Large (>1m) deformable mirrors with hundreds or thousands of actuators are attractive for extremely large telescopes. Use of force actuators coupled to the mirror via suction cups, and electret microphones for position sensing, has the potential of substantially reducing costs. However, a mirror controlled with force actuators will have many structural resonances within the desired system bandwidth, shifting the emphasis somewhat of the control aspects. Local velocity and position loop for each actuator can add significant damping, but gives poor performance at high spatial frequencies. We therefore introduce a novel control strategy with many parallel "actuator families", each controlled by single-input-single-output controllers. This fami...
We study a concept for a low-cost, large deformable mirror for an Extremely Large Telescope. The use...
Large (>1 m) deformable mirrors are attractive for adaptive optics on ground-based telescopes; the m...
itself rather than using relay optics within an instrument, the resulting large DM can be expensive,...
Large (>1m) deformable mirrors with hundreds or thousands of actuators are attractive for extremely ...
Large (> 1m) deformable mirrors with hundreds or thousands of actuators are attractive for extremely...
Large (> 1m) deformable mirrors with hundreds or thousands of actuators are attractive for extremely...
While it is attractive to integrate a deformable mirror (DM) for adaptive optics (AO) into the teles...
While it is attractive to integrate a deformable mirror (DM) for adaptive optics (AO) into the teles...
While it is attractive to integrate a deformable mirror (DM) for adaptive optics (AO) into the teles...
While it is attractive to integrate a deformable mirror (DM) for adaptive optics (AO) into the teles...
It is attractive to integrate a large deformable mirror for adaptive optics into an astronomical tel...
While it is attractive to integrate a deformable mirror (DM) for adaptive optics (AO) into the teles...
Large, high-bandwidth deformable mirrors (DMs) with thousands of actuators for adaptive optics are o...
While it is attractive to integrate a deformable mirror (DM) for adaptive optics (AO) into the teles...
Large (>1m) deformable mirrors are attractive for adaptive optics on ground-based telescopes; the mi...
We study a concept for a low-cost, large deformable mirror for an Extremely Large Telescope. The use...
Large (>1 m) deformable mirrors are attractive for adaptive optics on ground-based telescopes; the m...
itself rather than using relay optics within an instrument, the resulting large DM can be expensive,...
Large (>1m) deformable mirrors with hundreds or thousands of actuators are attractive for extremely ...
Large (> 1m) deformable mirrors with hundreds or thousands of actuators are attractive for extremely...
Large (> 1m) deformable mirrors with hundreds or thousands of actuators are attractive for extremely...
While it is attractive to integrate a deformable mirror (DM) for adaptive optics (AO) into the teles...
While it is attractive to integrate a deformable mirror (DM) for adaptive optics (AO) into the teles...
While it is attractive to integrate a deformable mirror (DM) for adaptive optics (AO) into the teles...
While it is attractive to integrate a deformable mirror (DM) for adaptive optics (AO) into the teles...
It is attractive to integrate a large deformable mirror for adaptive optics into an astronomical tel...
While it is attractive to integrate a deformable mirror (DM) for adaptive optics (AO) into the teles...
Large, high-bandwidth deformable mirrors (DMs) with thousands of actuators for adaptive optics are o...
While it is attractive to integrate a deformable mirror (DM) for adaptive optics (AO) into the teles...
Large (>1m) deformable mirrors are attractive for adaptive optics on ground-based telescopes; the mi...
We study a concept for a low-cost, large deformable mirror for an Extremely Large Telescope. The use...
Large (>1 m) deformable mirrors are attractive for adaptive optics on ground-based telescopes; the m...
itself rather than using relay optics within an instrument, the resulting large DM can be expensive,...