“…The 950-1150 cm −1 spectral region includes high-density absorption features of the ozone υ3 band (the strongest fundamental band) and minor absorption from interfering species. The υ3 band has been exploited in the tropospheric O 3 soundings by a suite of TIR satellite-borne, nadir-viewing instruments, including AIRS (Susskind et al, 2003(Susskind et al, , 2014Wei et al, 2010), Cross-track Infrared Sounder (CrIS) (Gambacorta et al, 2013), and IASI (Boynard et al, 2009(Boynard et al, , 2016Dufour et al, 2012;Oetjen et al, 2014Oetjen et al, , 2016, as well as the solar occultation satellite-borne (Bernath et al, 2005;Bernath, 2017), balloon-borne (Toon, 1991;Fu et al, 2007a), and ground-based (Hannigan et al, 2011) FTSs that quantify the stratospheric ozone layer and the species playing an essential role in the stratospheric ozone chemistry (Fu et al, 2007b(Fu et al, , 2009(Fu et al, , 2011Sung et al, 2007;Wunch et al, 2007;Allen, 2009;Boone, 2013;Nassar, 2013;Griffin et al, 2017). The spectral resolution of TES (resolving power (RP): 10 500) is significantly higher than the existing TIR, including AIRS (RP: 1200), CrIS (RP: 816), and IASI (RP: 5250).…”