The eruption of the Hunga Tonga–Hunga Ha’apai (HTHH) volcano on 15 January 2022 injected large amounts of water vapor (H
2O) directly into the stratosphere. While normal background levels of stratospheric H
2O are not detectable in radio occultation (RO) measurements,
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The eruption of the Hunga Tonga–Hunga Ha’apai (HTHH) volcano on 15 January 2022 injected large amounts of water vapor (H
2O) directly into the stratosphere. While normal background levels of stratospheric H
2O are not detectable in radio occultation (RO) measurements, effects of the HTHH eruption are clearly observed as anomalous refractivity profiles from COSMIC-2, suggesting the possibility of detecting the HTHH H
2O signal. To separate temperature and H
2O effects on refractivity, we use co-located temperature observations from the Microwave Limb Sounder (MLS) to constrain a simplified H
2O retrieval. Our results show enhancements of H
2O up to ~2500–3500 ppmv in the stratosphere (~29–33 km) in the days following the HTHH eruption, with propagating patterns that follow the dispersing volcanic plume. The stratospheric H
2O profiles derived from RO are in reasonable agreement with limited radiosonde observations over Australia. The H
2O profiles during the first few days after the eruption show descent of the plume at a rate of ~−1 km/day, likely due to strong radiative cooling (~−10 K/day) induced by high H
2O concentrations; slower descent (~−200 m/day) is observed over the following week as the plume disperses. The total mass of H
2O injected by HTHH is estimated as 110 ± 14 Tg from measurements in the early plumes during 16–18 January, which equates to approximately 8% of the background global mass of stratospheric H
2O. These RO measurements provide novel quantification of the unprecedented H
2O amounts and the plume evolution during the first week after the HTHH eruption.
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