On the Persistent Shape and Coherence of Pulsating Auroral Patches
B.K. Humberset, J.W. Gjerloev, I.R. Mann, R.G. Michell, M. Samara

TL;DR
This study quantitatively analyzes pulsating auroral patches, revealing their shape persistence over several minutes and their incoherent fluctuations, with implications for understanding auroral dynamics and streaming modes.
Contribution
It provides the first detailed quantitative assessment of the shape and coherence of pulsating auroral patches using all-sky camera data, avoiding space-time ambiguity.
Findings
Patches maintain their shape for 4.5-8.5 minutes with 85-100% similarity.
Larger patches show negative correlation with distance, indicating incoherent fluctuations.
Patches drift at 230-287 m/s NE, consistent with convection return flow.
Abstract
The pulsating aurora covers a broad range of fluctuating shapes that are poorly characterized. The purpose of this paper is therefore to provide objective and quantitative measures of the extent to which pulsating auroral patches maintain their shape, drift and fluctuate in a coherent fashion. We present results from a careful analysis of pulsating auroral patches using all-sky cameras. We have identified four well-defined individual patches that we follow in the patch frame of reference. In this way we avoid the space-time ambiguity which complicates rocket and satellite measurements. We find that the shape of the patches is remarkably persistent with 85-100% of the patch being repeated for 4.5-8.5 min. Each of the three largest patches has a temporal correlation with a negative dependence on distance, and thus does not fluctuate in a coherent fashion. A time-delayed response within…
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