EGU22-6159
https://doi.org/10.5194/egusphere-egu22-6159
EGU General Assembly 2022
© Author(s) 2023. This work is distributed under
the Creative Commons Attribution 4.0 License.

Quantification of SO2 emission rates from the Kilauea volcano in Hawaii by the divergence of the SO2 flux using S5P-TROPOMI satellite measurements and comparison to results from ground-based observations

Adrian Jost1, Steffen Beirle1, Steffen Dörner1, Christian Borger1, Simon Warnach1, Nicole Bobrowski2,3, Christoph Kern4, and Thomas Wagner1
Adrian Jost et al.
  • 1Max Planck Institute for Chemistry, Satellite Remote Sensing, Mainz, Germany (adrian.jost@mpic.de)
  • 2Institute of Environmental Physics, University of Heidelberg, Heidelberg, Germany
  • 3Istituto Nazionale Geofisica e Vulcanologia Catania, Italy
  • 4U.S. Geological Survey Cascades Volcano Observatory, Vancouver, WA 98683, USA

With a nearly continuously effusive eruption since 1983, the Kilauea volcano (Hawaii, USA) is one of the most active volcanoes in the world. From the beginning of May till the end of August 2018, a sequence of eruptions on the Lower East Rift Zone (LERZ) caused an enhanced outbreak of volcanic gases and aerosols, releasing them into the troposphere. Since these gases and particles affect climate, environment, traffic, and health on regional to global scales, a continuous monitoring of the emission rates is essential.

As satellites provide the opportunity to observe and quantify the emissions remotely from space, their contribution to the monitoring of volcanoes is significant. The TROPOspheric Monitoring Instrument (TROPOMI) onboard the Sentinel-5 Precursor satellite was successfully launched by the end of 2017 and provides measurements with unprecedented level of detail at a resolution of 3.5 x 7.0 km2 (3.5 x 5.5 km2 since August 2019). This also allows for an accurate retrieval of trace gas species such as volcanic SO2.  

Here, we show that the location and strength of SO2 emissions from Kilauea can be determined by the divergence of the temporal mean SO2 flux. This approach, which is based on the continuity equation, has been successfully demonstrated for NOX emissions of individual power plants (Beirle et al., Sci. Adv., 2019).

The present state of our work also indicates that emission maps of SO2 can be derived by the combination of satellite measurements and wind fields on high spatial resolution. As the divergence is highly sensitive on point sources like the erupting fissures in the 2018 Kilauea eruption, they can be localized very precisely. The obtained emission rates of about 1.5 Mt are substantially lower than the ones reported from ground-based measurements in other studies like the one from Kern et al. (Bull. Volcanol., 2020). 

We discuss several potential reasons for the discrepancies between the ground- and satellite-based observations like e.g. uncertainties of the air mass factor or possible rapid destruction of SO2 in the presence of clouds.

How to cite: Jost, A., Beirle, S., Dörner, S., Borger, C., Warnach, S., Bobrowski, N., Kern, C., and Wagner, T.: Quantification of SO2 emission rates from the Kilauea volcano in Hawaii by the divergence of the SO2 flux using S5P-TROPOMI satellite measurements and comparison to results from ground-based observations, EGU General Assembly 2022, Vienna, Austria, 23–27 May 2022, EGU22-6159, https://doi.org/10.5194/egusphere-egu22-6159, 2022.

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