Adaptive optics (AO) systems currently under investigation will require at least two orders of magitude increase in the number of actuators, which in turn translates to effectively a 104 increase in compute latency. Since the performance of an AO system invariably improves as the compute latency decreases, it is important to study how today's computer systems will scale to address this expected increase in actuator utilization. This paper answers this question by characterizing the performance of a single deformable mirror (DM) Shack-Hartmann natural guide star AO system implemented on the present-generation digital signal processor (DSP) TMS320C6701 from Texas Instruments. We derive the compute latency of such a system in terms of a few ba...
Adaptive optics (AO) is a technique for correcting aberrations introduced when light propagates thro...
The performance of a wide-field adaptive optics system depends on input design parameters. Here we i...
Refractive index variations in the earth's atmosphere cause wavefront aberrations and limit thereby ...
Adaptive optics (AO) systems currently under investigation will require at least two orders of magit...
We present a cost-effective scalable real-time wavefront control architecture based on off-the-shelf...
Atmospheric turbulence reduces the achievable resolution of ground based optical telescopes. Adapti...
This paper reflects, from a computational perspective, on the experience gathered in designing and i...
The forthcoming Extremely Large Telescopes (ELTs) all require adaptive optics systems for their succ...
The speed of real-time adaptive optical systems is primarily restricted by the data processing hardw...
We present a cost-effective scalable real-time wavefront control architecture based on off-the-shelf...
Prototyping and benchmarking was performed for the Real-Time Controller (RTC) of the Narrow Field In...
The new generation of extremely large telescopes will have adaptive optics. Due to the complexity an...
With two large deformable mirrors with a total of more than 7000 actuators that need to be driven fr...
The Real-Time Controller (RTC) for the Thirty Meter Telescope (TMT) Narrow Field Infrared Adaptive O...
Future light-weighted and segmented primary mirror systems require active optical control to maintai...
Adaptive optics (AO) is a technique for correcting aberrations introduced when light propagates thro...
The performance of a wide-field adaptive optics system depends on input design parameters. Here we i...
Refractive index variations in the earth's atmosphere cause wavefront aberrations and limit thereby ...
Adaptive optics (AO) systems currently under investigation will require at least two orders of magit...
We present a cost-effective scalable real-time wavefront control architecture based on off-the-shelf...
Atmospheric turbulence reduces the achievable resolution of ground based optical telescopes. Adapti...
This paper reflects, from a computational perspective, on the experience gathered in designing and i...
The forthcoming Extremely Large Telescopes (ELTs) all require adaptive optics systems for their succ...
The speed of real-time adaptive optical systems is primarily restricted by the data processing hardw...
We present a cost-effective scalable real-time wavefront control architecture based on off-the-shelf...
Prototyping and benchmarking was performed for the Real-Time Controller (RTC) of the Narrow Field In...
The new generation of extremely large telescopes will have adaptive optics. Due to the complexity an...
With two large deformable mirrors with a total of more than 7000 actuators that need to be driven fr...
The Real-Time Controller (RTC) for the Thirty Meter Telescope (TMT) Narrow Field Infrared Adaptive O...
Future light-weighted and segmented primary mirror systems require active optical control to maintai...
Adaptive optics (AO) is a technique for correcting aberrations introduced when light propagates thro...
The performance of a wide-field adaptive optics system depends on input design parameters. Here we i...
Refractive index variations in the earth's atmosphere cause wavefront aberrations and limit thereby ...