The Vertical Distribution of the Optical Emissions of a Steve and Picket Fence Event. Issue 19 (11th October 2019)

• Record Type: Journal Article
• Authors: 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.; Eurich, D.
• Is Part Of: Geophysical research letters. Volume 46:Issue 19(2019)
• Page Start: 10719
• Page End: 10725
• Publication Date: 2019-10-11
• Subjects: Steve -- photography -- altitude -- triangulation -- ionosphere; Geophysics -- Periodicals; Planets -- Periodicals; Lunar geology -- Periodicals; 550
• DOI: 10.1029/2019GL084473
• Languages: English
• ISSNs: 0094-8276

Abstract

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. Key Points: The optical emissions of Steve range from 130 to 270 km in altitude The optical emissions of the green Picket Fence range from 95 to 150 km in altitude Steve and the Picket Fence extend vertically along similar magnetic field lines