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A strong seasonal dependence in the Martian hydrogen exosphere
DOI: 10.1002/2015GL065804 Bibcode: 2015GeoRL..42.8678B

Bertaux, Jean-Loup; Chaufray, Jean-Yves; Clarke, John T. +2 more

Hubble Space Telescope and Mars Express observed unexpected rapid changes in the Martian hydrogen exosphere involving a decrease in scattered Lyman α intensity in fall 2007 (solar longitude, Ls = 331°-345°). These changes detected were speculated to be a combination of seasonal variation and/or dust storms and lower atmospheric dynamics…

2015 Geophysical Research Letters
MEx eHST 78
An ionized layer in the upper atmosphere of Mars caused by dust impacts from comet Siding Spring
DOI: 10.1002/2015GL063726 Bibcode: 2015GeoRL..42.4745G

Gurnett, D. A.; Persoon, A. M.; Morgan, D. D. +4 more

We report the detection of a dense ionized layer in the upper atmosphere of Mars caused by the impact of dust from comet Siding Spring. The observations were made by the ionospheric radar sounder on the Mars Express spacecraft during two low-altitude passes approximately 7 h and 14 h after closest approach of the comet to Mars. During these passes…

2015 Geophysical Research Letters
MEx 23
Ten years of Martian nitric oxide nightglow observations
DOI: 10.1002/2014GL062300 Bibcode: 2015GeoRL..42..720S

Montmessin, Franck; Bertaux, Jean-Loup; Stiepen, Arnaud +2 more

We present 10 years of Martian NO nightglow Spectroscopy for Investigation of Characteristics of the Atmosphere of Mars observations in limb and stellar occultation modes. The NO nightglow is used as a tracer of the summer-to-winter hemispherical circulation in the upper atmosphere of Mars. Its distribution roughly follows the curve latitude = -80…

2015 Geophysical Research Letters
MEx 11
The equivalent slab thickness of Mars' ionosphere: Implications for thermospheric temperature
DOI: 10.1002/2015GL063096 Bibcode: 2015GeoRL..42.3560M

Gurnett, D.; Mouginot, J.; Kofman, W. +4 more

The total electron content (TEC) of a planetary ionosphere is dominated by plasma near and above the height of maximum electron density (Nmax). The ratio TEC/Nmax represents the thickness (τ) of a TEC slab of uniform density (Nmax). For a photochemical ionosphere, τ relates to the scale height (H = kT/mg) of the io…

2015 Geophysical Research Letters
MEx 8