Europlanet Science Congress 2022
Palacio de Congresos de Granada, Spain
18 – 23 September 2022
Europlanet Science Congress 2022
Palacio de Congresos de Granada, Spain
18 September – 23 September 2022
EPSC Abstracts
Vol. 16, EPSC2022-724, 2022
https://doi.org/10.5194/epsc2022-724
Europlanet Science Congress 2022
© Author(s) 2023. This work is distributed under
the Creative Commons Attribution 4.0 License.

EMM EMUS Observations of Martian nightside discrete EUV and FUV Aurora

Robert Lillis1, Justin Deighan2, Sonal Jain2, Greg Holsclaw2, Matthew Fillingim1, Krishnaprasad Chirakkil2, Scott England3, Michael Chaffin2, David Brain2, Hessa Al Matroushi4, Fatma Lootah4, Hoor Al Mazmi4, Ed Thiemann2, Frank Eparvier2, Nick Schneider2, Jasper Halekas5, Suranga Ruhunusiri5, Jared Espley6, Jacob Gruesbeck6, and Shaosui Xu1
Robert Lillis et al.
  • 1Space Sciences Laboratory, University of California Berkeley, Berkeley, California, USA (rlillis@berkeley.edu)
  • 2Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, Colorado, USA
  • 3Department of Aerospace and Ocean Engineering, Virginia Tech, Blacksburg, Virginia, USA
  • 4Mohammed Bin Rashid Space Center, Dubai, United Arab Emirates
  • 5Department of Physics and Astronomy, University of Iowa, Iowa city, USA
  • 6Goddard Space Flight Center, Greenbelt, Maryland, USA

Here we report on synoptic (or “disk”) observations of Martian discrete aurora in the extreme and far ultraviolet (<200 nm), made by the Emirates Mars Ultraviolet Spectrometer (EMUS) on board the Emirates Mars Mission (EMM). EMM is well-suited to studying aurora due to its high altitude vantage point and regular observation cadence and the high sensitivity of the EMUS instrument.  The first EUV/EUV auroral spectra measured at Mars reveal O, C, and CO features from 99 to 165 nm. Auroral detection increases with solar activity and discrete aurorae display significant variability over ~20 minute timescales.  Three distinct types of discrete aurora have been identified based on these images.  The first type appears where Mars’ crustal magnetic fields are both strong and vertical and are consistent with point detections made by both Mars Express and MAVEN. The second appears in coherent patches away from crustal magnetic fields and is generally weak. The third is a new phenomenon, which we have named “sinuous discrete aurora” due to its serpentine shape, typically extending from the terminator thousands of kilometers into the nightside.  Investigation into its causes is ongoing but it likely reflects the morphology of Mars’ magnetotail current sheet.  Joint analysis of discrete aurora with EMM, MAVEN, and Mars Express promises to elucidate the processes driving the aurora on Mars.

How to cite: Lillis, R., Deighan, J., Jain, S., Holsclaw, G., Fillingim, M., Chirakkil, K., England, S., Chaffin, M., Brain, D., Al Matroushi, H., Lootah, F., Al Mazmi, H., Thiemann, E., Eparvier, F., Schneider, N., Halekas, J., Ruhunusiri, S., Espley, J., Gruesbeck, J., and Xu, S.: EMM EMUS Observations of Martian nightside discrete EUV and FUV Aurora, Europlanet Science Congress 2022, Granada, Spain, 18–23 Sep 2022, EPSC2022-724, https://doi.org/10.5194/epsc2022-724, 2022.

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