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On the Creation, Depletion, and End of Life of Polar Cap Patches

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AMER GEOPHYSICAL UNION
DOI: 10.1029/2023JA031739

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polar cap patches; airglow patches; plasma density decay; SuperDARN; ionospheric convection; plasma transport

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Ionospheric convection patterns from the Super Dual Auroral Radar Network were used to track the trajectories, transit times, and decay rates of polar cap patches. The study found that polar cap patches have variable plasma decay rates at different stages of their lifetime, and stagnation is considered a major determinant for complete decay.
Ionospheric convection patterns from the Super Dual Auroral Radar Network are used to determine the trajectories, transit times, and decay rates of three polar cap patches from their creation in the dayside polar cap ionosphere to their end of life on the nightside. The first two polar cap patches were created within 12 min of each other and traveled through the dayside convection throat, before entering the nightside auroral oval after 104 and 92 min, respectively. When the patches approached the nightside auroral oval, an intensification in the poleward auroral boundary occurred close to their exit point, followed by a decrease in the transit velocity. The last patch (patch 3) decayed completely within the polar cap and had a lifetime of only 78 min. After a change in drift direction, patch 3 had a radar backscatter power half-life of 4.23 min, which reduced to 1.80 min after a stagnation, indicating a variable decay rate. 28 minutes after the change in direction, and 16 min after coming to a halt within the Clyde River radar field-of-view, patch 3 appeared to reach its end of life. We relate this rapid decay to increased frictional heating, which speeds up the recombination rate. Therefore, we suggest that the slowed patch motion within the polar cap convection pattern is a major factor in determining whether the patch survives as a recognizable density enhancement by the time the flux tubes comprising the initial patch cross into the nightside auroral oval. Tracking of high-density plasma volumes in the ionosphere is a viable tool for uniting spatially distant observationsA drifting polar cap patch has variable plasma decay rate at different stages of its lifetimeStagnation of a polar cap patch is considered a major determinant for a complete decay

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