Search Publications

The structure and variability of Mars dayside thermosphere from MAVEN NGIMS and IUVS measurements: Seasonal and solar activity trends in scale heights and temperatures
DOI: 10.1002/2016JA023454 Bibcode: 2017JGRA..122.1296B

Stiepen, Arnaud; Schneider, Nicholas M.; Bougher, Stephen W. +10 more

Mars dayside thermospheric temperature and scale height trends were examined using measurements from the Neutral Gas Ion Mass Spectrometer (NGIMS) and the Imaging Ultraviolet Spectrograph (IUVS) on the Mars Atmosphere Volatile EvolutioN (MAVEN) spacecraft. Average scale heights (over 150-180 km for solar zenith angles ≤75°) from several different …

2017 Journal of Geophysical Research (Space Physics)
MEx 111
Interplanetary coronal mass ejection observed at STEREO-A, Mars, comet 67P/Churyumov-Gerasimenko, Saturn, and New Horizons en route to Pluto: Comparison of its Forbush decreases at 1.4, 3.1, and 9.9 AU
DOI: 10.1002/2017JA023884 Bibcode: 2017JGRA..122.7865W

Barabash, S.; Krupp, N.; Roussos, E. +48 more

We discuss observations of the journey throughout the Solar System of a large interplanetary coronal mass ejection (ICME) that was ejected at the Sun on 14 October 2014. The ICME hit Mars on 17 October, as observed by the Mars Express, Mars Atmosphere and Volatile EvolutioN Mission (MAVEN), Mars Odyssey, and Mars Science Laboratory (MSL) missions,…

2017 Journal of Geophysical Research (Space Physics)
MEx PROBA-2 Rosetta SOHO 96
Hot oxygen escape from Mars: Simple scaling with solar EUV irradiance
DOI: 10.1002/2016JA023461 Bibcode: 2017JGRA..122.1102C

Luhmann, J.; Cravens, T. E.; Combi, M. +8 more

The evolution of the atmosphere of Mars and the loss of volatiles over the lifetime of the solar system is a key topic in planetary science. An important loss process for atomic species, such as oxygen, is ionospheric photochemical escape. Dissociative recombination of O2+ ions (the major ion species) produces fast oxygen ato…

2017 Journal of Geophysical Research (Space Physics)
MEx 45
Martian magnetic storms
DOI: 10.1002/2016JA023513 Bibcode: 2017JGRA..122.6185L

Luhmann, J. G.; Russell, C. T.; Li, Y. +11 more

The response of Mars to the major space weather events called interplanetary coronal mass ejections (ICMEs) is of interest for both general planetary solar wind interaction studies and related speculations on their evolutionary consequences—especially with respect to atmosphere escape. Various particle and field signatures of ICMEs have been obser…

2017 Journal of Geophysical Research (Space Physics)
MEx 44
Global Mars-solar wind coupling and ion escape
DOI: 10.1002/2017JA024306 Bibcode: 2017JGRA..122.8051R

Barabash, Stas; Nilsson, Hans; Holmström, Mats +2 more

Loss of the early Martian atmosphere is often thought to have occurred due to an effective transfer of the solar wind energy through the Martian induced magnetic barrier to the ionosphere. We have quantified the coupling efficiency by comparing the power of the heavy ion outflow with the available power supplied by the upstream solar wind. Constra…

2017 Journal of Geophysical Research (Space Physics)
MEx 44
Solar wind- and EUV-dependent models for the shapes of the Martian plasma boundaries based on Mars Express measurements
DOI: 10.1002/2017JA024098 Bibcode: 2017JGRA..122.7279R

Barabash, Stas; Holmström, Mats; Futaana, Yoshifumi +1 more

The long operational life (2003-present) of Mars Express (MEX) has allowed the spacecraft to make plasma measurements in the Martian environment over a wide range of upstream conditions. We have analyzed ∼7000 MEX orbits, covering three orders of magnitude in solar wind dynamic pressure, with data from the on board Analyzer of Space Plasmas and En…

2017 Journal of Geophysical Research (Space Physics)
MEx 42
Comparative study of the Martian suprathermal electron depletions based on Mars Global Surveyor, Mars Express, and Mars Atmosphere and Volatile EvolutioN mission observations
DOI: 10.1002/2016JA023205 Bibcode: 2017JGRA..122..857S

André, N.; Fedorov, A.; Sauvaud, J. -A. +16 more

Nightside suprathermal electron depletions have been observed at Mars by three spacecraft to date: Mars Global Surveyor, Mars Express, and the Mars Atmosphere and Volatile EvolutioN (MAVEN) mission. This spatial and temporal diversity of measurements allows us to propose here a comprehensive view of the Martian electron depletions through the firs…

2017 Journal of Geophysical Research (Space Physics)
MEx 31
Mars plasma system response to solar wind disturbances during solar minimum
DOI: 10.1002/2016JA023587 Bibcode: 2017JGRA..122.6611S

Holmström, M.; Odstrcil, D.; Lester, M. +16 more

This paper is a phenomenological description of the ionospheric plasma and induced magnetospheric boundary (IMB) response to two different types of upstream solar wind events impacting Mars in March 2008, at the solar minimum. A total of 16 Mars Express orbits corresponding to five consecutive days is evaluated. Solar TErrestrial RElations Observa…

2017 Journal of Geophysical Research (Space Physics)
MEx 30
Nitric oxide nightglow and Martian mesospheric circulation from MAVEN/IUVS observations and LMD-MGCM predictions
DOI: 10.1002/2016JA023523 Bibcode: 2017JGRA..122.5782S

Forget, F.; Montmessin, F.; González-Galindo, F. +19 more

We report results from a study of nitric oxide nightglow over the northern hemisphere of Mars during winter, the southern hemisphere during fall equinox, and equatorial latitudes during summer in the northern hemisphere based on observations of the δ and γ bands between 190 and 270 nm by the Imaging UltraViolet Spectrograph (IUVS) on the Mars Atmo…

2017 Journal of Geophysical Research (Space Physics)
MEx 19
The transient topside layer and associated current sheet in the ionosphere of Mars
DOI: 10.1002/2016JA023591 Bibcode: 2017JGRA..122.5579K

Gurnett, Donald A.; Halekas, Jasper S.; DiBraccio, Gina A. +2 more

Radar soundings from the Mars Advanced Radar for Subsurface and Ionosphere Sounding (MARSIS) instrument on board the Mars Express spacecraft have shown that transient layers exist in the dayside upper ionosphere of Mars. The most prominent of these features is a second layer at an altitude near 200 km, well above that of the main photoionization l…

2017 Journal of Geophysical Research (Space Physics)
MEx 14