The seasonal cycle of atmospheric CO2 in South America over the last ten years seen by GOSAT
- 1Institute of Environmental Physics, Heidelberg University, Heidelberg, Germany
- 2NASA Goddard Space Flight Center, Greenbelt, Maryland, USA
- 3Earth System Science Interdisciplinary Center, University of Maryland, College Park, Maryland, USA
The number of in-situ CO2 measurements in the Southern Hemisphere is very limited. This leads to large
uncertainties in estimates of regional carbon fluxes by in-situ based inverse models. Satellite-based CO2
measurements, on the other hand, are available in the Southern Hemisphere with a dense spatial
coverage. By evaluating these, the regional carbon cycle can be studied in more detail and the results of
carbon cycle models can be validated against the satellite data.
Here, we present a comparison of atmospheric CO2 data provided by the Greenhouse gases Observing
SATellite (GOSAT) and in-situ based inverse models for South America from 2009 to 2019. The seasonal
cycle of atmospheric CO2 concentrations measured by the GOSAT satellite shows differences in both,
amplitude and timing, compared to in-situ based atmospheric inversions. To determine the reason for
these discrepancies, we use the TM5-4DVar atmospheric inversion model assimilating GOSAT satellite
data to obtain GOSAT based land-surface fluxes. This allows us to identify sub-regions responsible for the
differences. In order to gain a deeper understanding of the underlying processes, we also analyse various
climate parameters, fire emission data, and vegetation proxies (for example Solar Induced Fluorescence,
SIF). By doing so, we aim at improving our understanding of the mechanisms that influence the seasonal
carbon cycle in South America.
How to cite: Artelt, L., Metz, E.-M., Vardag, S., Basu, S., and Butz, A.: The seasonal cycle of atmospheric CO2 in South America over the last ten years seen by GOSAT, EGU General Assembly 2023, Vienna, Austria, 24–28 Apr 2023, EGU23-6152, https://doi.org/10.5194/egusphere-egu23-6152, 2023.