Based on the success of TEMPEST-D, a nearly identical TEMPEST sensor produced for risk reduction was delivered to the U.S. Space Force and integrated with NASA/JPL’s Compact Ocean Wind Vector Radiometer (COWVR). COWVR and TEMPEST were launched on December 21, 2021, on STP-H8 for 3 years of operations on the ISS. COWVR and TEMPEST have performed coordinated observations of Earth’s oceans and atmosphere from the ISS since January 7, 2022.
Atmospheric inversion techniques have been developed to retrieve water vapor altitude profiles, as well as single-layer cloud liquid water and cloud ice water, from TEMPEST brightness temperatures, using ECMWF Reanalysis v5 (ERA5) data as an initial guess. These retrievals are enhanced through the inclusion of geostationary infrared data from GOES-16 ABI channels, increasing the number of levels and reducing the error of water vapor retrieval, particularly in the upper troposphere.
Previous studies have validated accuracy and precision of TEMPEST brightness temperatures using only clear-sky oceanic observations. Recent studies extend the validation of TEMPEST to include observations over tropical cyclones, using GPM-GMI passive microwave brightness temperatures and GPM-DPR active microwave vertical cumulative reflectivity. Such active/passive microwave observations provide a basis for development of surface rain rate estimates and retrieval of the vertical structure of precipitation from combined TEMPEST and DPR observations.

