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New science in plain sight: Citizen scientists lead to the discovery of optical structure in the upper atmosphere

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...

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Detalles Bibliográficos
Autores principales: MacDonald, Elizabeth A., Donovan, Eric, Nishimura, Yukitoshi, Case, Nathan A., Gillies, D. Megan, Gallardo-Lacourt, Bea, Archer, William E., Spanswick, Emma L., Bourassa, Notanee, Connors, Martin, Heavner, Matthew, Jackel, Brian, Kosar, Burcu, Knudsen, David J., Ratzlaff, Chris, Schofield, Ian
Formato: Online Artículo Texto
Lenguaje:English
Publicado: American Association for the Advancement of Science 2018
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5851661/
https://www.ncbi.nlm.nih.gov/pubmed/29546244
http://dx.doi.org/10.1126/sciadv.aaq0030
Descripción
Sumario: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).