2017
DOI: 10.1364/josaa.34.001535
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Nonlinear spline wavefront reconstruction from Shack–Hartmann intensity measurements through small aberration approximations

Abstract: We propose an extension of the Spline based ABerration Reconstruction (SABRE) method to Shack-Hartmann (SH) intensity measurements, through small aberration approximations of the focal spot models. The original SABRE for SH slope measurements is restricted to the use of linear spline polynomials, due to the limited amount of data, and the resolution of its reconstruction is determined by the number of lenslets. In this work, a fast algorithm is presented that directly processes the pixel information of the foc… Show more

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Cited by 5 publications
(6 citation statements)
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“…(13) in a distributed manner without approximation errors, future work should investigate the formulation of the distributed DM projection problem, e.g., as a sharing optimization problem with ADMM [19]. Coupling constraints on local command vectors u i can be employed to achieve consensus between actuators that are shared by neighboring partitions or whose influence functions reach neighboring partitions [17].…”
Section: A Distributed Projection Problemmentioning
confidence: 99%
See 1 more Smart Citation
“…(13) in a distributed manner without approximation errors, future work should investigate the formulation of the distributed DM projection problem, e.g., as a sharing optimization problem with ADMM [19]. Coupling constraints on local command vectors u i can be employed to achieve consensus between actuators that are shared by neighboring partitions or whose influence functions reach neighboring partitions [17].…”
Section: A Distributed Projection Problemmentioning
confidence: 99%
“…The SH sensor is an array of lenslets that creates a focal spot pattern from which approximations of the local spatial WF gradients in each subaperture are derived [1,15]. Whereas the limited amount of processed data, i.e., two slope measurements per subaperture, restricts the slope-based D-SABRE method to linear B-spline polynomials, two approaches have been introduced that can extend the method to higher degree polynomials: (1) by exploiting the integrative nature of the SH sensor, a more advanced sensor model has been implemented that utilizes first-and second-order moment measurements of the focal spots [16]; and (2) by combining the standard D-SABRE with an additional correction step in which the pixel information in the focal spots is directly worked with, using an algorithm based on small aberration approximations of the focal spot models [17]. Employing a cubic B-spline representation of the phase, both approaches can achieve WF estimates that are superior to the linear D-SABRE WF estimates if applied to a given SH array.…”
Section: Introductionmentioning
confidence: 99%
“…9,10 The SHWFS operates on two fundamental procedures: wavefront slope calculation and wavefront reconstruction algorithms. The previous research on reconstruction algorithms primarily focused on spatial domain analysis [11][12][13][14] to evaluate the performance of the reconstructors. Departing from conventional metrics, the spatial frequency response provides comprehensive insights into assessing distinct wavefront reconstructors.…”
Section: Introductionmentioning
confidence: 99%
“…A reason is that the use of double exposure procedures for such a measurement process would inevitably generate unwanted noise to the obtained data. Fortunately, under certain circumstances the phase can be estimated from only one PSF image; see, for example, [3,5,7]. In this paper, we investigate the phase retrieval problem, given a single PSF image, with a priori information that the phase is sparse.…”
mentioning
confidence: 99%
“…The Frobenius norm and the maximum norm are denoted by \| \cdot \| and \| \cdot \| \infty , respectively. Mathematical operations including the multiplication, the division, the modulus, the argument, 3 the exponential, the square, the square root, and the equality are understood elementwise in this paper. The distance function associated to a set \Omega \subset \BbbC n\times n is defined by dist(\cdot , \Omega ) : \BbbC n\times n \rightar \BbbR + : x \mapsto \rightar inf w\in \Omega \| x -w\| , and the set-valued mapping P \Omega : \BbbC n\times n \rightri \Omega : x \mapsto \rightar \{ w \in \Omega | \| x -w\| = dist(x, \Omega ) \} is the corresponding projector.…”
mentioning
confidence: 99%