Analysis of HST, VLT and Gemini coordinated observations of Uranus late 2017 : a multi-spectral search for auroral signatures
L. Lamy, C. Berland, N. Andre, R. Prange, T. Fouchet, T. Encrenaz, E., Gendron, X. Haubois, C. Tao, T. Kim

TL;DR
This study analyzes multi-spectral observations of Uranus during a solar storm in 2017, revealing widespread H3+ emissions but no localized auroras, enhancing understanding of Uranus's magnetospheric response.
Contribution
It provides new high-resolution NIR images of Uranus's ionosphere, comparing them with FUV data to improve understanding of auroral activity during a solar event.
Findings
Detected bright southern auroral spot in FUV images.
Mapped H3+ emission across Uranus's disc, brighter near the south pole.
Found no evidence of localized auroral emission in NIR images.
Abstract
On 6 Sept. 2017, an exceptional coronal mass ejection departed from the Sun toward the Earth and Uranus, whose magnetospheres are sensitive to the solar wind. The resulting interplanetary shock triggered geomagnetic storm and intense aurora at Earth the next day and was predicted by MHD models to reach Uranus around 10-11 Nov. This event provided a unique opportunity to investigate the auroral response of the asymmetric Uranian magnetosphere in its intermediate equinox-to-solstice configuration. Coordinated multi-spectral observations were acquired with the Hubble Space Telescope (HST) in the far-UV (FUV), with the Very Large Telescope (VLT) and Gemini North in the near-IR (NIR) and with Chandra in the X-ray domain. In this study, we focus on the analysis of NIR images obtained between 9 and 17 Nov. 2017 which are compared to one FUV image acquired on 11 Nov. The latter reveals a bright…
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Taxonomy
TopicsAstro and Planetary Science
