The extremely large telescopes that should see first light in coming years demand so-called adaptive optics systems to overcome the devastating effect of the atmospheric turbulence on the image quality. A sensor measures the incoming distortion of the light and is used for reshaping the latter using a deformable mirror. Processing the large number of sensor channels to operate the actuators at kilohertz frequencies is challenging on the computational point of view. The correction applied by the mirror and based on the sensor measurements should indeed not be already outdated because the turbulence has evolved during the computation time. In order to reduce the memory storage and the computational requirements, prior knowledge on the system ...
Nowadays, the adaptive optics (AO) system is of fundamental importance to improve the real resolutio...
AbstractThe wave front field aberrations induced by atmospheric turbulence can severely degrade the ...
We present a method to reduce the noise in the interaction matrix by calibration of the adaptive opt...
The extremely large telescopes that should see first light in coming years demand so-called adaptive...
International audiencehe linear quadratic Gaussian regulator provides the minimum-variance control s...
The visualization of objects within or beyond a turbulent medium is hampered by the aberrations the ...
Adaptive Optics (AO) play an essential role in the field of astronomical seeing for ground-based tel...
Nowadays, the adaptive optics (AO) system is of fundamental importance to reduce the effect of atmos...
Telescope resolution is theoretically limited by the diffraction effect, and hence it is inversely p...
AbstractWe derive efficient approaches for two-parameter Hankel transforms. Such transforms arise, f...
AbstractRecently there has been growing interest and progress in using numerical linear algebra tech...
Future large optical telescopes require adaptive optics (AO) systems whose deformable mirrors (DM) h...
After a brief presentation of atmospheric turbulence and its effects on image degradation, followed ...
Current and next generation of telescopes resort to adaptive optics in order to compensate for atmos...
Abstract. Observations with ground based telescopes suffer from atmospheric turbulence. Inde-pendent...
Nowadays, the adaptive optics (AO) system is of fundamental importance to improve the real resolutio...
AbstractThe wave front field aberrations induced by atmospheric turbulence can severely degrade the ...
We present a method to reduce the noise in the interaction matrix by calibration of the adaptive opt...
The extremely large telescopes that should see first light in coming years demand so-called adaptive...
International audiencehe linear quadratic Gaussian regulator provides the minimum-variance control s...
The visualization of objects within or beyond a turbulent medium is hampered by the aberrations the ...
Adaptive Optics (AO) play an essential role in the field of astronomical seeing for ground-based tel...
Nowadays, the adaptive optics (AO) system is of fundamental importance to reduce the effect of atmos...
Telescope resolution is theoretically limited by the diffraction effect, and hence it is inversely p...
AbstractWe derive efficient approaches for two-parameter Hankel transforms. Such transforms arise, f...
AbstractRecently there has been growing interest and progress in using numerical linear algebra tech...
Future large optical telescopes require adaptive optics (AO) systems whose deformable mirrors (DM) h...
After a brief presentation of atmospheric turbulence and its effects on image degradation, followed ...
Current and next generation of telescopes resort to adaptive optics in order to compensate for atmos...
Abstract. Observations with ground based telescopes suffer from atmospheric turbulence. Inde-pendent...
Nowadays, the adaptive optics (AO) system is of fundamental importance to improve the real resolutio...
AbstractThe wave front field aberrations induced by atmospheric turbulence can severely degrade the ...
We present a method to reduce the noise in the interaction matrix by calibration of the adaptive opt...