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Was Magnetic Storm the Only Driver of the Long-Duration Enhancements of Daytime Total Electron Content in the Asian-Australian Sector Between 7 and 12 September 2017?

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This article is published in Journal of Geophysical Research.The article was published on 2018-04-01 and is currently open access. It has received 91 citations till now. The article focuses on the topics: Geomagnetic storm & Daytime.

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Penetration of high latitude electric fields effects tolow latitude during Sundial 1984

TL;DR: In this article, electric field penetration events were identified using F-region vertical-drift measurements obtained in the October 6-13, 1984 period by Jicamarcan incoherent-backscatter radar and corresponding h-prime F measurements from ionosondes at Fortaleza, Cachoeira Paulista, and Dakar.
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Merging of Storm Time Midlatitude Traveling Ionospheric Disturbances and Equatorial Plasma Bubbles

TL;DR: In this paper, a combination of the Millstone Hill incoherent scatter radar data and 2D detrended total electron content (TEC) from ground-based Global Navigation Satellite System receivers was used to analyze the characteristics of midlatitude traveling ionospheric disturbances (TIDs) and equatorial plasma bubbles (EPBs) over American sector during the geomagnetic storm on 8 September 2017.

African Meridian B-field Education and Research (AMBER) Array

TL;DR: The AMBER array as discussed by the authors is the largest land-based gap in global magnetometer coverage, and it will address two fundamental areas of space physics: (1) the processes governing electrodynamics of the equatorial ionosphere as a function of latitude (or L-shell), local time, longitude, magnetic activity, and season, and (2) ULF pulsation strength and its connection with equatorial electrojet strength at low/mid-latitude regions.
References
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Journal ArticleDOI

What is a geomagnetic storm

TL;DR: In this article, an attempt is made to define a geomagnetic storm as an interval of time when a sufficiently intense and long-lasting interplanetary convection electric field leads, through a substantial energization in the magnetosphere-ionosphere system, to an intensified ring current sufficiently strong to exceed some key threshold of the quantifying storm time Dst index.
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The ionospheric disturbance dynamo

TL;DR: In this article, a numerical simulation study of the thermospheric winds produced by auroral heating during magnetic storms, and of their global dynamo effects, establishes the main features of the ionospheric disturbance dynamo.
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Ionospheric Storms — A Review

TL;DR: In this paper, the authors reviewed the current understanding and recent advances in the study of ionospheric storms with emphasis on the F2-region, and proposed a global first principle physical model to simulate the storm response of the coupled neutral and ionized upper atmospheric constituents.
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Response of the thermosphere and ionosphere to geomagnetic storms

TL;DR: In this paper, four numerical simulations have been performed, at equinox, using a coupled thermosphere-ionosphere model, to illustrate the response of the upper atmosphere to geomagnetic storms.
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Improved Ionospheric Electrodynamic Models and Application to Calculating Joule Heating Rates

TL;DR: In this article, the authors used a hybrid technique to construct the high-latitude electric potentials and magnetic field aligned currents (FAC) as a function of the solar wind parameters.
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