... Sensitivity of mass content of hydrogen at the level of 10 -3 in 1 m layer of Martiansurface; . ... Sensitivity of mass content of hydrogen at the level of 10 -3 in 1 m layer of Martiansurface with spatial resolution 300 km; . ...
... Tem-fast 48 sounding instrument have been initially developed to be employed within the frames of Mars'94 project and should be installed on Mars lander to conduct TEM sounding of Martiansurface. ...
... surface area every four orbits: the Orbiter has 4 revolutions for every 7 Martian ... The descent path distance to the Martiansurface will range from 550 - 250 km ... up of overlapping imaging of the Martiansurface in four gradually increasing areas ...
... has as its primary science objectives to: 1) monitor the daily weather and atmospheric conditions; 2) record changes on the martiansurface due to wind and other atmospheric effects, 3) determine temperature profiles of the atmosphere; and 4) monitor the ...
... Using a 60њ lens an image of a portion of the Martiansurface is a projected onto a vertical CCD-array (1024 pixels); the optical system is placed at the top of the station and is rotated by a step motor (6000 lines). ...
... Trace Gas Orbiter (TGO) to detect and study atmospheric trace gases, such as methane, and water ice distribution in the upper layer of Martiansurface. ...
... elemental composition), gas-analytical suit to study the dynamics of trace components of the Martian atmosphere near the surface, laser spectrometer for atmosphere composition studyies, seismometer, dust suit, soil radiometer, and an instrument to study ...