165 results about "Atmospheric refraction" patented technology

A device for detecting the effects of an atmospheric turbulence to space laser communication provided by the invention consists of an emitting terminal and a receiving terminal; the emitting terminal consists of a laser expanding lens (1), a laser expanding lens (2), a laser expanding lens (3), a fixing mechanism (4), a semiconductor laser array (5), a pitch rotating floor (6) and a course rotating floor (7); the receiving terminal consists of an adjustable diaphragm (8), a card type system (9), a lens (10), a lens (11), a photodetector (12), a computer (13), a lens (14), a CCD camera (16), a pitch rotating floor (17), a course rotating floor (18) and a dispersion prism(19). The detecting device can realize the detecting of the effects of the atmospheric turbulence to space laser communication, can measure an atmospheric refraction index constant, can validate different receiving calibers and different CCD integral times as well as an atmospheric twinkling variance during multi-caliber emitting and can give the time domain and space domain distribution situations of light intensity.

The invention discloses a ship-borne high-precision star sensor setting angle calibrating method, and relates to the field of spacecraft attitude control ground application to solve the problem of unable reaction of accurate calibration of the setting angle of a ship-borne star sensor in the prior art. A ship-borne radar equipment pedestal is provided with a star sensor; when a ship docks, a ship-borne alignment calibration theodolite determines the course angle of a measurement ship through a star measurement or azimuth vane tracking technology, and the horizontal reference pitching angle and rolling angle of a whole ship are calibrated to obtain an inertial navigation horizontal system to deck coordinate system transformation matrix; and the star sensor shoots a star atlas, the observation vectors and the reference vectors of i fixed stars are obtained, the azimuths and the pitching angles of the i fixed stars in a view field are calculated, the pitching angles undergo atmospheric refraction correction one by one, the inertial navigation horizontal system reference vectors of the i fixed stars are reconstructed, and star sensor attitude matrix and the ship-borne star sensor setting matrix under the inertial navigation horizontal system are calculated to resolve the setting angle. The method improves the measurement precision of the attitude of the body of a spaceflight measurement ship.

The present invention discloses a method for measuring second-grade river-crossing leveling height difference by using an intelligent total station. The method is characterized in that, various river-crossing leveling points are firstly arranged; the height difference among the river-crossing leveling points is measured; an intelligent total station and a reflecting prism are adopted among the river-crossing leveling points positioned on different banks during the measurement process to carry out the synchronous and opposite observation of both banks of the river. According to the present invention, the equipment height is fixed, the alignment is forced to be performed, the intelligent total station and the reflecting prism are arranged integratedly; because the optical alignment and the measurement of the equipment height are not required, the error of the optical alignment and the error of the measurement of the equipment height are avoided; the synchronously-performed river-crossing leveling height measurement counteracts the atmospheric refraction error so as to substantially improve work efficiency and measurement accuracy.

The invention provides a method for correcting the influence of atmospheric refraction on the precision of a star sensor, which comprises the following steps: according to the optic axis orientation of an image of the star sensor, calculating the zenith distance of the optic axis orientation of the star sensor; recognizing the star image coordinates of fixed stars in the viewing field of the starsensor by using a star map recognition algorithm; calculating the zenith distances of the recognized fixed stars in the viewing field of the star sensor; decomposing an atmospheric refraction value into an X-axis direction component and a Y-axis direction component under an image space coordinate system of the star sensor; and subtracting the deviation delta X and delta Y (arising from the atmospheric refraction value) from all successfully-recognized star images of the fixed stars, thus calculating attitude quaternions. When the influence of atmospheric refraction is eliminated, the star sensor can provide high-precision navigation information for shipborne, missile-mounted and airborne aircraft and other aircraft which carry out low-altitude flying; and after carriers adopt atmospheric-refraction-corrected high-precision navigation information, a basis is provided for planning a better navigation path for the carriers, thereby further reducing the fuel consumption of the carriers and improving the efficiency.

A system and method are disclosed for determining geoposition of an observer. The system includes a sensor such as a wide field of view camera or telescope that can capture an image of the sky. The image of the sky is used to compile a table or list of the stars in the sky along with their positions. This table or list is pattern-matched with a predetermined list or table of stars to identify each star. In one embodiment, the distances between all stars in the image are computed and compared to star images from an atmospheric refraction model. A comparison of the measured table or list and the refraction model, using an optimization algorithm, is performed to determine the geoposition of the observer. In an alternative embodiment, a sensor capable of measuring two different frequency bands obtains two images of each star in the sky simultaneously. A difference in displacement is determined between the two frequencies for each imaged star; and a magnitude and direction of the difference in displacement is used to determine the geoposition of a body.

An illumination device that illuminates an original document by propagating an illuminating light beam output from each of a plurality of light emitting diodes from a first end surface of a light guide to a second end surface of the light guide. Assuming that A is a dimension from the first end surface of the light guide to the second end surface of the light guide, B is an interval between adjoining light emitting diodes, the light emitting diodes being arranged in an array format in a main scanning direction, n1 is a refractive index of atmosphere outside of the light guide, and n2 is a refractive index of the light guide, a condition of tan⁻¹(B/2A)≦β≦π/2−{sin⁻¹(n1/n2)} is satisfied.

The invention discloses a solar energy sun chasing and state monitoring system and a method thereof. According to the system, an upper computer is used as a control center; an astronomical calendar theory expansion formula is used to calculate an azimuth angle and a height angle of the sun. Then, an error caused by atmospheric refraction and an altitude is corrected, a horizontal angle and a pitch angle of a power generation plate are calculated and are transmitted to each tracking transmission mechanism so that sun chasing motion is executed. Simultaneously, software acquires local weather phenomena through a network, such as a cloudy sky, rain, snow, wind and other information, complements on-site illumination and a wind power detection result, and sends instructions of protection, stopping, starting, tracking and the like to a sun chasing control device. The system has the advantages that concentration control is used; cost is low; an anti-interference performance is strong and a tracking error is small.

The disclosed technology relates to systems and methods for determining three-dimensional atmospheric and ionospheric density using refraction of electromagnetic waves. A method is provided for receiving, at a processing system, and from a plurality of Global Navigation Satellite Systems (GNSS) stations, navigation data corresponding to computed positions of the plurality of GNSS stations. The method can further include determining, based at least in part on received navigation data and received GNSS transmitter information, ionosphere and atmosphere refractivity corresponding to intersections of two or more GNSS signals. The method can include calculating, based on the determined 3D density states, data fields of a model representing the three-3D density states. The method can include transmitting position adjustment data to calibrate a navigation position of at least one of the plurality of the GNSS stations based at least in part on the calculated data fields of the model.

The invention provides a high orbit area array optical satellite in orbit geometry calibration method considering atmospheric refraction rectifications; the method comprises the following steps: usingpolynomial fitting probe directional angles to build an internal calibration model, parsing influence rules on the image geometry precision by the atmospheric refraction, building an external calibration model considering the atmospheric refraction rectification, and introducing the internal and external calibration models into a strict geometry imaging model so as to build a high orbit optical satellite in orbit geometry calibration model; parsing internal and external calibration parameter initial values according to sub-satellite point images; using the parsed internal calibration parameter as the true-value, using images obtained by different sequence imaging angles, and parsing the external calibration parameter according to the external calibration parameter initial value. In the high orbit optical satellite in orbit geometry calibration process, the method can fully consider the influences on the imaging geometry precision by the atmospheric refraction, thus building the more strict in orbit geometry calibration model, and obviously improving the high orbit optical satellite image direct geometry positioning precision.

The invention provides a method for forward simulation of occultation. The method is applicable to the GNSS earth atmosphere occultation exploration constellation design and analysis application. According to the method, satellite orbit parameters serve as design input, constellation construction parameters are supplemented to serve as design input, and constellation design and analysis application are facilitated; influence of atmospheric refraction is taken into comprehensive consideration in the process of occultation event judgment and positioning, and occultation measuring point positioning accuracy is improved; ground data transmission station modeling is added, and downloading timeliness of occultation exploration data can be supplemented and analyzed.

The invention discloses a method for on-line correcting low-angle radar electric wave refraction error. When a radar measures a target, radar measured parameter distance and angle are used to obtain radar positioning parameters with atmosphere refraction errors eliminated through a device formed by a GPS receiver, a ground atmospheric refractivity measuring instrument, an atmosphere profile database, a control and data processor and related interface circuits. The parameters are used for positioning a target, and the radar positioning precision is improved. The refraction error correction method is simple, and low in computation burden, short in time, high in precision, high in automation level and easy for realization. The method realizes on-line correcting radar electric wave refraction error in a high-precision way.

A polar scope for a telescope mount includes a reticle having a pattern with multiple markings that allows users to accurately position pole stars for precise polar alignment. A system and mount may be provided including a polar scope of this kind. The polar scope may be provided with a controller that calculates the apparent position of a pole star, while accounting for errors, such as proper motion, precession of the earth's axis, and/or atmospheric refraction.

The invention discloses a method and a system for compensating atmospheric refraction in optical satellite remote sensing data geographic positioning. The method for compensating the atmospheric refraction in the optical satellite remote sensing data geographic positioning comprises an earth radius compensating step, and is used for calculating the coordinate of a ground point corresponding to a certain pixel point in a satellite image by supposing that the earth radius is equal to the summation of the actual earth radius and the compensation amount of the earth radius. The method not only can be used for performing correction on the remote sensing data of SPOT-5, but also can be used for performing correction on other satellite remote sensing data; and due to the adoption of the method, the positioning accuracy after the compensation of the atmospheric refraction is obviously improved.

The invention relates to a star sensor calibrating method based on detection data of a high-precision telescope. The star sensor calibrating method comprises the following steps: shooting on a number of star maps in the current view field on an orbit by using the telescope and a star sensor respectively, and in order to reduce influence of a random error, performing multi-frame averaging on star coordinates of the star maps and performing other on-orbit processing; performing comparative analysis on observation data of the high-precision telescope and star map data of the star sensor; according to a star sensor calibrating model, determining a star sensor calibrating coefficient so as to achieve high-precision calibration of the star sensor. By the star sensor calibrating method based on the detection data of the high-precision telescope, provided by the invention, influence of atmospheric refraction and other factors on ground calibration can be eliminated, calibration parameter changes caused by temperature, vibration and other reasons can be compensated, high-precision on-orbit calibration of the star sensor can be achieved, and the accuracy of star sensor measurement is further improved; therefore, the star sensor calibrating method has an engineering application value.

The invention discloses a target positioning method applicable to a vehicle-mounted photoelectric watching-aiming system with atmospheric refraction and belongs to the technical field of vehicle-mounted photoelectric observation. By adopting the target positioning method, geographical location information of a target can be solved in real time by modifying light deflection with atmospheric refraction and implementing coordinate conversion calculation of different coordinate systems according to geographical location information of a carrying vehicle, posture angles of the carrying vehicle, angles of a photoelectric turret, laser ranging values, the altitude of a target point and atmospheric parameters of a carrying vehicle point. By adopting the target positioning method, target positioning errors caused by atmospheric refraction can be modified on the basis of a conventional vehicle-mounted target positioning way, that is, vehicle-mounted target positioning precision is improved through innovation of techniques, and the method has the characteristics of being high in calculation precision, simple to operate, and the like.

An atmospheric refraction profile is determined using an imaging system positioned at a location that is simultaneously within line-of-sight of two celestial light sources. A variety of active or passive methods can be employed to cause the line-of-sight to vertically traverse through a refractive portion of an atmosphere. Images of the two celestial light sources are captured as the line-of-sight vertically traverses through the refractive portion of the atmosphere. Each such image indicates an apparent distance between the two celestial light sources. The apparent distances are used to determine refraction angles.

The invention belongs to the field of deformation measurement of buildings and structures, and in particular relates to a method for observing the deformation of a blast furnace. The method for observing the deformation of the blast furnace is characterized in that deformation observing points are respectively set on a brace and a crane beam representing the basic deformation of the blast furnace for using as deformation observing objects for reflecting the incline degree of the furnace body, with the aid of a laser total station and a leveling instrument, the measurement is respectively performed by the planar method and the elevation method, and then the arithmetic mean value of the two measurement results are used as the deformation of the blast furnace. Compared with the prior art, the method for observing the deformation of the blast furnace has the beneficial effects that (1) the cost is saved, the investment is reduced, and important actual guiding significance is provided; (2) reference is provided for the optimal design of the blast furnace; (3) influence of environment, pressure, temperature and atmospheric refraction on the measurement is reduced; and (4) the evaluation of the blast furnace is much closer to the real situation.

The invention relates to an inversion method of the atmospheric refractivity profile. The method comprises the steps that an atmospheric layer is layered; beacon laser is emitted; air sounding equipment vertically ascends to the sounding height of each atmospheric sub layer; the deflection angle of a reflector when the reflector in the air sounding equipment intercepts and captures the beacon laser and returns the beacon laser to a laser receiver, and the received light intensity is maximum is measured; the geocentric angle of the reflector in each atmospheric sub layer and the incidence angle of the beacon laser in each atmospheric sub layer are calculated; the total refraction angle of each atmospheric sub layer and the gradient of the atmospheric refractivity along with the height change are calculated; a drawing is made by using the height as the X axis, the atmospheric refractivity as the Y axis, the atmospheric refractivity of each atmospheric sub layer as a starting point and the gradient of the atmospheric refractivity along with the height change as the slope at each section; the atmospheric refractivity profile is obtained. The inversion method disclosed by the method has the advantages that the atmospheric refractivity profile can be reversed in real time on the spot; technical support and theoretical support are provided for laser application to various engineering fields of satellite high-precision orbit determination, space high-precision measurement and the like which use precise phase information as a basis.

The invention discloses a test system and method for scintillation characteristic of fake partially coherent light transmitted in atmosphere turbulence, and belongs to the technical field of laser signal transmission and detection in an atmospheric channel. The test system comprises a light beam emission sub system and a light beam receiving and detecting sub system, wherein different variances are used to count and calculate parameters, so that a scintillation variance of the fake partially coherent light transmitted in the atmosphere turbulence under different detector integral time conditions is calculated. The system and the method provided by the invention can synchronously measure the scintillation variance of coherent lasers transmitted in the atmosphere turbulence, and a correspondence between the measured scintillation variance and an actual structural constant value of atmospheric. The result tested by the system and the method disclosed by the invention is helpful for optimizing the design of the application system using the fake partially coherent light to restrain the scintillation caused by the atmosphere turbulence.

The invention belongs to the technical field of astrometry and relates to a method for correcting influences of atmosphere inclination on ground star observation values. The method is used for correcting influences of the atmosphere inclination on astronomical longitude and latitude measured values obtained during ground star observation and solves the problem of inaccuracy of existing atmospheric refraction error correction. The method includes the steps: firstly, selecting a plurality of stars as sample stars, establishing a regression model among the observation values of the sample stars, and resolving influence quantity of atmosphere isodensity layer inclination caused by factors such as climate change in observation of each star group; and secondly, correcting the observation values of the stars according to the resolved quantity of the atmosphere isodensity layer inclination. By the method, an apparent zenith distance measured value of each star obtained by observation and star passing record moments can be accurately corrected for atmosphere isodensity layer inclination, and measurement accuracy of astrometric and geodetic instruments is improved.