TY - JOUR
T1 - New science in plain sight
T2 - Citizen scientists lead to the discovery of optical structure in the upper atmosphere
AU - MacDonald, Elizabeth A.
AU - Donovan, Eric
AU - Nishimura, Yukitoshi
AU - Case, Nathan A.
AU - Megan Gillies, D.
AU - Gallardo-Lacourt, Bea
AU - Archer, William E.
AU - Spanswick, Emma L.
AU - Bourassa, Notanee
AU - Connors, Martin
AU - Heavner, Matthew
AU - Jackel, Brian
AU - Kosar, Burcu
AU - Knudsen, David J.
AU - Ratzlaff, Chris
AU - Schofield, Ian
N1 - Publisher Copyright:
Copyright © 2018 The Authors, some rights reserved; exclusive licensee American Association for the Advancement of Science.
PY - 2018/3/14
Y1 - 2018/3/14
N2 - A glowing ribbon of purple light running east-west in the night sky has recently been observed by citizen scientists. This narrow, subauroral, visible structure, distinct from the traditional auroral oval, was largely undocumented in the scientific literature and little was known about its formation. Amateur photo sequences showed colors distinctly different from common types of aurora and occasionally indicated magnetic field-aligned substructures. Observations from the Swarm satellite as it crossed the arc have revealed an unusual level of electron temperature enhancement and density depletion, along with a strong westward ion flow, indicating that a pronounced subauroral ion drift (SAID) is associated with this structure. These early results suggest the arc is an optical manifestation of SAID, presenting new opportunities for investigation of the dynamic SAID signatures from the ground. On the basis of the measured ion properties and original citizen science name, we propose to identify this arc as a Strong Thermal Emission Velocity Enhancement (STEVE).
AB - A glowing ribbon of purple light running east-west in the night sky has recently been observed by citizen scientists. This narrow, subauroral, visible structure, distinct from the traditional auroral oval, was largely undocumented in the scientific literature and little was known about its formation. Amateur photo sequences showed colors distinctly different from common types of aurora and occasionally indicated magnetic field-aligned substructures. Observations from the Swarm satellite as it crossed the arc have revealed an unusual level of electron temperature enhancement and density depletion, along with a strong westward ion flow, indicating that a pronounced subauroral ion drift (SAID) is associated with this structure. These early results suggest the arc is an optical manifestation of SAID, presenting new opportunities for investigation of the dynamic SAID signatures from the ground. On the basis of the measured ion properties and original citizen science name, we propose to identify this arc as a Strong Thermal Emission Velocity Enhancement (STEVE).
UR - http://www.scopus.com/inward/record.url?scp=85043989693&partnerID=8YFLogxK
U2 - 10.1126/sciadv.aaq0030
DO - 10.1126/sciadv.aaq0030
M3 - Journal Article
C2 - 29546244
AN - SCOPUS:85043989693
VL - 4
JO - Science Advances
JF - Science Advances
IS - 3
M1 - eaaq0030
ER -