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Storm-Time Penetration Electric Fields and Their Effects

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TLDR
In this article, it was shown that when the magnetospheric convection is enhanced following a southward turning of the interplanetary magnetic field (IMF), the initial high-latitude electric field will penetrate to the equatorial latitudes.
Abstract
The ‘convection’ electric field, set up in the magnetosphere by the interaction of the solar wind plasma flowing around the Earth's magnetic field, projects along magnetic field lines to low altitudes where it drives the high-latitude ionospheric convection. During active times, ionospheric electric fields are thought to originate from two sources: a disturbed wind dynamo and electric fields that penetrate from high latitudes. In the latter, when the magnetospheric convection is enhanced following a southward turning of the interplanetary magnetic field (IMF), the initial high-latitude electric field will penetrate to the equatorial latitudes.

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Citations
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Response of the equatorial ionosphere at dusk to penetration electric fields during intense magnetic storms

TL;DR: In this article, the authors investigated the response of the equatorial ionosphere at dusk to the intense magnetic storms of 30 October 2003 and 20 November 2003, different aspects of which have been widely studied by the community.
Journal ArticleDOI

Penetration electric fields: Efficiency and characteristic time scale

TL;DR: In this paper, the authors presented a statistical result of the efficiency of IEF penetration to the dayside equatorial ionosphere; the efficiency is defined as the ratio of the change of the equatorial Ionospheric electric field to the change in the IEF.
Journal ArticleDOI

Local time dependent response of postsunset ESF during geomagnetic storms

TL;DR: In this paper, the authors report the results of a multi-instrumental (ground-based and space-borne) and multistation study on the development/inhibition of postsunset ESF during five moderate to intense geomagnetic storms occurred during the low and descending phase of the solar activity period, 2004-2006.
References
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Journal ArticleDOI

Self‐consistent calculation of the motion of a sheet of ions in the magnetosphere

TL;DR: In this paper, the effects of Birkeland currents from the inner edge of a sheet of ions that moves under the influence of the computed electric fields were investigated, and the results of the model calculations support the idea that convection electric fields bring low-energy ions in from the tail to form the storm time ring current.
Journal ArticleDOI

SAPS: A new categorization for sub‐auroral electric fields

TL;DR: The continued use of descriptive terms such as penetration electric fields, polarization jets, and sub-auroral ion drifts could lead to misunderstanding, especially when comparing the broad/narrow, persistent/transient regions of sub- auroral electric field and plasma flow.
Journal ArticleDOI

On the control of magnetospheric convection by the spatial distribution of ionospheric conductivities

TL;DR: In this article, a self-consistent semianalytical model of magnetospheric convection including the effect of the latitude and local time variations of ionospheric conductivities is presented.
Journal ArticleDOI

Long‐duration penetration of the interplanetary electric field to the low‐latitude ionosphere during the main phase of magnetic storms

TL;DR: In this paper, the authors present the observations of the dayside ionospheric electric field enhancements at middle and low latitudes in association with reorientations of the interplanetary magnetic field.

SAPS: A new categorization for sub-auroral electric fields

TL;DR: Sub-auroral electric fields play critical roles in energizing and transporting ring current ions, as well as convecting thermal plasma in the inner magnetosphere and in the mid- to low-latitude ionosphere as mentioned in this paper.
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