Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
1780935 | Planetary and Space Science | 2015 | 9 Pages |
Abstract
The absence of visible spectrometers dedicated to these observations onboard existing space missions and the location of the different Martian rovers, far from the vertically aligned crustal magnetic field lines of Mars, have prevented so far the observations of such an aurora. In the foreseeable future, two missions may help observing these aurorae: the exo-Mars/Trace Gas Orbiter mission will carry a visible spectrometer which could be used to detect these events in the visible spectral range. NOMAD (Nadir and Occultation for Mars Discovery) will carry a UV-visible spectrometer in the 200-650Â nm range.
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Geophysics
Authors
J. Lilensten, D. Bernard, M. Barthélémy, G. Gronoff, C. Simon Wedlund, A. Opitz,