Mikhail Yu. Kulikov,1 Mikhail V. Belikovich,1 Alexey G. Chubarov,1,2 Alexander M. Feigin1,2
1Institute of Applied Physics of the Russian Academy of Sciences (Russian Federation) 2Lobachevsky State University of Nizhny Novgorod (Russian Federation)
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The revised model of excited OH with constants corresponding to the published data was applied to retrieve daytime O and H distributions at 77 km–100 km from the data of the SABER/TIMED satellite measurements in 2002–2021. It was found that changes of parameters in the retrieved procedure lead to (1) a noticeable (up to 30%) increase of the O concentration below 85-86 km, (2) a significant (up to 170%) increase of the H concentration below 90 km and a moderate (up to 40%) decrease near 100 km. The influence of revised O and H data on the retrieval of OH and HO2 is also analyzed.
Mikhail Yu. Kulikov,Mikhail V. Belikovich,Alexey G. Chubarov, andAlexander M. Feigin
"Retrieval of daytime O and H distributions at the altitudes of the mesosphere - lower thermosphere from satellite measurement data", Proc. SPIE 12341, 28th International Symposium on Atmospheric and Ocean Optics: Atmospheric Physics, 123417K (7 December 2022); https://doi.org/10.1117/12.2645002
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Mikhail Yu. Kulikov, Mikhail V. Belikovich, Alexey G. Chubarov, Alexander M. Feigin, "Retrieval of daytime O and H distributions at the altitudes of the mesosphere - lower thermosphere from satellite measurement data," Proc. SPIE 12341, 28th International Symposium on Atmospheric and Ocean Optics: Atmospheric Physics, 123417K (7 December 2022); https://doi.org/10.1117/12.2645002