019-0264-3Magnetic stormsComputer simulationMagnetosphereIonosphereInner magnetosphereRing current |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Yusuke Ebihara |
spellingShingle |
Yusuke Ebihara Simulation study of near-Earth space disturbances: 1. magnetic storms Progress in Earth and Planetary Science Magnetic storms Computer simulation Magnetosphere Ionosphere Inner magnetosphere Ring current |
author_facet |
Yusuke Ebihara |
author_sort |
Yusuke Ebihara |
title |
Simulation study of near-Earth space disturbances: 1. magnetic storms |
title_short |
Simulation study of near-Earth space disturbances: 1. magnetic storms |
title_full |
Simulation study of near-Earth space disturbances: 1. magnetic storms |
title_fullStr |
Simulation study of near-Earth space disturbances: 1. magnetic storms |
title_full_unstemmed |
Simulation study of near-Earth space disturbances: 1. magnetic storms |
title_sort |
simulation study of near-earth space disturbances: 1. magnetic storms |
publisher |
SpringerOpen |
series |
Progress in Earth and Planetary Science |
issn |
2197-4284 |
publishDate |
2019-02-01 |
description |
Abstract A magnetic storm is the world-wide geomagnetic disturbance taking place in near-Earth space environment, lasting for a few days. Geomagnetic fields can be depressed by ~ 1% on the ground for large magnetic storms. The prime cause of the long-lasting, world-wide geomagnetic disturbance is the development of the ring current that surrounds the Earth. The ring current is an electric current carried by charged particles. Thus, the growth and decay of the ring current correspond to accumulation and loss of the ring current particles, respectively. The ring current is strong enough to modulate near-Earth space environment, and leads to many observable effects. In this sense, the ring current can be regarded as an important mediator in the near-Earth space environment. Here, the dynamics and structure of the ring current and its active role are briefly reviewed on the basis of numerical simulation results. |
topic |
Magnetic storms Computer simulation Magnetosphere Ionosphere Inner magnetosphere Ring current |
url |
http://link.springer.com/article/10.1186/s40645-019-0264-3 |
work_keys_str_mv |
AT yusukeebihara simulationstudyofnearearthspacedisturbances1magneticstorms |
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1724711804451422208 |