NASA NTRS · 20120010325
Persistent, Widespread Pulsating Aurora: A Case Study
Abstract
Observations of a pulsating aurora event occurring on February 11, 2008, using the THEMIS all-sky imager array, indicate a spatially and temporally continuous event with a duration of greater than 15 hours and covering a region with a maximum size of greater than 9 hours MLT. The optical pulsations are at times locally interrupted or drowned out by auroral substorm activity, but are observed in the same location once the discrete aurora recedes. The pulsations following the auroral breakup appear to be brighter and have a larger patch size than pre-substorm. This suggests that, while the onset of pulsating aurora is not necessarily dependent upon a substorm precursor, the pulsations are affected and possibly enhanced by the substorm process. The long duration of such pulsating aurora events, enduring for several hours without interruption, is far longer than the expected recovery phase of a substorm, suggesting that pulsating aurora is not strictly a recovery phase phenomenon.
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Jones, S. L., Lessard, M. R., Rychert, K., Spanswick,. E., Donovan, E., Jaynes, A. N.. 2012-01-01. Persistent, Widespread Pulsating Aurora: A Case Study. https://ntrs.nasa.gov/citations/20120010325
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