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.
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Formation of Continuum Emission Structures Associated With the Aurora
Abstract Recent observations enabled by improvements in geospace remote‐sensing instrumentation have revealed the spatial structure of continuum emissions that appear to be associated with the aurora, but little is known about the formation and drivers of these structures. We perform the first comprehensive statistical study of 52 auroral continuum structures identified using the Transition Region Explorer (TREx) network of broadband color all‐sky imagers and meridian imaging spectrographs. Superposed epoch analyses of global geomagnetic conditions reveal storm‐level activity and show that these structures appear statistically during the peak of geomagnetic disturbances. On average, the disturbance storm‐time index (Dst) decreases by approximately 50 nT to moderate storm levels in the 30 hr preceding emission observation, while the planetaryK(Kp) index rises from roughly 2 to 4.5. TREx optical data reveal a sharply peaked, spectrally “gray” luminosity that exceeds that of the surrounding aurora. The TREx auroral transport model indicates a surge of precipitating electron energy flux of approximately 5 erg/cm2/s spatially coincident with the structures themselves. A multi‐imager case study indicates that this enhancement is a coherent mesoscale region that tracks the visible structure. These results demonstrate that active geomagnetic conditions support the formation of these structures and suggest a direct coupling to energetic electron precipitation. Simultaneous observation of a broadband continuum enhancement with enhanced precipitation may favor a chemiluminescent nitric‐oxide continuum generation mechanism, although uncertainties remain regarding the viability of this mechanism.
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- Award ID(s):
- 2445467
- PAR ID:
- 10674374
- Publisher / Repository:
- Wiley
- Date Published:
- Journal Name:
- Journal of Geophysical Research: Space Physics
- Volume:
- 131
- Issue:
- 3
- ISSN:
- 2169-9380
- Format(s):
- Medium: X
- Sponsoring Org:
- National Science Foundation
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