With a view to the next generation of large space telescopes, we investigate guide-starfree, image-based aberration correction using a unimorph deformable mirror in a plane conjugate to the primary mirror.We designed and built a high-resolution imaging testbed to evaluate control algorithms. In this paper we use an algorithm based on the heuristic hill climbing technique and compare the correction in three different domains, namely the voltage domain, the domain of the Zernike modes, and the domain of the singular modes of the deformable mirror. Through our systematic experimental study, we found that successive control in two domains effectively counteracts uncompensated hysteresis of the deformable mirror.Team Raf Van de Pla
A deformable mirror (DM) is an important component of an adaptive optics system. It is known that an...
Concepts for future large space telescopes require an active optics system to mitigate aberrations c...
The wave front corrector is one of the three key elements in adaptive optics, along with the wave fr...
With a view to the next generation of large space telescopes, we investigate guide-starfree, image-b...
Fast adaptive optics and comparatively slower active optics are cornerstones of modern-day astronomy...
Adaptive optics offer the potential to reduce the high cost and long lead time associated with manuf...
We have developed a new type of unimorph deformable mirror for the correction of low-order Zernike m...
Large space telescopes made of deployable and lightweight structures suffer from aberrations caused ...
Some first results of simulation studies for the control of deformable mirrors used to correct the e...
International audienceHigh-contrast imaging (HCI) techniques appear like the best solutions to direc...
International audienceWe present a new active optics method for making smooth aspheric, or freeform,...
Launch costs for high-resolution space telescopes for Earth observation can be reduced when the tele...
The refractive index of air varies a.o. with temperature, humidity, pressure and the CO2 concentrati...
The degradation of astronomical images caused by atmospheric turbulence will be much more severe in ...
Summarization: Some first results of simulation studies for the control of deformable mirrors used t...
A deformable mirror (DM) is an important component of an adaptive optics system. It is known that an...
Concepts for future large space telescopes require an active optics system to mitigate aberrations c...
The wave front corrector is one of the three key elements in adaptive optics, along with the wave fr...
With a view to the next generation of large space telescopes, we investigate guide-starfree, image-b...
Fast adaptive optics and comparatively slower active optics are cornerstones of modern-day astronomy...
Adaptive optics offer the potential to reduce the high cost and long lead time associated with manuf...
We have developed a new type of unimorph deformable mirror for the correction of low-order Zernike m...
Large space telescopes made of deployable and lightweight structures suffer from aberrations caused ...
Some first results of simulation studies for the control of deformable mirrors used to correct the e...
International audienceHigh-contrast imaging (HCI) techniques appear like the best solutions to direc...
International audienceWe present a new active optics method for making smooth aspheric, or freeform,...
Launch costs for high-resolution space telescopes for Earth observation can be reduced when the tele...
The refractive index of air varies a.o. with temperature, humidity, pressure and the CO2 concentrati...
The degradation of astronomical images caused by atmospheric turbulence will be much more severe in ...
Summarization: Some first results of simulation studies for the control of deformable mirrors used t...
A deformable mirror (DM) is an important component of an adaptive optics system. It is known that an...
Concepts for future large space telescopes require an active optics system to mitigate aberrations c...
The wave front corrector is one of the three key elements in adaptive optics, along with the wave fr...