Changes in upper stratosphere and lower mesosphere temperatures are early indicators of overall climate-driven processes. For example, increasing CO 2 is expected to produce cooling in these regions (Roble & Dickinson, 1989), and such cooling has already been observed by a number of instruments. Recently, Zhao et al. (2020) detected a cooling trend of ∼0 to −0.14 K/decade at all latitudes using the annual mean temperatures from Sounding of the Atmosphere Using Broadband Emission Radiometry (SABER) instrument from 2002 to 2019. Li et al. (2020) used merged Halogen Occultation Experiment (HALOE) and SABER observations between 1991 and 2018 to investigate cooling trends between 40 and 80 km altitude with a maximum value of ∼1.2 K/decade. In the summer polar mesosphere, Bailey et al. ( 2021) identified a cooling trend of 1-2 K/decade using Solar Occultation for Ice Experiment (SOFIE) measurements. Such cooling trends will likely increase the abundance of Polar Mesospheric Clouds (PMCs). All of these satellite-based temperature trends are inferred from data produced by systems that have functioned well past their expected lifetimes and/or require merging of data sets generated using different techniques. With the Suomi National Polar-orbiting Partnership/Joint Polar Satellite System (SNPP/ JPSS) systems, which are expected to operate into the 2030s, we have the opportunity to generate a temperature record from a series of Ozone Mapping and Profiler Suite (OMPS) Limb Profiler (LP) (OMPS-LP) instruments that spans decades. This paper describes our technique for producing temperature profiles between 35 and 70 km from Rayleigh scattered radiance fields.Upper atmospheric temperatures have been measured using a variety of techniques including in situ measurements from occasional very high altitude balloons, GNSS radio occultation, satellite microwave, IR measurements, and ground based lidar. One of the first satellite global temperature and density measurements in the 40-92 km altitude range was derived from the Solar Mesosphere Explorer (SME) limb radiance profiles at 304, 313, and 442 nm (Clancy et al., 1994). Shepherd et al. (2001) retrieved temperature from 65 to 90 km using radiance data at 553 nm from the Wind Imaging Interferometer (WINDII) instrument. Sheese et al. (2012) retrieved temperature profiles using Optical Spectrograph and InfraRed Imaging System (OSIRIS) bright limb observations at 318.5 and 347.5 nm in the altitude range 45-85 km, and Hauchecorne et al. ( 2019) created temperature and density profiles from 35 to 85 km using limb radiances in the spectral band 420-480 nm from the Global Ozone Monitoring by Occultation of Stars (GOMOS) instrument on ENVISAT. Among the currently operating instruments, Microwave Limb Sounder (MLS) and SABER temperatures are the primary source of stratospheric