2021
DOI: 10.1029/2020gl091527
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Auroral Energy Flux and Joule Heating Derived From Global Maps of Field‐Aligned Currents

Abstract: We calculate auroral energy flux and Joule heating in the high‐latitude ionosphere for 27 geomagnetically active days using two‐dimensional maps of field‐aligned currents determined by the Active Magnetosphere and Planetary Response Experiment. The energy input to the ionosphere due to Joule heating increases more rapidly with geomagnetic activity than that due to precipitating particles. The energy flux varies more smoothly with time than Joule heating, which is impulsive in nature on time scales from minutes… Show more

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Cited by 15 publications
(16 citation statements)
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“…It is possible the Joule heating seen is associated with the partial ring currents present even during geomagnetically quiet days at all Dst index levels, as shown by Le et al [37]. The relativistic electron fluxes seen could result from viscous interactions that transfer energy from the solar wind to the magnetic field lines, which can energize the electrons in the radiation belts [36].…”
Section: Discussionmentioning
confidence: 85%
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“…It is possible the Joule heating seen is associated with the partial ring currents present even during geomagnetically quiet days at all Dst index levels, as shown by Le et al [37]. The relativistic electron fluxes seen could result from viscous interactions that transfer energy from the solar wind to the magnetic field lines, which can energize the electrons in the radiation belts [36].…”
Section: Discussionmentioning
confidence: 85%
“…When the solar wind enters the Earth's magnetosphere, the density of relativistic electrons increases in the initial phase, these electrons are then lost by different processes such as charge exchange of magnetospheric ions and pitch angle loss at mirror points in the radiation belts [36]. The precipitation of ions and electrons from the magnetosphere onto the ionosphere causes the aurora through collisions of these ions and electrons with neutral atoms in the atmosphere.…”
Section: Discussionmentioning
confidence: 99%
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“…(2018), Robinson et al. (2020, 2021), and Robinson and Zanetti (2021). Our model provides another option for the community to estimate the global conductance distribution using the FAC information from measurements, empirical models of FACs, or numerical models that can calculate FACs.…”
Section: Discussionmentioning
confidence: 94%