“…These two emissions are the dominant mechanisms of thermospheric radiative cooling below 250 km. The NO concentration is highly variable, and its abundance has been the object of observational efforts and modeling studies for many years (e.g., Barth, 1992;Barth et al, 2003;Dobbin & Aylward, 2008;Maeda et al, 1992;Siskind, Barth, Evans, & Roble, 1989;Wang et al, 2024). There is now also substantial interest in CO 2 as its abundance is increasing in the thermosphere with the effect of imposing a long-term cooling trend (Qian et al, 2021;Roble & Dickinson, 1989) with potential implications for space operations and the space economy (Brown et al, 2021;Mlynczak, Yue, et al, 2021).…”