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Mars submillimeter sensor on microsatellite: sensor feasibility study

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Figure

Figure 1. Sketch of sensor electronics design. The radio frequency(RF) between 474.65–475.65 and 486.65–487.65 GHz enters fromthe left in the figure and is split by a circular polarizer (CP) intoleft-handed, and right-handed, circular polarization (LHCP, RH
Figure 2. Temperature and volume mixing ratio profiles used in the simulations.
Figure 4. Simulated signal for the sensor. The signal unit is in Planck-equivalent brightness temperature as expected with the sensor calibrated(used in later figures)
Figure 5. Forward model parameter error estimations for the atmosphere of Fig. 2 in limb-scanning mode with 1 s integration time at each ofthe tangent altitudes of Fig
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