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ACTIVITIES
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Activity - Projects
Dragon 2 Cooperation Programme
The Dragon 2 Programme focussed on the exploitation of ESA, ESA's Third Party Missions and Chinese Earth observation data for science and applications development in land, ocean and atmospheric applications.
Activity - Projects
TOLEOS
The TOLEOS (Thermosphere Observations from Low-Earth Orbiting Satellites) project will produce thermosphere mass density observations from the accelerometer measurements of the GRACE, GRACE-FO, and CHAMP satellites.
Activity - General activities
GSCB and LTDP
The Copernicus programme is based on a fleet of European Earth observation satellites, built and operated by ESA, member states and commercial entities. Copernicus will also offer data from non-European satellites.
Activity - Instrument characterisation and algorithm studies
ESA satellites and instruments calibration landing page
ESA satellites and instruments calibration landing page.
Activity - Fiducial Reference Measurements
FRM4VEG: Fiducial Reference Measurements for Vegetation
Fiducial Reference Measurements for Vegetation (FRM4VEG) is an ESA managed project focused on establishing the protocols required for traceable in-situ measurements of vegetation
Activity - Instrument characterisation and algorithm studies
PV-LAC-ATMO
The objective of PV-LAC-ATMO Activity is to investigate the added value of a joint surface reflectance.
Activity - Instrument characterisation and algorithm studies
PV-CDRR
The objective of the Proba-V Cloud Detection Round Robin (PV-CDRR) is to learn advantages and drawbacks of the different approaches for various cloud and surface conditions.
Activity - Instrument characterisation and algorithm studies
PV-LAC-COAST
The PV-LAC project objectives are to develop, test, and validate two advanced algorithms for the scientific exploitation of the Proba-V mission products.
Activity - Projects
Auroral Electrojet and auroral Boundaries estimated from Swarm observations
In the Swarm-AEBS project, a set of new Swarm data products that characterise the auroral electrojets and auroral oval boundaries will be derived from Swarm magnetic field measurements.