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Differentiating Diffuse Aurora Based on Phenomenology

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Abstract. There is mounting evidence which suggests that pulsating auroral patches often move with convection. This study is an initial step at identifying the differences between patches that move with convection and those that do not. While many properties of pulsating patches vary, here we outline criteria for separating pulsating auroral patches into three categories based on two properties: their structural stability and the spatial extent of their pulsations. Patchy aurora is characterized by stable structures whose pulsations are limited to small regions. Patchy pulsating aurora consists of stable patches whose pulsations are much less subtle and occur throughout much of their area. Amorphous pulsating auroral structures are unstable – very rapidly evolving – and can pulsate over their entire area. The speed with which amorphous pulsating aurora evolves makes their motion difficult to ascertain and seems unrelated to the E × B drifting of cold, equatorial plasma.
Title: Differentiating Diffuse Aurora Based on Phenomenology
Description:
Abstract.
There is mounting evidence which suggests that pulsating auroral patches often move with convection.
This study is an initial step at identifying the differences between patches that move with convection and those that do not.
While many properties of pulsating patches vary, here we outline criteria for separating pulsating auroral patches into three categories based on two properties: their structural stability and the spatial extent of their pulsations.
Patchy aurora is characterized by stable structures whose pulsations are limited to small regions.
Patchy pulsating aurora consists of stable patches whose pulsations are much less subtle and occur throughout much of their area.
Amorphous pulsating auroral structures are unstable – very rapidly evolving – and can pulsate over their entire area.
The speed with which amorphous pulsating aurora evolves makes their motion difficult to ascertain and seems unrelated to the E × B drifting of cold, equatorial plasma.

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