CN1124470C - Precise azimuth measuring method - Google Patents
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Abstract
一种方位的精确测定方法,包括以下工作步骤:将成像系统指向太阳,采集太阳图象,根据太阳图象读出其方位值,将太阳的方位值输入计算机,由GPS系统向计算机输入观测点的座标与标准时间,计算机算出测点的精确方位。本发明不受时间和太阳位置的限制,可以随时、方便地校准设备的座标,且动作快捷地显示精确方位,精度可以提高到1/10度或1/100度,能满足现代科研、军事以及工业生产等领域的需要。
A method for accurately measuring the orientation, including the following working steps: point the imaging system to the sun, collect the image of the sun, read out the orientation value according to the image of the sun, input the orientation value of the sun into the computer, and input the observation point into the computer from the GPS system The coordinates and standard time, the computer calculates the precise orientation of the measuring point. The present invention is not limited by time and the position of the sun, can calibrate the coordinates of the equipment conveniently at any time, and can quickly display the precise orientation, and the precision can be increased to 1/10 degree or 1/100 degree, which can meet the needs of modern scientific research, military And the needs of industrial production and other fields.
Description
本发明涉及一种测定天文方位的方法,特别是一种全新的,方位的精确测定方法。The invention relates to a method for determining astronomical orientation, in particular to a brand-new method for accurately determining orientation.
在当今科学技术高度发达的时代,在科研、军事、运输以及其他工业生产等许多领域中,都需要对某个物体或地点的精确方位与精确高度及时地测得数据。例如要测量飞机、火箭、导弹等飞行物,每一个瞬间在天空中的位置及其变化,就要不断测出其方位、高度,以研究其速度及变化。再如移动式车载雷达等设备,每到达一个新的地点,需要迅速调整自己的座标系统,以便精确测量目标的方位和高度。又例如在天文观测研究中,移动式天文望远镜到达一个新观测点时,需要在尽可能短的时间内投入观测,设备的调整也需要有精确的方位与高度显示。其中方位确定以后,根据水平线和仰角即可确定高度,所以技术上较复杂的是方位的测定。现有技术常用的方位测定法有三种:一是使用指南针确定南北线,但既使采用最精密的指南针,其精度只能达到1度左右。二是采用正午时刻的日影线确定方位,其精度也只有几十分,该方法还要受天气情况的制约。许多技术领域的方位测定要求精确到1/10度或1/100度,这两种方法都无法实现。第三种方法是测定北极星的方位以推算出测点的方位。该方法精度虽然较高,但必须在夜间进行,白天无法作业,在时间紧迫的情况下,该方法不能满足需要。In today's era of highly developed science and technology, in many fields such as scientific research, military affairs, transportation and other industrial production, it is necessary to measure the precise position and height of an object or place in a timely manner. For example, to measure the position and changes of flying objects such as airplanes, rockets, and missiles in the sky at every moment, it is necessary to continuously measure their azimuth and altitude to study their speed and changes. Another example is the mobile vehicle radar and other equipment, each time it reaches a new location, it needs to quickly adjust its own coordinate system in order to accurately measure the target's azimuth and height. Another example is in astronomical observation research, when a mobile astronomical telescope arrives at a new observation point, it needs to be put into observation in the shortest possible time, and the adjustment of the equipment also needs to have accurate azimuth and altitude display. Among them, after the azimuth is determined, the altitude can be determined according to the horizontal line and elevation angle, so the technically more complicated is the determination of azimuth. There are three kinds of azimuth determination methods commonly used in the prior art: the one is to use a compass to determine the north-south line, but even if the most precise compass is used, its accuracy can only reach about 1 degree. The second is to use the shadow line at noon to determine the azimuth, and the accuracy is only a few tens of points, and this method is also restricted by the weather conditions. Azimuth determination in many technical fields requires an accuracy of 1/10 degree or 1/100 degree, which cannot be achieved by these two methods. The third method is to determine the azimuth of Polaris to deduce the azimuth of the measuring point. Although the accuracy of this method is high, it must be carried out at night and cannot be operated during the day. In the case of tight time, this method cannot meet the needs.
本发明提供一种全新的方位的精确测定方法,可以将测量精度提高到1/10度或1/100度,其测量时间也可以不限于正午或夜间,可以随时、方便地测定出精确的方位,使方位测定的方便程度与精确程度都能满足现代科研、军事以及工业生产等领域的需要。The present invention provides a brand-new method for accurately measuring azimuth, which can increase the measurement accuracy to 1/10 degree or 1/100 degree, and the measurement time is not limited to noon or night, and the precise azimuth can be determined conveniently at any time , so that the convenience and accuracy of azimuth determination can meet the needs of modern scientific research, military and industrial production and other fields.
完成上述发明任务的技术方案是:一种全新的方位的精确测定方法,包括以下工作步骤:The technical solution for completing the task of the above invention is: a brand-new method for accurately measuring orientation, comprising the following working steps:
将成像系统指向太阳,采集太阳图象,Point the imaging system to the sun to collect solar images,
根据太阳图象读出其方位值,Read out its azimuth value according to the sun image,
将太阳的方位值输入计算机,Input the azimuth value of the sun into the computer,
由GPS系统向计算机输入观测点的座标与标准时间,The coordinates and standard time of the observation point are input into the computer by the GPS system,
计算机内事先存储有计算太阳座标的天文软件和观测归算软件,计算机根据该时间太阳座标值,与测量得到的太阳座标值之差,计算出测点的精确方位。The astronomical software and observation reduction software for calculating the solar coordinates are stored in the computer in advance, and the computer calculates the precise orientation of the measuring point according to the difference between the solar coordinate value at that time and the measured solar coordinate value.
上述计算结果可以通过显示系统显示出来。这里所说的“成像系统”包括图象采集装置和成像装置,图象采集装置可以采用简易光学望远镜、军用炮镜或对目镜略加改装的导星镜等,甚至一个简单的透镜也可构成图像采集装置。成像装置包括划有分划线的毛玻璃和数字式摄象头等。采集太阳图象的方法可以是:将太阳成象于毛玻璃中心,再由座标指示系统读出其方位值;或者是由数字摄象头拍摄太阳图象,由计算机处理后,得到图象中心座标,由座标指示系统读出方位值。前者的精度可优于0.1度;后者的精度可优于0.01度。显示该结果的装置可以采用码盘、编码器或刻度盘,可按不同的精度要求选择。The above calculation results can be displayed by the display system. The "imaging system" mentioned here includes an image acquisition device and an imaging device. The image acquisition device can use a simple optical telescope, a military gunscope or a guide mirror with a slight modification to the eyepiece, etc., or even a simple lens. Image acquisition device. The imaging device includes frosted glass with reticles and a digital camera. The method of collecting the sun image can be: the sun is imaged in the center of the ground glass, and then the coordinate indicating system reads out its azimuth value; or the sun image is taken by a digital camera, and the image center is obtained after being processed by a computer. Coordinates, the orientation value is read out by the coordinate indicating system. The accuracy of the former can be better than 0.1 degree; the accuracy of the latter can be better than 0.01 degree. The device for displaying the result can use a code disc, an encoder or a dial, which can be selected according to different precision requirements.
本发明提供的这种全新的方位精确测定方法,可以不受时间限制,只要天空中出现太阳,不管其处于什么位置,都可以随时、方便地校准设备的座标,且动作快捷,几十分钟即可完成校验工作,校准后设备的方向及高度的指向即可显示精确方位与高度,精度可以提高到1/10度或1/100度,其方便程度与精确程度都能满足现代科研、军事以及工业生产等领域的需要。The brand-new precise measurement method of azimuth provided by the present invention is not limited by time, as long as the sun appears in the sky, no matter what position it is in, the coordinates of the equipment can be calibrated conveniently at any time, and the action is fast, within tens of minutes The calibration work can be completed. After calibration, the direction and altitude of the equipment can display the precise azimuth and altitude, and the accuracy can be increased to 1/10 degree or 1/100 degree. Its convenience and accuracy can meet modern scientific research, The needs of military and industrial production and other fields.
现结合附图与实施例做进一步说明。Further description will now be made in conjunction with the accompanying drawings and embodiments.
图1为本发明工作流程图。Fig. 1 is the working flow chart of the present invention.
实施例1,参照图1:一种全新的方位的精确测定方法,包括以下工作步骤:将成像系统中的图象采集装置——简易光学望远镜指向太阳,采集太阳图象,将太阳成象于划有分划线的毛玻璃中心,再由座标指示系统根据太阳图象读出其方位值。将太阳的方位值输入计算机,同时由GPS系统向计算机输入观测点的座标与标准时间。计算机内事先存储有计算太阳座标的天文软件和观测归算软件,计算机根据该时间太阳座标值,与测量得到的太阳座标值之差,计算出测点的精确方位。方位值由码盘显示,精度为0.1度。Embodiment 1, with reference to Fig. 1: the accurate measuring method of a kind of brand-new azimuth comprises the following working steps: the image acquisition device in the imaging system---simple and simple optical telescope is pointed to the sun, gathers solar image, and the sun image is in The center of the frosted glass with a reticle is read out by the coordinate indicating system according to the sun image. Input the azimuth value of the sun into the computer, and at the same time input the coordinates and standard time of the observation point into the computer from the GPS system. The astronomical software and observation reduction software for calculating the solar coordinates are stored in the computer in advance, and the computer calculates the precise orientation of the measuring point according to the difference between the solar coordinate value at that time and the measured solar coordinate value. The azimuth value is displayed by the code disc with an accuracy of 0.1 degrees.
实施例2,将成像系统中的图象采集装置——军用炮镜指向太阳,由成像装置——数字式摄象头采集太阳图象并输入计算机,由计算机处理后,得到图象中心座标,由座标指示系统读出方位值。同时由GPS系统向计算机输入观测点的座标与标准时间,计算机根据该时间太阳座标值,与测量得到的太阳座标值之差,计算出测点的精确方位。方位值由编码器显示,精度为0.01度。Embodiment 2, pointing the image acquisition device in the imaging system-the military gun mirror to the sun, collecting the sun image by the imaging device-the digital camera and inputting it into the computer, after being processed by the computer, the coordinates of the center of the image are obtained , read out the azimuth value from the coordinate indicating system. At the same time, the GPS system inputs the coordinates and standard time of the observation point to the computer, and the computer calculates the precise orientation of the observation point according to the difference between the solar coordinate value at this time and the measured solar coordinate value. The bearing value is displayed by the encoder with an accuracy of 0.01 degrees.
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CN102722183A (en) * | 2012-06-15 | 2012-10-10 | 中国科学院安徽光学精密机械研究所 | Image tracking system and image tracking algorithm for double-cylinder multi-FOV (field of view) sun photometer |
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CN1332176C (en) * | 2005-06-07 | 2007-08-15 | 中国科学院紫金山天文台 | Space-target real-time astronomical positioning method |
CN100451550C (en) * | 2005-11-25 | 2009-01-14 | 中国科学院上海光学精密机械研究所 | High precision polarized light navigator |
NO323440B1 (en) * | 2006-04-28 | 2007-05-07 | Sunsim As | Interactive indication of directions in images |
JP2008281552A (en) * | 2007-04-09 | 2008-11-20 | Seiko Epson Corp | First positioning output position calculation determination method, program, storage medium, positioning device, and electronic device |
CN100592231C (en) * | 2008-03-05 | 2010-02-24 | 中国科学院国家天文台 | All-day navigation method and system |
CN103630116B (en) | 2013-10-10 | 2016-03-23 | 北京智谷睿拓技术服务有限公司 | Image acquisition localization method and image acquisition locating device |
CN103900538B (en) * | 2014-04-14 | 2017-03-01 | 中国科学院国家天文台 | The method that ccd detector is used for Astrometric Telescope accurate measurement star place |
CN106546231A (en) * | 2016-10-08 | 2017-03-29 | 深圳市金立通信设备有限公司 | A kind of method and terminal for realizing compass functional |
CN115655249A (en) * | 2022-10-21 | 2023-01-31 | 维沃移动通信有限公司 | Compass calibration method and device, electronic equipment and readable storage medium |
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CN102722183A (en) * | 2012-06-15 | 2012-10-10 | 中国科学院安徽光学精密机械研究所 | Image tracking system and image tracking algorithm for double-cylinder multi-FOV (field of view) sun photometer |
CN102722183B (en) * | 2012-06-15 | 2014-03-12 | 中国科学院安徽光学精密机械研究所 | Image tracking system and image tracking algorithm for double-cylinder multi-FOV (field of view) sun photometer |
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