1998
DOI: 10.1117/12.321687
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Wavefront control system for the Keck telescope

Abstract: The laser guide star adaptive optics system currently being developed for the Keck 2 telescope consists d several major subsystems: the optical bench, wavefront control, user interface and supervisory control, and the laser system. The paper describes the design and implementation of the wavefront control subsystem that controls a 349 actuator deformable mirror for high order correction and tip-tilt mirrors for stabilizing the image and laser positions.

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Cited by 9 publications
(8 citation statements)
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“…For an AO application one should consider that context switching is done most of the time on very few processes (2)(3)(4)(5)(6)(7)(8). For the fastest machines context switch times for up to 8 processes are below 10 mus, a number that is certainly acceptable.…”
Section: Memory Latency and Context Switching Benchmarking With Lmbenchmentioning
confidence: 98%
“…For an AO application one should consider that context switching is done most of the time on very few processes (2)(3)(4)(5)(6)(7)(8). For the fastest machines context switch times for up to 8 processes are below 10 mus, a number that is certainly acceptable.…”
Section: Memory Latency and Context Switching Benchmarking With Lmbenchmentioning
confidence: 98%
“…[35] Norathyriol and its C-glycosylated analogue mangiferin [36] are xanthone natural products isolated from the skin of mangoes that exhibit abroad range of biological activities. [37] Thes ynthesis of 13 is accomplished by cross-coupling of phloroglucinol 10 with 2a on multigram scale (Scheme 3B). Oxidation of the C5 methyl group to the carboxylic acid provides 12,w hich is subsequently converted into 13 by aF riedel-Crafts acylation.…”
Section: Angewandte Chemiementioning
confidence: 99%
“…The WFC consists of two separate real-time control loops: a tip-tilt coniroller to remove tilt from the incoming wavefront [3], and a deformable mirror controller to remove higher-order aberrations [4]. A block diagram of the two nested control loops is shown in Figure 1.…”
Section: Atmospheric Wavefront Disturbancementioning
confidence: 99%
“…It is discussed in detail in reference [4]. The controller initially receives raw CCD image data from the wavefront sensor (a Hartmann sensor using an Adaptive Optics Associates camera with a MiT Lincoln Lab CCD) and computes centroids for each of the subapertures using a quad-cell calculation to estimate the wavefront gradient.…”
Section: The Deformable Mirror Controllermentioning
confidence: 99%