Preprints
https://doi.org/10.5194/egusphere-2024-2165
https://doi.org/10.5194/egusphere-2024-2165
02 Oct 2024
 | 02 Oct 2024
Status: this preprint is open for discussion and under review for Atmospheric Chemistry and Physics (ACP).

Has the 2022 Hunga eruption impacted the noctilucent cloud season in 2023/24 and 2024?

Sandra Wallis, Matthew DeLand, and Christian von Savigny

Abstract. The 2022 Hunga Tonga – Hunga Ha'apai eruption emitted approximately 150 Tg H2O into the middle atmosphere which is still detectable two years after the event. Microwave Limb Sounder (MLS) observations show that the Hunga H2O reached the upper polar mesosphere in the Southern Hemisphere in the beginning of 2024, increasing the H2O mixing ratio in January by about 1 ppmv  between 70° S – 80° S up to an altitude of 83 km. No clear signal was detected for the noctilucent cloud occurrence frequency inferred from Ozone Mapping and Profiling Suite – Limb Profiler (OMPS-LP) measurements. It cannot, however, be ruled out that a slight increase from mid-January to February is potentially caused by the additional water vapour from the Hunga event. Several months later, the water vapour anomaly reached the polar summer mesopause region in the NH during the 2024 NLC season. However, a subsequent anomalous warming during the second half of the season might have hindered the ice particle formation, leading to a decrease in occurrence frequency of the mesospheric clouds compared to previous years. To summarise, the volcanic water vapour seems to need two years to reach the summer polar mesopause region. This resembles the Krakatau case that is argued to have caused the first sightings of noctilucent clouds two years after its eruption in 1883.       

Publisher's note: Copernicus Publications remains neutral with regard to jurisdictional claims made in the text, published maps, institutional affiliations, or any other geographical representation in this preprint. The responsibility to include appropriate place names lies with the authors.
Sandra Wallis, Matthew DeLand, and Christian von Savigny

Status: open (until 13 Nov 2024)

Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor | : Report abuse
Sandra Wallis, Matthew DeLand, and Christian von Savigny
Sandra Wallis, Matthew DeLand, and Christian von Savigny

Viewed

Total article views: 57 (including HTML, PDF, and XML)
HTML PDF XML Total Supplement BibTeX EndNote
49 4 4 57 5 1 2
  • HTML: 49
  • PDF: 4
  • XML: 4
  • Total: 57
  • Supplement: 5
  • BibTeX: 1
  • EndNote: 2
Views and downloads (calculated since 02 Oct 2024)
Cumulative views and downloads (calculated since 02 Oct 2024)

Viewed (geographical distribution)

Total article views: 57 (including HTML, PDF, and XML) Thereof 57 with geography defined and 0 with unknown origin.
Country # Views %
  • 1
1
 
 
 
 
Latest update: 05 Oct 2024
Download
Short summary
The 2022 Hunga eruption emitted about 150 Tg H2O that partly reached the upper polar SH mesosphere in the beginning of 2024. Noctilucent clouds (NLC) did not show a clear perturbation in their occurrence frequency, but the slight increase from mid-January to February could potentially be caused by the additional H2O. It needs 2 years to reach the summer polar mesopause region, analogous to the 1883 Krakatau eruption that is argued to have caused the first sightings of NCLs.