Literature DB >> 26542577

Discovery of diffuse aurora on Mars.

N M Schneider1, J I Deighan2, S K Jain2, A Stiepen2, A I F Stewart2, D Larson3, D L Mitchell3, C Mazelle4, C O Lee3, R J Lillis3, J S Evans5, D Brain2, M H Stevens6, W E McClintock2, M S Chaffin2, M Crismani2, G M Holsclaw2, F Lefevre7, D Y Lo8, J T Clarke9, F Montmessin8, B M Jakosky2.   

Abstract

Planetary auroras reveal the complex interplay between an atmosphere and the surrounding plasma environment. We report the discovery of low-altitude, diffuse auroras spanning much of Mars' northern hemisphere, coincident with a solar energetic particle outburst. The Imaging Ultraviolet Spectrograph, a remote sensing instrument on the Mars Atmosphere and Volatile Evolution (MAVEN) spacecraft, detected auroral emission in virtually all nightside observations for ~5 days, spanning nearly all geographic longitudes. Emission extended down to ~60 kilometer (km) altitude (1 microbar), deeper than confirmed at any other planet. Solar energetic particles were observed up to 200 kilo--electron volts; these particles are capable of penetrating down to the 60 km altitude. Given minimal magnetic fields over most of the planet, Mars is likely to exhibit auroras more globally than Earth.
Copyright © 2015, American Association for the Advancement of Science.

Entities:  

Year:  2015        PMID: 26542577     DOI: 10.1126/science.aad0313

Source DB:  PubMed          Journal:  Science        ISSN: 0036-8075            Impact factor:   47.728


  1 in total

1.  Discrete Aurora at Mars: Dependence on Upstream Solar Wind Conditions.

Authors:  Z Girazian; N M Schneider; Z Milby; X Fang; J Halekas; T Weber; S K Jain; J-C Gérard; L Soret; J Deighan; C O Lee
Journal:  J Geophys Res Space Phys       Date:  2022-04-05       Impact factor: 3.111

  1 in total

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