# US 2013/0278763 A1 · Method and system for compensating optical aberrations in a telescope > Agents: this data is available as JSON from the patentgrep API and MCP server — see https://patentgrep.com/llms.txt - Number: US 2013/0278763 A1 - Document ID: US20130278763A1 - Status: Published application - Kind: A1 - Application number: 13/813,408 - Filed: 2011-07-22 - Published: 2013-10-24 - Earliest claimed: 2010-07-30 - Assignees: Pontificia Universidad Catolica De Chile; Universitat Politecnica De Catalunya - Inventors: Santiago Royo Royo; Vincent Suc - Web page: https://patentgrep.com/patent/US20130278763A1 ## CPC - G02B 23/06: having a focussing action, e.g. parabolic mirror - G02B 27/0025: {for optical correction, e.g. distorsion, aberration} - G02B: OPTICAL ELEMENTS, SYSTEMS OR APPARATUS ## Abstract A method and a system are for compensating optical aberrations in a telescope. The method is applicable to a telescope wherein the element for receiving a primary beam is an image acquisition device (3), and involves using an algorithm without an image processing sensor for: a) detecting optical aberrations affecting the primary focus, by analyzing the images acquired by the image acquisition device (3), and b) calculating and generating first positional correction values, by processing the detected optical aberration values. The method also includes a step c) consisting in moving, in a controlled manner, the image acquisition device (3), applying suitable control signals generated from the first positional correction values. The system is suitable for implementing the proposed method. ## Claims ### Claim 1 Method for compensating optical aberrations in a telescope, comprising carrying out the following steps in an automatic manner: a) detecting optical aberrations affecting the primary focus, by analysis of at least one image acquired by the image acquisition device; b) calculating, based on said optical aberrations detected in a), to compensate for the aberrations detected first positional correction values, c) moving, in a controlled manner, at least one element for receiving a primary beam after being reflected by a primary mirror or refracted by a focus lens of said telescope, by application of suitable control signals generated from said first positional correction values, the method being applied to a telescope wherein said element for receiving a primary beam to be moved in c) is said image acquisition device, and comprising using an algorithm without an image processing sensor to carry out said step a), by said analysis of at least one image acquired by said image acquisition device, and to carry out said step b), by processing of the values of the detected optical aberrations and the generation of said first positional correction values as a result of said processing. ### Claim 2 (depends on 1) The method according to claim 1, wherein said sensorless algorithm is a sensorless adaptive optics algorithm. ### Claim 3 (depends on 1) The method according to claim 1 further comprising carrying out a calibration process including carrying out a plurality of steps a) for a corresponding plurality of positions of said telescope, correlating data of the detected optical aberrations with data of the positions of the telescope for which they have been detected, and recording said correlations in an aberration correction registry. ### Claim 4 (depends on 3) The method according to claim 3, wherein said calibration process also comprises carrying out a plurality of said steps b) for said plurality of positions of the telescope and correlating the data of the first positional correction values calculated with the data relative to the detected optical aberrations and with the data of the corresponding positions of the telescope, and including said data of the first positional correction values in said aberration correction registry. ### Claim 5 (depends on 3) The method according to claim 3, further comprising orienting the telescope towards determined coordinates, consulting said aberration correction registry to look for the data of the position of the telescope after being oriented in this manner and the correlated data of the detected optical aberrations, and moving, in step c), the image acquisition device depending on the optical aberration data obtained as a result of said consultation of said aberration correction registry. ### Claim 6 (depends on 4) The method according to claim 4, further comprising orienting the telescope towards determined coordinates, consulting said aberration correction registry to look for the data of the position of the telescope after being oriented and the correlated data of the first positional correction values and moving, in step c), the image acquisition device depending on the first positional correction values extracted from said aberration correction registry. ### Claim 7 (depends on 5) The method according to claim 5 further comprising with the purpose of determining said orientation of the telescope towards said determined coordinates, correcting positioning errors with respect to a mounting system, detecting at least values of said positioning errors, directly and/or indirectly, and using a pointing algorithm to process said values, and supplying, as a result of said processing, second positional correction values. ### Claim 8 (depends on 7) The method according to claim 7, further comprising carrying out said correction of positioning errors, also detecting values of one or more non-positional parameters that have an influence on generation of said positioning errors, and using said pointing algorithm to also process said values of said non-positional parameters. ### Claim 9 (depends on 8) The method according to claim 8, further comprising carrying out a training system including detecting values of said positioning errors for a plurality of positions of the telescope regarding the mounting system, in detecting and/or calculating values of said non-positional parameters for at least each one of said plurality of positions of the telescope and/or for different working temperatures to which the telescope is submitted, and in using said pointing algorithm to process all of said values, to supply and correlate the corresponding second positional correction values with the values of the positioning errors and non-positional parameters, and to record said correlations in a pointing registry. ### Claim 10 (depends on 8) The method according to claim 8 wherein among said non-positional parameter or parameters that have an influence on the generation of said positioning errors, the method comprises supplying the values of the non-positional parameter or parameters that also have an influence on the optical system of the telescope, to said sensorless algorithm, and processing the values of the non-positional parameter or parameters by means thereof, together with the values of the detected optical aberrations in order to calculate, in step b), said first positional correction values. ### Claim 11 (depends on 10) The method according to claim 10, wherein said calibration process also comprises at least detecting and/or calculating the values of said non-positional parameters for at least each one of said plurality of positions of the telescope and/or for different working temperatures to which the telescope is submitted, and including said detected values in said aberration correction registry, as well as using said detected values for the calculation, in said plurality of steps b), of said data of the first positional correction values and including the first positional correction values in the aberration correction registry, also correlated with the detected and/or calculated values of said non-positional parameters. ### Claim 12 (depends on 11) The method according to claim 11, further comprising orienting the telescope towards determined coordinates, consulting said aberration correction registry to look for the data of the telescope position after being oriented, the values of said detected and/or calculated non-positional parameters, and the correlated data of the first positional correction values, and moving, in step c), the image acquisition device according to the data of the first correctional position values consulted in said aberration correction registry. ### Claim 13 (depends on 12) The method according to claim 12 further comprising with the purpose of obtaining, with respect to a region in space located in determined coordinates, images that are substantially free from influence of optical aberrations and positioning errors, carrying out the following actions:—detecting, for the position of the telescope with respect to mounting system, corresponding to said coordinates, the values of the positioning errors and working temperature and detecting and/or calculating the values of said non-positional parameters corresponding to said position and working temperature;—consulting the detected values of the positioning errors and the detected and/or calculated values of the non-positional parameters in said pointing registry, obtaining the correlated second positional correction values and using the correlated second positional correction values to orient the telescope towards said coordinates in a precise manner; consulting said aberration correction registry to look for the first positional correction values correlated with the data of the position of the telescope corresponding to said coordinates and to the values of said detected and/or calculated values of said non-positional parameters; and—moving, in step c), the image acquisition device according to the data of the first positional correction values obtained in said consultation of the aberration correction registry. ### Claim 14 The method according to wherein said step b) also comprises calculating, based on at least said optical aberrations detected in a), with the purpose of compensating for said optional aberrations detected in a), third positional correction values for an element for receiving a beam reflected by a secondary mirror of the telescope, and wherein said step c) also comprises moving said elements for receiving said beam reflected by said secondary mirror by application of suitable signals generated based on said third positional correction values. ### Claim 15 (depends on 1) The method according to claim 1, further comprising using said sensorless algorithm by adjusting width of a frequency spectrum to be analyzed and processed to limit effects related to shadows due to obstructions appearing in the image or images, caused by interposition of said image acquisition device and/or any other element, between incident light and the primary mirror. ### Claim 16 (depends on 15) The method according to claim 15, wherein said frequency spectrum to be analyzed and processed by the sensorless algorithm is between 0.5 and 20% of the a total frequency spectrum of the acquired images. ### Claim 17 (depends on 1) The method according to claim 1, wherein said at least one of the aberrations to be compensated belong to the group consisting of the following low-order optical aberrations: defocus, distortion, tilt, coma, or a combination thereof. ### Claim 18 (depends on 8) The method according to claim 8, wherein one or more of said non-positional parameters belong to the group consisting of the following non-positional parameters: expansion coefficients due to temperature, flexure of the support of a mirror, flexure of a support of an image capture device, flexure of the tube of the telescope, flexure of the mounting system or mount of the telescope, or a combination thereof, and because said positioning errors refer to at least one of the following positional parameters related to the mounting system of the telescope: delta displacement parameter and alpha displacement parameter of the reference of each axis, delta non-perpendicularity parameter and alpha non-perpendicularity parameter of the axes, horizontal alignment error parameter and vertical alignment error parameter to the pole, for an equatorial mounting system or mount, or to the zenith point, for an alt-azimuth mounting system or mount, or a combination thereof. ### Claim 19 (depends on 1) The method according to claim 1, further comprising moving said image acquisition device by moving a mobile support thereof according to different degrees of freedom. ### Claim 20 System for compensating optical aberrations in a telescope, said telescope comprising at least one element for receiving a primary beam after being reflected by a primary mirror or refracted by a focus lens of said telescope, the system comprising:—first detecting means that comprise, an image acquisition device, and are envisaged to detect the optical aberrations that affect primary focus of a telescope by analysis of one or more images acquired by said image acquisition device; and an electronic system connected or integrating at least part of said first detecting means and connected at least to said element for receiving a primary beam, said electronic system being configured to calculate, based on the detected optical aberrations with the purpose of compensating for the detected optical aberrations first positional correction values to generate, based on the the first correction values, control signals to apply them to at least one actuating device of said element for receiving a primary beam, or on a mobile support thereof, with the purpose of moving the mobile support in a controlled manner; wherein the system is applied to a telescope wherein said element for receiving a primary beam to be moved in a controlled manner is said image acquisition device wherein said first detecting means are integrated in part to said electronic system, and wherein said electronic system implements an algorithm without an image processing sensor to carry out said detection of aberrations by said analysis of said image or images acquired by said image acquisition device, to process the values of the detected optical aberrations and to generate said first positional correction values and said control signals. ### Claim 21 (depends on 20) The system according to claim 20, wherein said sensorless algorithm implemented in said electronic system is a sensorless adaptive optics sensor. ### Claim 22 (depends on 20) The system according to claim 20, wherein said mobile support of the image acquisition device is mounted on a support and positioning structure arranged in the telescope and provided to displace the mobile support, and with the mobile support the image acquisition device according to at least the following movements:—linear backward/forward movement along the direction of the longitudinal axis of the tube of the telescope, to compensate defocus aberrations;—rotary movement with respect to both axes, perpendicular to one another and with respect to said longitudinal axis of the tube of the telescope, to compensate distortion and tilt aberrations; and—lateral movement along a perpendicular plane of the longitudinal axis of the telescope, to compensate coma aberrations. ### Claim 23 (depends on 22) The system according to claim 22, wherein said support and positioning structure comprises at least three actuating mechanisms mounted in three respective points along a contour of the tube of the telescope, protruding outwards from a tube, each one of which also being connected to a respective point of the mobile support by a respective connecting element, the electronic system being configured to control said actuating mechanisms, which are at least three, by generation and application of said control signals to provoke a combined actuation that moves the mobile support to compensate the detected optical aberrations. ### Claim 24 (depends on 23) The system according to claim 23, wherein said three points are separated from each other at an angular distance of substantially 120°. ### Claim 25 (depends on 23) The system according to claim 23, wherein each one of the said actuating mechanisms, which are at least three, is configured to move a respective connecting element and therefore the mobile support, along a respective plane that contains, or is parallel to a plane that contains, the longitudinal axis of the tube of the telescope. ### Claim 26 (depends on 25) The system according to claim 25, wherein each one of the actuating mechanisms, which are at least three, comprise:—at least one first arm joined by an intermediate area to said connecting element and a second arm joined, by a first extremity or by an area close to said first extremity, by a first articulation, to said point of the contour of tube of the telescope, and also joined, by said first extremity, to a first extremity of said first arm by a second articulation, and—at least two motors, each one of the mothers connected to one of said first and second arms to move the first and second arms, respectively, according to a rotary movement around said first and second articulations. ### Claim 27 (depends on 23) The system according to claim 23, wherein said connecting elements are respective metal sheets arranged occupying respective planes that contain, or are parallel to planes that contain, the longitudinal axis of the tube of the telescope, with the purpose of minimizing the interference thereof in a path of a beam directed towards the primary mirror. ### Claim 28 (depends on 23) The system according to claim 23, wherein said connecting elements are arranged under tension, and wherein the electronic system is configured to control the actuating mechanisms, which are at least three, by application of said control signals in successive increments, in each one of the actuating mechanisms to displace the mobile support from a compensation point to a neighboring point without loosening the connecting elements. ### Claim 29 (depends on 1) A system configured to implement the method of claim 1, carrying out said steps a) and b) by the electronic system and the image acquisition device, and said step c) by the electronic device in collaboration with said actuation means.