The Vertical Distribution of the Optical Emissions of a Steve and Picket Fence Event
Document Type
Article
Publication Date
10-16-2019
Abstract
So-called “Steve” subauroral purple emissions have recently been uncovered by auroral photographers and have rapidly become an intense subject of debate as to their origin. In some events, nearby periodic green emissions have also been uncovered and given the name “picket fence,” owing to their appearance. The present paper advances our understanding of these phenomena by narrowing down the altitude extent of the Steve and picket fence emissions. Our determination is based on the event of 16 September 2017, which was simultaneously observed from two vantage points, allowing for a determination of the height range of Steve and picket fence through triangulation. We show that the picket fence extend between 95- and 150-km altitude and is aligned with the geomagnetic field, while the Steve altitude spread is between 130 and 270 km. We also show the two phenomena to be on nearby or perhaps the same magnetic field lines.
Identifier
85074189138 (Scopus)
Publication Title
Geophysical Research Letters
External Full Text Location
https://doi.org/10.1029/2019GL084473
e-ISSN
19448007
ISSN
00948276
First Page
10719
Last Page
10725
Issue
19
Volume
46
Fund Ref
Natural Sciences and Engineering Research Council of Canada
Recommended Citation
Archer, W. E.; St.- Maurice, J. P.; Gallardo-Lacourt, B.; Perry, G. W.; Cully, C. M.; Donovan, E.; Gillies, D. M.; Downie, R.; Smith, J.; and Eurich, D., "The Vertical Distribution of the Optical Emissions of a Steve and Picket Fence Event" (2019). Faculty Publications. 7268.
https://digitalcommons.njit.edu/fac_pubs/7268