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Verification of Substorm Onset From Intruding Flow Channels With High‐Resolution SuperDARN Radar Flow Maps

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TLDR
In this article , the authors used two-dimensional ionospheric flow maps for further testing and found that the lower entropy of the new plasma likely changes the entropy distribution of the inner plasma sheet, a change possibly important for the substorm onset instability seen via the growing waves that demarcate substorm auroral onset.
Abstract
Auroral observations were first to identify the substorm, and later used to propose that substorm onset is triggered in the inner plasma sheet (equatorward portion of the auroral oval) by an intrusion of low entropy plasma comprising plasma sheet flow channels. Longitudinal localization makes the intruding flow channels difficult to observe with spacecraft. However, they are detectable in the ionosphere via the broader, two‐dimensional coverage by radars. Line‐of‐sight radar flow measurements have provided considerable support for the onset proposal. Here we use two‐dimensional, ionospheric flow maps for further testing. Since these maps are derived without the smoothing from global fits typically used for global convection maps, their spatial resolution is significantly improved, allowing representation of localized spatial structures. These maps show channels of enhanced ionospheric flow intruding to the time and location of substorm onset. We also see evidence that these intruding flows enter the plasma sheet from the polar cap, and that azimuthal spread of the reduced entropy plasma in the inner plasma sheet contributes to azimuthal onset spreading after initial onset. Identified events with appropriate radar data remain limited, but we have found no exceptions to consistency with flow channel triggering. Thus, these analyses strongly support the proposal that substorm onset is due to the intrusion of new plasma to the onset region. The lower entropy of the new plasma likely changes the entropy distribution of inner plasma sheet, a change possibly important for the substorm onset instability seen via the growing waves that demarcate substorm auroral onset.

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Unsolved problems: Mesoscale polar cap flow channels' structure, propagation, and effects on space weather disturbances

TL;DR: In this article, the authors uncover the features of these flow enhancements, including their structure, how they propagate across the polar cap, and what controls their dynamic effects after reaching the night-side plasma sheet.
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Global Observations of the Short‐Term Disturbances in the Geomagnetic Field and Induced Currents During the Supersubstorms Events of Solar Cycle 24

TL;DR: In this article , four supersubstorms of the solar cycle 24 are analyzed to investigate the global variations in the H•component and geomagnetic induced currents (GICs), and the response to the storm sudden commencement (SSC of the 2012 and 2017 events is observed differently over different latitude bands.
References
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TL;DR: In this paper, a working model of simultaneous auroral activity over the entire polar region is presented in terms of the auroral substorm, which has two characteristic phases, an expansive phase and a recovery phase.
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TL;DR: In this paper, the cross-tail current sheet shows a rapid growth in the current density, a large upsurge in the duskward ion bulk speed to nearly the ion thermal speed, an increase in the plasma pressure and its isotropy, a rise in the ion beta, and a decrease in the thickness of the current sheet to a length scale comparable to the thermal ion gyroradius.
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Plasma sheet instability related to the westward traveling surge

TL;DR: In this article, a detailed analysis of an isolated dispersionless substorm is performed on the basis of field and particle data collected in situ by the geostationary satellite GEOS 2 and of data from ground-based instruments installed close to the GEOS2 magnetic footprint.
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Detection of localized, plasma‐depleted flux tubes or bubbles in the midtail plasma sheet

TL;DR: In this article, the authors present multi-instrument observations from the ISEE1 and ISEE 2 spacecraft to argue that when the plasma sheet becomes thick and close to its equilibrium state, the plasma and magnetic field signatures of high-speed flow events are consistent with the theoretically predicted signatures of plasma-depleted flux tubes or "bubbles".
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The THEMIS Array of Ground-based Observatories for the Study of Auroral Substorms

TL;DR: The NASA Time History of Events and Macroscale Interactions during Substorms (THEMIS) project as mentioned in this paper is intended to investigate magnetospheric substorm phenomena by using five in-situ satellites and ground-based all-sky imagers and magnetometers.