Earth Observation satellites
using passive diffraction limited techniques of solar system planets and adaptive optics R&D.
at BsC, MsC and PhD levels and European networking in astronomy and geosciences.
geostationnary and low orbit satellites.
for the long term (since 35 years) solar variability follow-up and simultaneous atmospheric turbulence monitoring applicable to space-weathering programs.
with versatile focal instruments with and field photopoalrimetric CCD imging, EMCCD 1kx1k diffraction limited imaging, a prototype of large-field adaptive optics for high contrast imaging in the IR (up to the H 1.6µ band).
for lunar and satellite laser-ranging (fast tracking mount), with secondary instrumentations : e.g. adaptive optics for imaging in the visible of low orbit satellites and space-debris survey programs in addition to time-frequency ground-space synchronization.
integrated in the global network of the RESIF broadband sismometry.
for remote observations of transcient events (astronomical gamma bursts, space debris, NEO asteroids, etc..).