EGU2020-19643, updated on 10 Jan 2024
https://doi.org/10.5194/egusphere-egu2020-19643
EGU General Assembly 2020
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

The TANGO mission: A satellite tandem to measure major sources of anthropogenic greenhouse gas emissions

Jochen Landgraf1, Stephanie Rusli1, Ryan Cooney1, Pepijn Veefkind2, Tim Vemmix2, Zeger de Groot3, Andrew Bell4, James Day4, Anton Leemhuis4, and Bernd Sierk5
Jochen Landgraf et al.
  • 1SRON Netherlands Institute for Space Research, Utrecht, The Netherlands
  • 2KNMI Royal Netherlands Meteorological Institute, De Bilt, The Netherlands
  • 3ISIS Innovative Solutions in Space, Delft, The Netherlands
  • 4TNO Netherlands Organisation for Applied Scientific Research, The Netherlands
  • 5ESA-ESTEC, Noordwijk, The Netherlands

In this contribution, we present the Twin ANthropogenic Greenhouse Gas Observers (TANGO) mission, which is one of four candidate missions of ESA’s SCOUT program for the rapid prototyping and demonstration of observation techniques and science application using small-satellites. Over the period 2024-2027, TANGO will provide the unique opportunity for the global and independent monitoring of the major emission sources of the anthropogenic greenhouse gases CH4 and CO2. It will demonstrate a distributed monitoring system that can pave the way for future larger constellations of small-satellites allowing for enhanced coverage and temporal resolution. The TANGO mission consists of two agile small-satellites, each carrying one spectrometer flying in conjunction with the Copernicus Sentinel 5 mission. Regular joint TANGO and Sentinel 5 observations will be used to enhance the radiometric accuracy of the TANGO spectrometers. The first satellite measures spectral radiances in the shortwave infrared part of the solar spectrum (1.6 µm) to determine moderate to strong emissions of CH4 (≥ 10 Kt/yr) and CO2 (≥ 5 Mt/yr). The instrument has a field of view of 30 x 30 kmat spatial resolutions small enough to monitor individual large industrial facilities (300 x 300 m2), with an accuracy to determine emissions on the basis of a single observation. Using the same strategy, the second satellite yields collocated NO2 observations from radiance measurements in the visible spectral range, supporting plume detection and exploiting the use of CO2/NO2 ratio observations to estimate CO2 emissions from offshore NO2 sources. TANGO will provide surface fluxes of specific emission types based on the combination of CH4, CO2 and NO2 observations at a high spatial resolution. In doing so, TANGO aims to uniquely complement the large current and planned Copernicus monitoring missions like Sentinel-5(P) and the CO2M High Priority Candidate Mission (HPCM) by providing unrivalled high-resolution monitoring of the major anthropogenic greenhouse gas emissions at a regular basis.

How to cite: Landgraf, J., Rusli, S., Cooney, R., Veefkind, P., Vemmix, T., de Groot, Z., Bell, A., Day, J., Leemhuis, A., and Sierk, B.: The TANGO mission: A satellite tandem to measure major sources of anthropogenic greenhouse gas emissions, EGU General Assembly 2020, Online, 4–8 May 2020, EGU2020-19643, https://doi.org/10.5194/egusphere-egu2020-19643, 2020.