Abstract
Atomic hydrogen (H) is crucial for understanding photochemistry and the energy budget in the mesopause region. However, there is still no consensus on the H abundance in this region. This study presents a new hydrogen data set derived from Scanning Imaging Absorption Spectrometer for Atmospheric Chartography (SCIAMACHY) OH(9–6) band spectra, collocated with temperature and ozone profiles from other remote sensing instruments. H number densities peak at 82–87 km and range from (Formula presented.) to (Formula presented.) (Formula presented.), depending on season and latitude. Two other H data sets obtained from the Sounding of the Atmosphere using Broadband Emission Radiometry (SABER) are presented for comparison: those from Mlynczak et al. (2018, https://doi.org/10.1029/2018GL077377) and Panka et al. (2021, https://doi.org/10.1029/2020GL091053) are approximately 30% lower and 50% higher than the SCIAMACHY data at peak altitudes, respectively. Additionally, the H number density retrieved in this study partly shows better agreement with the only direct rocket in situ measurements than those from SABER.
| Original language | English |
|---|---|
| Article number | e2025GL116311 |
| Journal | Geophysical Research Letters |
| Volume | 52 |
| Issue number | 15 |
| DOIs | |
| State | Published - Aug 16 2025 |
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