EGU24-5350, updated on 08 Mar 2024
https://doi.org/10.5194/egusphere-egu24-5350
EGU General Assembly 2024
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

Using a portable EM27/SUN FTIR-spectrometer for validating the TCCON site-to-site consistency: The COCCON Travel Standard

Benedikt Herkommer1, Frank Hase1, Jochen Groß1, Carlos Alberti1, Paolo Castracane2, Angelika Dehn2, Jia Chen5, Florian Dietrich5, Isamu Morino3, Matthias Max Frey3, Lawson Gillespie4, Nasrin Mostafavi Pak4,8, Debra Wunch4, Nicholas Deutscher6, Brittany Walker6, and Omaira Elena García7
Benedikt Herkommer et al.
  • 1KIT, IMK, ASF, Germany (benedikt.herkommer@kit.edu)
  • 2European Space Agency/Centre for Earth Observation (ESA/ESRIN), Frascati, Italy
  • 3National Institute for Environmental Studies (NIES), Tsukuba, Japan
  • 4Department of Physics, University of Toronto, Toronto, Canada
  • 5Environmental Sensing and Modeling, Department of Electrical and Computer Engineering, Technische Universität München, Munich, Germany
  • 6Centre for Atmospheric Chemistry, School of Earth, Atmospheric and Life Sciences, University of Wollongong, Wollongong, NSW, 2522, Australia
  • 7Izaña Atmospheric Research Centre (IARC), Agencia Estatal de Meteorología (AEMET), Santa Cruz de Tenerife, Spain
  • 8Now at: Institute of Meteorology and Climate Research Atmospheric Environmental Research (IMK-IFU), Karlsruhe Instute of Technology (KIT), Garmisch-Partenkirchen, Germany

The precise knowledge of the global atmospheric concentrations of green-house gases (GHG) are crucial for understanding and monitoring climate change.
Satellites for measuring GHGs are offering a global coverage, however, they need precise ground-based reference data for validation.
This reference data is provided by ground-based measurements, foremost the Total Column Carbon Observing Network (TCCON).
The TCCON measures column averages of GHG abundances at about 25 stations around the globe using Fourier Transform Infrared (FTIR) spectrometer.

For achieving the high data quality needed for the validation of current and upcoming GHG measuring satellite missions the control of site-by-site biases across the network is of utmost importance. So far, the verification of the individual TCCON sites mainly depends on the collection of collocated in situ measurements of GHG profiles, using airplane overflights or balloon air-core measurements, the use of calibrated HCl gas cells and on the evaluation of XAIR.
 
In this work we present a new supplemental approach by using the portable EM27/SUN FTIR spectrometer, which is the standard instrument of the Collaborative Carbon Column Observing Network (COCCON). This instrument type has proven its high stability in various field campaigns and long-term studies. In the framework of the ESA project “Fiducial Reference Measurements for Green-House Gases II” we are exploiting the stability of the instrument to use it as a Travel Standard (TS) for the TCCON. We visited sites in Japan, Canada, Germany, Australia, France and the Canary Islands to perform side-by-side measurements with the local TCCON spectrometers. Between the visits, the stability of the TS was monitored using the Karlsruhe TCCON site and the COCCON reference spectrometer.
This allows to compare the different TCCON sites to a common reference and hence, to verify the level of station-to-station consistency currently achieved by the TCCON and support further improvements. Here, we present the results of the TS visit at the TCCON site Tsukuba(Japan), Wollongong(Australia) and Izana(Canary Islands).

How to cite: Herkommer, B., Hase, F., Groß, J., Alberti, C., Castracane, P., Dehn, A., Chen, J., Dietrich, F., Morino, I., Frey, M. M., Gillespie, L., Pak, N. M., Wunch, D., Deutscher, N., Walker, B., and García, O. E.: Using a portable EM27/SUN FTIR-spectrometer for validating the TCCON site-to-site consistency: The COCCON Travel Standard, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-5350, https://doi.org/10.5194/egusphere-egu24-5350, 2024.