Satellite-measured SO2 mass loadings and ground-based measurements of SO2 emission rate
are not directly comparable, with ∼40% differences between mean emissions reported by each technique
from Tungurahua volcano, Ecuador, during late 2007. Numerical simulations of postemission processing and
dispersal of Tungurahua’s SO2 emissions enable more effective comparison of ground- and satellite-based
SO2 data sets, reducing the difference between them and constraining the impact of plume processing on
satellite SO2 observations. Ground-based measurements of SO2 emission rate are used as the model input,
and simulated SO2 mass loadings are compared to those measured by the Ozone Monitoring Instrument
(OMI). The changing extent of SO2 processing has a significant impact on daily variation in SO2 mass loading
for a fixed volcanic emission rate. However, variations in emission rate at Tungurahua are large, suggesting
that overall volcanic source strength and not subsequent processing is more likely to be the dominant
control on atmospheric mass loading. SO2 emission rate estimates are derived directly from the OMI
observations using modeled SO2 lifetime. Good agreement is achieved between both observed and
simulated mass loadings (∼21%) and satellite-derived and ground-measured SO2 emission rates (∼18%),
with a factor of 2 improvement over the differences found by simple direct comparison. While the balance
of emission source strength and postemission processing will differ between volcanoes and regions, under
good observation conditions and where SO2 lifetime is ∼24 hours, satellite-based sensors like OMI may
provide daily observations of SO2 mass loading which are a good proxy for volcanic source strength.B.T.M. acknowledges funding from the
National Centre for Earth Observation,
part of the UK’s Natural Environment
Research Council, and latterly the
Deep Carbon Observatory and
the Smithsonian Institution. B.T.M.,
M.E., and T.A.M. are supported by
and contribute to the NERC NCEO
Dynamic Earth and Geohazards group.
S.A.C. acknowledges funding from
NASA through grants NNX09AJ40G
(Aura Validation), NNX10AG60G
(Atmospheric Chemistry Modeling and
Analysis Program), and NNX11AF42G
(Aura Science Team). J.Y. was funded
by the Isaac Newton Trust at the
University of Cambridge for the
duration of this project. The authors
thank Anja Schmidt and two anonymous
reviewers for their thorough
and constructive comments. We
acknowledge the Goddard Earth
Sciences Data and Information
Services Center for making OMI SO2
data publicly available.This is the final published version. It first appeared at http://onlinelibrary.wiley.com/doi/10.1002/2013JD019771/abstract