Exploring the impact of sea surface temperature and salinity on SMAP excess surface emissivity

The Soil Moisture Active Passive instrument (SMAP) has been used to infer sea surface wind speed from its brightness temperature measurements. To do so, the SMAP wind speed retrieval process requires the removal of sea surface temperature (sst) and salinity (sss) impact to brightness temperature. Estimating the so-called excess surface emissivity (Δ e ), that is the sst normalized difference between measured brightness temperature of the sea surface and the corresponding brightness temperature of a flat surface, is one way of accomplishing such a task. In this paper, we investigate whether SMAP Δ e contains residual dependencies to sst and sss. To do so, v5.0 SMAP brightness temperature measurements, derived by the Jet Propulsion Laboratory, are used. For any fixed numerical weather prediction model wind speed above 15 m/s, down to a 20 % decrease in SMAP Δ e is observed as the sst increases from 274 to 304 K. For any fixed wind speed between 8 and 15 m/s, the sst residual dependence is weaker with SMAP Δ e exhibiting a 1-2 % decrease as the sst increases. Below 8 m/s, this pattern becomes prevalent again, when the significant waveheight (Hs) is greater than 3.5 m. SMAP Δ e decreases as much as 50 % with increasing sss, most notably below 8 and above 15 m/s when Hs is considered. This analysis has also shown that below 8 m/s and for swell dominant seas, a decrease in either sss or sst results in a decrease in SMAP Δ e sensitivity to wind induced sea surface roughness.