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Substorm Current Wedge Revisited

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TLDR
In this article, the substorm current wedge was developed to explain the magnetic signatures observed on the ground and in geosynchronous orbit during substorm expansion, and new observations, including radar and low altitude spacecraft, MHD simulations, and theoretical considerations have tremendously ad-vanced our understanding of this system.
Abstract
Almost 40 years ago the concept of the substorm current wedge was developed to explain the magnetic signatures observed on the ground and in geosynchronous orbit during substorm expansion. In the ensuing decades new observations, including radar and low- altitude spacecraft, MHD simulations, and theoretical considerations have tremendously ad- vanced our understanding of this system. The AMPTE/IRM, THEMIS and Cluster missions have added considerable observational knowledge, especially on the important role of fast flows in producing the stresses that generate the substorm current wedge. Recent detailed, multi-spacecraft, multi-instrument observations both in the magnetosphere and in the iono- sphere have brought a wealth of new information about the details of the temporal evolution and structure of the current system. While the large-scale picture remains valid, the new

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Challenges to Understanding the Earth's Ionosphere and Thermosphere

TL;DR: In this paper, the authors discuss the challenges to understanding and description of the coupled plasma and neutral gas that make up the ionosphere and thermosphere (I•T) and discuss some of the challenges that must be addressed to understand how the I•T responds to coupling from the surrounding regions of geospace.
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SAPS/SAID revisited: A causal relation to the substorm current wedge

TL;DR: In this article, multispacecraft observations of enhanced flow/electric field channels in the inner magnetosphere and conjugate subauroral ionosphere were presented, and it was shown that the poleward electric field inherent in the SCW2L circuit, which demands closure of the Region 1 and Region 2 sense field aligned currents via meridional currents, is the ultimate cause of fast RC injection and SAPS on the duskside.
References
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Journal ArticleDOI

Interplanetary Magnetic Field and the Auroral Zones

TL;DR: In this article, it was found that a model with a southward interplanetary magnetic field leads to a natural explanation of the SD currents and speculative aspects of the problem as they appear at this time are discussed.
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The development of the auroral substorm.

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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A unifying theory of high-latitude geophysical phenomena and geomagnetic storms

TL;DR: In this article, the occurrence at high latitudes of a large number of geophysical phenomena, including geomagnetic agitation and bay disturbances, aurorae, and various irregular distri...
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Satellite studies of magnetospheric substorms on August 15, 1968: 9. Phenomenological model for substorms

TL;DR: In this paper, the authors present a phenomenological model of the magnetospheric substorm sequence, which can be divided into three main phases: the growth phase, the expansion phase, and the recovery phase.
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Neutral line model of substorms: Past results and present view

TL;DR: In this article, the authors reviewed the NENL model of magnetospheric substorms, including the role of coupling with the solar wind and interplanetary magnetic field, the growth phase sequence, the expansion phase (and onset), and the recovery phase.
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