A potential solution to improving remotely sensed soundings of the PBL is to combine space-based sounders with a network of ground-based sensors. This has previously been shown to provide significant improvements in information content, vertical resolution, and reductions in retrieval uncertainty in the lowest 1000 m above ground level compared to space-based sounding alone. A critical component of planning a new satellite mission are the sensor design decisions; with IR sounders, identifying the critical spectral band coverage is one of the major decisions. This presentation will assess information content of the thermodynamic profile across the lowest 2000 m above ground level across various spectral bands in the thermal IR from both space-based and ground-based perspectives in order to inform IR sensor design for future observing missions. Initial results suggest that the majority of information about the PBL, from a space-based perspective, is in the atmospheric window around 12.5 um. These results will be compared to the typical Cross-track Infrared Sounder (CrIS) and Infrared Atmospheric Sounding Interferometer (IASI) channel selections for NWP data assimilation to identify the key spectral regions where additional near-surface information may be gained from space-based IR sounders. Furthermore, the priority of spectral channels from a synergy of space-based and ground-based IR sensors will be shown.
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