Journal ArticleFirst observations of continuum emission in dayside auroraPartamies, Noora; Dayton-Oxland, Rowan (ORCID:0000000196427647); Herlingshaw, Katie; Virtanen, Ilkka (ORCID:0000000271118888); Gallardo-Lacourt, Bea (ORCID:0000000336907547); Syrjäsuo, Mikko; Sigernes, Fred; Nishiyama, Takanori (ORCID:0000000236486589); Nishimura, Toshi; Barthelemy, Mathieu; Aruliah, Anasuya; Whiter, Daniel (ORCID:000000017130232X); Mielke, Lena; Grandin, Maxime (ORCID:0000000263739756); Karvinen, Eero (ORCID:0000000329464397); Spijkers, Marjan; Ledvina, Vincent E (ORCID:0000000301275105)<p>Abstract. We report the first observations of continuum emission at the poleward boundary of the dayside auroral oval. Spectral measurements of high-latitude continuum emissions resemble those of Strong Thermal Emission Velocity Enhancement (STEVE), with light characterized by colours such as white, pale pink, or mauve. The emission enhancement spans the entire visible wavelength range. However, unlike STEVE, the high-latitude dayside continuum emission events tightly follow the auroral particle precipitation, often forming field-aligned rays and other dynamic shapes. Some dayside emissions appeared as wide arcs or cloud-like structures within the red-emission-dominated dayside aurora. Our spectral measurements further suggest that the broadband continuum emission may extend into the near-infrared (NIR) regime. Similar to the STEVE emission, low-Earth-orbit measurements of plasma flow in the region of continuum emission show a strong horizontal cross-track velocity shear. Ground-based radar and optical observations provide evidence of both plasma and neutral heating, as well as upwelling, in connection to the continuum emissions. We conclude that the interplay between different heating mechanisms may be an important factor in generating high-latitude continuum emissions.</p>Copernicus2025-01-0110674372Annales Geophysicae432349 to 3671432-0576https://doi.org/10.5194/angeo-43-349-20252445467National Science Foundation