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Ion distributions in the vicinity of Mars: Signatures of heating and acceleration processes
DOI: 10.5047/eps.2011.04.011 Bibcode: 2012EP&S...64..135N

Fedorov, A.; Barabash, S.; Lundin, R. +5 more

More than three years of data from the ASPERA-3 instrument on-board Mars Express has been used to compile average distribution functions of ions in and around the Mars induced magnetosphere. We present samples of average distribution functions, as well as average flux patterns based on the average distribution functions, all suitable for detailed …

2012 Earth, Planets and Space
MEx 45
Control of ion loss from Mars during solar minimum
DOI: 10.5047/eps.2011.05.037 Bibcode: 2012EP&S...64..165B

Brecht, Stephen H.; Ledvina, Stephen A.

A hybrid particle code has been used to examine the interaction of the solar wind with Mars during solar minimum. The results were surprising as they produced ion loss rates from Mars far in excess of what is estimated from MEX. The results are analyzed and found to be consistent with the competition between photochemical rates and advection of th…

2012 Earth, Planets and Space
MEx 26
Upper ionosphere of Mars is not axially symmetrical
DOI: 10.5047/eps.2011.05.022 Bibcode: 2012EP&S...64..113D

Gurnett, D. A.; Barabash, S.; Lundin, R. +6 more

The measurements carried out by the ASPERA-3 and MARSIS experiments on board the Mars Express (MEX) spacecraft show that the upper Martian ionosphere (h ≥ 400 km) is strongly azimuthally asymmetrical. There are several factors, e.g., the crustal magnetization on Mars and the orientation of the interplanetary magnetic field (IMF) which c…

2012 Earth, Planets and Space
MEx 20
Ion acceleration by multiple reflections at Martian bow shock
DOI: 10.5047/eps.2011.07.007 Bibcode: 2012EP&S...64...61Y

Fedorov, A.; Barabash, S.; Lundin, R. +7 more

The ion mass analyzer (IMA) on board Mars Express revealed bundled structures of ions in the energy domain within a distance of a proton gyroradius from the Martian bow shock. Seven prominent traversals during 2005 were examined when the energy-bunched structure was observed together with pick-up ions of exospheric origin, the latter of which is u…

2012 Earth, Planets and Space
MEx 6
Ionogram inversion for MARSIS topside sounding
DOI: 10.5047/eps.2012.03.006 Bibcode: 2012EP&S...64..753H

Wan, Weixing; Han, Xiuhong

In the present paper, we propose a method of ionogram inversion to retrieve the electron density profile, Ne(h), of the Martian ionosphere from the topside ionogram, which is measured by the Mars Advanced Radar for Subsurface and Ionosphere Sounding (MARSIS) instrument on board the Mars Express spacecraft. The new inversion technique is…

2012 Earth, Planets and Space
MEx 2