2010
DOI: 10.1117/12.845608
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Preliminary results of large-actuator-count MEMS DM development

Abstract: Compensating for atmospheric turbulence in meter-class telescopes and for free-space communications can require deformable mirrors (DM) with hundreds of actuators. Advances in high-contrast imaging techniques and increased telescope sizes require DMs mirrors with thousands of actuators [1]- [3]. In response to these needs, Iris AO has been developing a nearly 500-actuator DM and is conducting pathfinding research into 3000-actuator class DMs. This paper begins with an overview of the segmented DM design and de… Show more

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“…where the terms appearing before the sums in Equation 13 and Equation 14 are the ratios between the area of one segment and the normalization coefficients of the Zernike or hexagonal polynomials. The comparison between the theoretical fitting errors and the values obtained by means of simulations are presented in Fig.…”
Section: Zernike Modesmentioning
confidence: 99%
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“…where the terms appearing before the sums in Equation 13 and Equation 14 are the ratios between the area of one segment and the normalization coefficients of the Zernike or hexagonal polynomials. The comparison between the theoretical fitting errors and the values obtained by means of simulations are presented in Fig.…”
Section: Zernike Modesmentioning
confidence: 99%
“…Control authority for the wavefront is largely assigned to a second stage of optical system and thus on active or adaptive optics element (i.e., small-size deformable mirrors.) In adaptive optics, advanced wavefront control devices such as small-size segmented deformable mirrors [12][13][14][15] made of hexagonal segments are intensively used in astronomy [16][17][18], laser shaping [19], retinal imaging systems [7,20], microscopy [21,22] or laser communication [23].…”
Section: Introductionmentioning
confidence: 99%
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