https://egusphere.copernicus.org/preprints/2026/egusphere-2025-5446/

*Authors: *Anna Lange, Ulrike Niemeier, Alexei Rozanov, and Christian von
Savigny

*11 January 2026*

*Abstract*
Stratospheric aerosol injections have been proposed to mitigate the effects
of global warming. The injection of sulphur dioxide into the stratosphere
is one possible idea. However, depending on the latitude, high emission
rates can lead to very low transmissions from the perspective of a typical
satellite solar occultation instrument, leading to the so-called zero
transmission problem. Consequently, it is highly unlikely that a physically
meaningful retrieval of the stratospheric aerosol extinction profiles is
possible, depending on the latitude and wavelength. The current study
analyses, using MAECHAM5-HAM and SCIATRAN, continuous injections of 30 Tg
S/y as a hypothetical large-scale stratospheric aerosol injection scenario.
For this purpose, sulphur dioxide was continuously injected at an altitude
of 60 hPa (about 19 km) into one grid box (2.8°x 2.8°) centred on the
Equator at 121°E. Specifically, it is investigated which wavelengths,
depending on the latitude, are necessary for plausible aerosol extinction
profile retrievals. While a wavelength of 520 nm is insufficient for the
retrieval for 5°N, the opposite can be concluded for 75°N and 75°S. For the
latitudes 45°N and 45°S, a wavelength of at least 1543 nm is necessary. In
contrast, 1900 nm is sufficient for 15°N and 15°S, as well as 5°N.
Simulation results for an emission rate of 10 Tg S/y show that a minimum
wavelength of 1543 nm is already sufficient for 5°N. The results emphasize
that the zero transmission problem does not mean that solar occultation
measurements are entirely useless. Consistent with expectations, a longer
wavelength is required for the latitude range of and near the injection.
These findings are therefore also relevant for satellite solar occultation
measurements after major volcanic eruptions.

*Source: EGUSphere*

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