Abstract. We present a feasibility study for a submillimeter instrument on a small Mars
platform now under construction. The sensor will measure the emission from
atmospheric molecular oxygen, water, ozone, and hydrogen peroxide in order to
retrieve their volume mixing ratios and the changes therein over time. In
addition to these, the instrument will be able to limit the crustal magnetic
field, and retrieve temperature and wind speed with various degrees of
precision and resolution. The expected measurement precision before spatial
and temporal averaging is 15 to 25 ppmv for the molecular oxygen mixing
ratio, 0.2 ppmv for the gaseous water mixing ratio, 2 ppbv for the hydrogen
peroxide mixing ratio, 2 ppbv for the ozone mixing ratio, 1.5 to
2.5 µT for the magnetic field strength, 1.5 to 2.5 K for the
temperature profile, and 20 to 25 m s−1 for the horizontal wind
speed.