CN103353922B - A kind of OTF observes scan method - Google Patents
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Abstract
本发明涉及一种OTF观测扫描方法,该方法将一个扫描区域分成若干行,每次扫描多个相间隔的行,进行多次的隔行扫描,完成整个扫描区域的扫描。采用隔行扫描方法,在天线扫描速度、采样间隔、观测参考点时间间隔等参数相同的情况下,一次扫描能快速覆盖一个区域,减小望远镜系统性能和天气变化等因素对整个区域分布的影响;隔行扫描的结果在做重网格化处理时,一个网格化区域内相邻几行的数据使用的参考点是不同时间观测的,不同行的参考点是独立的,不同行的参考点的积分时间之和为参考点的有效积分时间,所以对参考点的积分时间可以用逐行扫描时的1/k,k为一个扫描区域的扫描次数。
The invention relates to an OTF observation scanning method, which divides a scanning area into several lines, scans a plurality of spaced lines each time, performs multiple interlaced scanning, and completes scanning of the entire scanning area. Using the interlaced scanning method, in the case of the same parameters such as antenna scanning speed, sampling interval, and observation reference point time interval, one scan can quickly cover an area, reducing the influence of factors such as telescope system performance and weather changes on the distribution of the entire area; When the results of interlaced scanning are re-grid, the reference points used by adjacent rows of data in a grid area are observed at different times, the reference points of different rows are independent, and the reference points of different rows The sum of the integration time is the effective integration time of the reference point, so the integration time for the reference point can be 1/k of the progressive scanning, k is the number of scans of a scanning area.
Description
技术领域 technical field
本发明涉及射电天文望远镜领域,具体涉及一种OTF观测扫描方法。 The invention relates to the field of radio astronomical telescopes, in particular to an OTF observation and scanning method.
背景技术 Background technique
OTF(On The Fly)是射电望远镜的一种观测方法,天线以恒定的速率对指定的区域进行扫描,而不对单个格点进行跟踪,多个源点可以共用参考点和黑体校准,节约时间;由于整个区域被快速的扫描,系统性能和天气随时间的变化对观测的影响就会比较小。 OTF (On The Fly) is an observation method for radio telescopes. The antenna scans the specified area at a constant rate without tracking a single grid point. Multiple source points can share reference points and blackbody calibration, saving time; Since the entire area is quickly scanned, changes in system performance and weather over time will have less impact on observations.
为了避免由于采样不够而导致信息的丢失,OTF扫描参数有一些限制,如相邻两个扫描行的间距不能大于“Nyquist间隔”;采样间隔,即单次积分时间,它应该大于接收机后端获取一组有效数据所需要的最短时间;采样间隔内天线扫过的距离要求跟行间距接近。 In order to avoid the loss of information due to insufficient sampling, there are some restrictions on OTF scanning parameters, such as the distance between two adjacent scanning lines cannot be greater than the "Nyquist interval"; the sampling interval, that is, the single integration time, should be greater than the receiver backend The minimum time required to obtain a set of valid data; the distance scanned by the antenna within the sampling interval must be close to the line spacing.
OTF观测的过程中进行了很密集的空间采样,这些采样点不一定是等间隔分布,需要进一步的重网格化处理(regrid),以获取通常形式的格点数据。 In the process of OTF observation, very dense spatial sampling is carried out. These sampling points are not necessarily equally spaced, and further regrid processing (regrid) is required to obtain grid point data in the usual form.
传统的扫描方式是把一个扫描区域分成若干行,从一个方向开始逐行扫描(如图1), 对于一个比较大的扫描区域,要想很快的扫描完一遍,就要加快扫描速度,加快扫描速度意味着缩短每个点的积分时间;缩短每个点的积分时间意味着单次扫描的数据regrid后每个网格点积分时间短,噪声大,需要多遍扫描;缩短每行的扫描时间意味着天线频繁掉头,不利于提高观测效率;如果扫描速度慢,完成一次扫描的时间较长,不利于减小望远镜系统性能和天气变化对观测的影响。 The traditional scanning method is to divide a scanning area into several lines, and start scanning line by line from one direction (as shown in Figure 1). Scanning speed means shortening the integration time of each point; shortening the integration time of each point means that the integration time of each grid point is short after the data regrid of a single scan, and the noise is large, requiring multiple scans; shortening the scan of each row Time means that the antenna turns around frequently, which is not conducive to improving observation efficiency; if the scanning speed is slow, it will take a long time to complete a scan, which is not conducive to reducing the impact of telescope system performance and weather changes on observation.
另外,对参考点的积分时间是有限制的,太长会浪费时间,降低观测效率,太短会增大噪声;多长时间观测一次参考点也受接收机稳定性、俯仰角变化量等因素制约,间隔太长会导致谱线基线不平,太短会浪费时间;regrid时某个网格点的值由此点附近一定范围内的采样点的数据,按照该采样点距网格点的距离用某个函数进行加权,通常采用gaussian函数;加权的这些点对参考点的有效积分时间与的对源的有效积分时间相等为最佳。如果这个范围内的点共用一个参考点,那么对参考点的有效积分就是单次参考点的积分时间,单次参考点的积分时间就要等于对源的有效积分时间。 In addition, the integration time of the reference point is limited, too long will waste time and reduce the observation efficiency, too short will increase the noise; how long to observe the reference point is also affected by factors such as receiver stability, pitch angle change, etc. Constraints, if the interval is too long, the baseline of the spectral line will be uneven, and if it is too short, it will waste time; when regrid, the value of a certain grid point is the data of sampling points within a certain range near this point, according to the distance between the sampling point and the grid point Use a certain function for weighting, usually using a gaussian function; the effective integration time of these weighted points to the reference point is equal to the effective integration time of the source. If the points in this range share a reference point, then the effective integration of the reference point is the integration time of a single reference point, and the integration time of a single reference point must be equal to the effective integration time of the source.
如何在不加快扫描速度的情况下,快速对整个区域进行一次覆盖,减小系统性能和天气变化等因素对整个区域分布的影响;如何在不增大噪声水平的前提下,减小对参考点的积分时间,提高观测效率,成为需要解决的技术问题。 How to quickly cover the entire area without increasing the scanning speed, and reduce the influence of system performance and weather changes on the distribution of the entire area; how to reduce the impact on the reference point without increasing the noise level The integration time and improving the observation efficiency have become technical problems that need to be solved.
发明内容 Contents of the invention
本发明的目的在于克服现有技术的缺陷,提供一种能快速覆盖整个区域,对参考点的积分时间小的OTF观测扫描方法,提高了观测效率。 The purpose of the present invention is to overcome the defects of the prior art, provide an OTF observation and scanning method that can quickly cover the entire area, and has a short integration time for the reference point, and improves the observation efficiency.
实现本发明目的的技术方案是:一种OTF观测扫描方法,将一个扫描区域分成若干行,每次扫描多个相间隔的行,进行多次的隔行扫描,完成整个扫描区域的扫描。 The technical solution for realizing the purpose of the present invention is: an OTF observation scanning method, which divides a scanning area into several lines, scans a plurality of spaced lines each time, performs multiple interlaced scanning, and completes the scanning of the entire scanning area.
所述OTF观测扫描方法,具体包括下列步骤: Described OTF observation scanning method specifically comprises the following steps:
S1.计算扫描一个区域总行数:n=扫描范围÷扫描行间距 S1. Calculate the total number of lines scanned in an area: n = scan range ÷ scan line spacing
S2.设定扫描次数k, 计算每次扫描行数x:x=n/k,计算结果向上取整数; S2. Set the number of scans k, calculate the number of lines x for each scan: x=n/k, and round up the calculation result to an integer;
S3.根据设定的参考点观测时间间隔和扫描一行所用时间,计算出扫描多少行后,需观测一次参考点; S3. According to the set reference point observation time interval and the time used for scanning one line, after calculating how many lines to scan, the reference point needs to be observed once;
S4.计算第i行的扫描遍数m,i=1,2……n,m=i/x,计算结果向上取整数; S4. Calculate the scan times m of the i-th row, i=1, 2...n, m=i/x, and round up the calculation result to an integer;
S5.计算扫描第i行时,实际扫描的行数y: S5. Calculate the number of rows y actually scanned when scanning the i-th row:
y=(i-1-x*(m-1))*k+m; y=(i-1-x*(m-1))*k+m;
S6.如果实际扫描的行数y达到需观测参考点的间隔行数,则观测参考点; S6. If the number of lines y actually scanned reaches the number of interval lines required to observe the reference point, then observe the reference point;
S7.从第y行开始继续扫描; S7. Continue scanning from the yth row;
S8. 重复执行步骤S4-S7,至达到设定扫描遍数k,结束。 S8. Steps S4-S7 are repeatedly executed until the set scanning times k is reached, and the process ends.
本发明的有益效果是:①采用隔行扫描方法,在天线扫描速度、采样间隔、观测参考点时间间隔等参数相同的情况下,一次扫描能快速覆盖一个区域,重网格化处理后一个位置的谱线是多次结果平均,每次时间相隔较长,一个网格化范围内的点分布在不同时间段,所以能减小望远镜系统性能和天气变化等因素对整个区域分布的影响;②隔行扫描的结果在做重网格化处理时,一个网格化区域内相邻几行的数据使用的参考点是不同时间观测的,不同行的参考点是独立的,不同行的参考点的积分时间之和为参考点的有效积分时间,所以对参考点的积分时间可以用逐行扫描时的1/k,k为一个扫描区域的扫描次数。 The beneficial effects of the present invention are as follows: 1. By adopting the interlaced scanning method, under the condition that the parameters such as antenna scanning speed, sampling interval, and observation reference point time interval are the same, one scan can quickly cover an area, and the data of a position after regrid processing The spectral line is the average of multiple results, and each time is separated by a long time. The points in a gridded range are distributed in different time periods, so it can reduce the influence of factors such as telescope system performance and weather changes on the distribution of the entire area; ②Interlacing When the scanning results are regrid, the reference points used by adjacent rows of data in a gridded area are observed at different times, the reference points of different rows are independent, and the integration of the reference points of different rows The sum of time is the effective integration time of the reference point, so the integration time of the reference point can be 1/k of the progressive scanning, k is the number of scans of a scanning area.
附图说明 Description of drawings
图1是本发明的现有技术中逐行扫描示意图 ; Fig. 1 is a schematic diagram of progressive scanning in the prior art of the present invention;
图2是本发明实施例1的隔行扫描示意图 ; Fig. 2 is the interlaced scanning schematic diagram of embodiment 1 of the present invention;
图3是本发明的流程图 。 Fig. 3 is a flowchart of the present invention.
具体实施方式 detailed description
如图2所示,一种OTF观测隔行扫描方法,将一个扫描区域的n行分成3次扫描,第一次扫描1、4、7……行,第二次扫描2、5、8……行,第三次扫描3、6、9……行。 As shown in Figure 2, an OTF observation interlaced scanning method divides n lines of a scanning area into 3 scans, the first scan is 1, 4, 7... lines, and the second scan is 2, 5, 8... Line, the third scan 3, 6, 9... lines.
如图3所示,OTF观测隔行扫描方法具体包括以下步骤: As shown in Figure 3, the OTF observation interlaced scanning method specifically includes the following steps:
S1.计算扫描一个区域总行数:n=扫描范围÷扫描行间距 S1. Calculate the total number of lines scanned in an area: n = scan range ÷ scan line spacing
S2.设定扫描次数k, 计算每次扫描行数x:x=n/k,计算结果向上取整数; S2. Set the number of scans k, calculate the number of lines x for each scan: x=n/k, and round up the calculation result to an integer;
S3.根据设定的参考点观测时间间隔和扫描一行所用时间,计算出扫描多少行后,需观测一次参考点; S3. According to the set reference point observation time interval and the time used for scanning one line, after calculating how many lines to scan, the reference point needs to be observed once;
S4.计算第i行的扫描遍数m,i=1,2……n,m=i/x,计算结果向上取整数; S4. Calculate the scan times m of the i-th row, i=1, 2...n, m=i/x, and round up the calculation result to an integer;
S5.计算扫描第i行时,实际扫描的行数y: S5. Calculate the number of rows y actually scanned when scanning the i-th row:
y=(i-1-x*(m-1))*k+m; y=(i-1-x*(m-1))*k+m;
S6.如果实际扫描的行数y达到需观测参考点的间隔行数,则观测参考点; S6. If the number of lines y actually scanned reaches the number of interval lines required to observe the reference point, then observe the reference point;
S7.从第y行开始继续扫描; S7. Continue scanning from the yth row;
S8. 重复执行步骤S4-S7,至达到设定扫描遍数k,结束。 S8. Steps S4-S7 are repeatedly executed until the set scanning times k is reached, and the process ends.
扫描次数k根据扫描一个区所用总时间和接收机稳定性、后期数据处理要求等因素综合考虑,一般分2-4次。 The number of scans k is generally divided into 2-4 times based on the overall consideration of factors such as the total time used to scan an area, receiver stability, and post-data processing requirements.
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CN101976297A (en) * | 2010-09-30 | 2011-02-16 | 中国科学院国家天文台 | Processing method of moon brightness temperature data observed by foundation single antenna |
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US6484306B1 (en) * | 1999-12-17 | 2002-11-19 | The Regents Of The University Of California | Multi-level scanning method for defect inspection |
CN1520179A (en) * | 2003-02-03 | 2004-08-11 | 三星电子株式会社 | Method and appts. for coding/decoding interlaced scanning video signal |
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