Space Missions

High-Resolution Thermal Missions

The GCU actively contributes to three next-generation satellite missions that will provide unprecedented thermal Earth observation at ~50 m resolution and 2-day revisit.

ESA · Copernicus Programme

LSTM

Land Surface Temperature Monitoring

LSTM is the next Copernicus Sentinel-10 mission developed by ESA and the European Commission. It will provide systematic, global observations of land surface temperature at high spatial and temporal resolution, addressing a critical observational gap in our rapidly warming climate.

Prof. José Antonio Sobrino is a member of the ESA Mission Advisory Group (MAG) for the LSTM mission. ESA has recognized the GCU's essential contribution to preparing unprecedented global thermal Earth observation capabilities.

Spatial Resolution
~50 m
Revisit Time
2 days
Spectral Bands
TIRS (TIR)
GCU Role
MAG member / Algorithm dev.
LSTM

GCU Contributions

  • LST and LSE algorithm development for TIRS sensor
  • Participation in ESA Mission Advisory Group
  • Calibration/validation campaigns (Italy, France, Spain, USA)
  • In-situ data from 6 permanent stations
  • Product validation against Landsat 9 and ECOSTRESS
  • Algorithm ATBD (Algorithm Theoretical Basis Document)
TRISHNA

GCU Contributions

  • Member of the TRISHNA Scientific Committee
  • LST retrieval algorithm development
  • Participation in French-organized field campaigns
  • Two annual trips to CNES headquarters in Toulouse
  • Collaboration with CESBIO, ONERA, University of Strasbourg
CNES · ISRO · Franco-Indian Mission

TRISHNA

Thermal infraRed Imaging Satellite for High-resolution Natural resource Assessment

TRISHNA is a joint mission between CNES (France) and ISRO (India) aimed at monitoring the land surface energy budget and evapotranspiration at high resolution. Prof. Sobrino is a member of the TRISHNA Scientific Committee.

Spatial Resolution
57 m
Agencies
CNES / ISRO
Primary Focus
Energy budget / ET
GCU Role
Scientific Committee
NASA · ASI · Earth System Explorer

SBG

Surface Biology and Geology

The Surface Biology and Geology (SBG) mission from NASA and ASI will provide global hyperspectral and thermal infrared imagery. It fills a critical gap in Earth observation by combining surface mineralogy, vegetation biochemistry, and thermal data into a unified platform.

Spatial Resolution
~60 m
Agencies
NASA / ASI
Spectral Range
VSWIR + TIR
GCU Role
Algorithm development
SBG

GCU Contributions

  • LST algorithm development for TIR instrument
  • Collaboration with NASA Jet Propulsion Laboratory
  • Joint field campaigns in USA and Europe
  • Cross-validation with LSTM and TRISHNA products
  • Participation in SBG scientific workshops