HAL will be down for maintenance from Friday, June 10 at 4pm through Monday, June 13 at 9am. More information
Skip to Main content Skip to Navigation
Journal articles

Global Aurora on Mars during the September 2017 Space Weather Event

Nicholas Schneider 1 Sonal Jain 1 Justin Deighan 1 Nasr Camella-Rosa 1 David Brain 1 Davin Larson 2 Robert Lillis 2 Ali Rahmati 2 Jasper Halekas 3 Christina O. Lee 2 Michael Chaffin 1 Arnaud Stiepen 4 Matteo Crismani 1 J. Evans 5 Michael H. Stevens 6 Daniel Lo 7 William E. Mcclintock 1 A. Stewart 1 Roger V. Yelle 7 John Clarke 8 Gregory Holsclaw 1 Franck Lefèvre 9 Franck Montmessin 9 Bruce Jakosky 1
1 LASP - Laboratory for Atmospheric and Space Physics [Boulder]
2 SSL - Space Sciences Laboratory [Berkeley]
3 Department of Physics and Astronomy [Iowa City]
4 LPAP - Laboratoire de Physique Atmosphérique et Planétaire
5 Computational Physics, Inc.
6 NRL - Naval Research Laboratory
7 LPL - Lunar and Planetary Laboratory [Tucson]
8 CSP - Center for Space Physics [Boston]
9 PLANETO - LATMOS
LATMOS - Laboratoire Atmosphères, Milieux, Observations Spatiales
Abstract : We report the detection of bright aurora spanning Mars’ nightside during the space weather event occurring in September 2017. The phenomenon was similar to diffuse aurora detected previously at Mars, but 25 times brighter and detectable over the entire visible nightside. The observations were made with the Imaging UltraViolet Spectrograph (IUVS), a remote sensing instrument on the Mars Atmosphere and Volatile EvolutioN (MAVEN) spacecraft orbiting Mars. Images show that the emission was brightest around the limb of the planet, with a fairly uniform faint glow against the disk itself. Spectra identified four molecular emissions associated with aurora, and limb scans show the emission originated from an altitude of ~60 km in the atmosphere. Both are consistent with very high energy particle precipitation. The auroral brightening peaked around 13 September, when the flux of solar energetic electrons and protons both peaked. During the declining phase of the event, faint but statistically significant auroral emissions briefly appeared against the disk of the planet in the form of narrow wisps and small patches. These features are approximately aligned with predicted open field lines in the region of strong crustal magnetic fields in Mars’ southern hemisphere.
Document type :
Journal articles
Complete list of metadata

Cited literature [17 references]  Display  Hide  Download
https://hal-insu.archives-ouvertes.fr/insu-01803835
Contributor : Catherine Cardon Connect in order to contact the contributor
Submitted on : Thursday, August 6, 2020 - 4:32:02 PM
Last modification on : Friday, December 3, 2021 - 11:42:50 AM
Long-term archiving on: : Monday, November 30, 2020 - 3:58:09 PM

File

Vignette du document
2018GL077772.pdf
Publisher files allowed on an open archive

Identifiers

Collections

SORBONNE-UNIVERSITE | SU-SCIENCES | LATMOS | UPMC | UNIV-PARIS-SACLAY | CNRS | INSU | UVSQ | SU-TI | GS-ENGINEERING | INSTITUT-SCIENCES-LUMIERE | GS-GEOSCIENCES

Citation

Nicholas Schneider, Sonal Jain, Justin Deighan, Nasr Camella-Rosa, David Brain, et al.. Global Aurora on Mars during the September 2017 Space Weather Event. Geophysical Research Letters, American Geophysical Union, 2018, 45 (15), pp.7391-7398. ⟨10.1029/2018GL077772⟩. ⟨insu-01803835⟩

Export

BibTeX TEI DC DCterms EndNote Datacite

Share

Metrics

Record views

122

Files downloads

84