CN112945384B - A Data Preprocessing Method for Multi-Angle Polarization Satellites - Google Patents

A Data Preprocessing Method for Multi-Angle Polarization Satellites Download PDF

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CN112945384B
CN112945384B CN202110222941.XA CN202110222941A CN112945384B CN 112945384 B CN112945384 B CN 112945384B CN 202110222941 A CN202110222941 A CN 202110222941A CN 112945384 B CN112945384 B CN 112945384B
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谢一凇
李正强
伽丽丽
葛邦宇
朱思峰
侯梦雨
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Abstract

本发明公开了一种适用于高分五号卫星多角度偏振成像仪(DPC/GF‑5)及类似星载传感器的L1级辐射/偏振观测和观测几何的多角度数据重组匹配方法,包括整轨影像数据分块技术;参考像元选择方法;基于观测天顶角和观测方位角联合的邻近像元观测角度匹配方法;逐像元多角度数据定序重组技术。本发明提出的辐射/偏振观测数据的多角度重组匹配方法,能够解决国产多角度偏振卫星影像因裁切和拼接导致的数据跳变和条带问题,克服其对大气、地表参数反演造成的影响,有效提升定量反演精度。

Figure 202110222941

The invention discloses a multi-angle data recombination and matching method for L1 radiation/polarization observation and observation geometry suitable for the Gaofen-5 satellite multi-angle polarization imager (DPC/GF-5) and similar on-board sensors, comprising the following steps: Orbit image data block technology; reference pixel selection method; adjacent pixel observation angle matching method based on the combination of observation zenith angle and observation azimuth angle; pixel-by-pixel multi-angle data sequencing and reorganization technology. The multi-angle recombination and matching method for radiation/polarization observation data proposed by the invention can solve the problems of data jumping and banding caused by cropping and splicing of domestic multi-angle polarization satellite images, and overcome the problems caused by the inversion of atmospheric and surface parameters. It can effectively improve the quantitative inversion accuracy.

Figure 202110222941

Description

一种多角度偏振卫星的数据预处理方法A Data Preprocessing Method for Multi-Angle Polarization Satellites

技术领域technical field

本发明涉及遥感科学、图像处理领域的卫星影像多角度数据重组匹配方法,适用于多角度偏振卫星的多角度辐射/偏振数据的重组匹配方法,特别是国产高分辨率卫星。The invention relates to a satellite image multi-angle data recombination and matching method in the fields of remote sensing science and image processing, and is suitable for the multi-angle radiation/polarization data recombination and matching method of multi-angle polarization satellites, especially domestic high-resolution satellites.

背景技术Background technique

卫星遥感对地成像观测技术是目前能够实现地球陆地、海洋、大气等多个圈层快速探测的最为有效的手段之一,其具有的空间连续覆盖、大范围信息探测、瞬时成像、高空间分辨率等探测优势能够满足气候、环境、资源、生态等多个不同领域对地球关键参数定量和定性探测的需求,因此成为近几十年来的研究热点和重要发展方向。在遥感定量化应用中,遥感影像的成像质量和影像预处理效果是决定遥感参数反演精度的重要影响因素,例如,辐射校正精度、光谱校正精度、几何配准精度、大气校正效果等,均是对遥感定量反演结果产生不可忽视影响的重要指标。Satellite remote sensing earth imaging observation technology is currently one of the most effective means to achieve rapid detection of the earth's land, ocean, atmosphere and other layers. It has continuous spatial coverage, large-scale information detection, instantaneous imaging, and high spatial resolution. The detection advantages such as rate can meet the needs of quantitative and qualitative detection of key parameters of the earth in different fields such as climate, environment, resources, ecology, etc., so it has become a research hotspot and an important development direction in recent decades. In remote sensing quantitative applications, the imaging quality and image preprocessing effect of remote sensing images are important factors that determine the inversion accuracy of remote sensing parameters. For example, radiometric correction accuracy, spectral correction accuracy, geometric registration accuracy, atmospheric correction effect, etc. It is an important indicator that has a non-negligible impact on the quantitative inversion results of remote sensing.

大气颗粒物是指地球大气中的固体或液体颗粒悬浮物质,包括来源于自然产生的沙尘、海盐、火山灰、生物气溶胶等粒子,以及人为活动排放产生的碳气溶胶、二次颗粒物等,粒径范围跨越达到5个数量级,成为地球复杂巨系统的重要组成部分。大气颗粒物含量及其光学、物理、化学、辐射等方面的特性,在空气质量、气候变化、对地观测等国家社会发展层面和科研领域均有重要影响,因此是卫星遥感探测的重点目标之一。Atmospheric particulate matter refers to solid or liquid particulate suspended matter in the earth's atmosphere, including naturally occurring particles such as sand dust, sea salt, volcanic ash, and biological aerosols, as well as carbon aerosols, secondary particulate matter, etc. The diameter range spans up to 5 orders of magnitude, and it has become an important part of the complex giant system of the earth. Atmospheric particulate matter content and its optical, physical, chemical, radiation and other characteristics have an important impact on air quality, climate change, earth observation and other national social development levels and scientific research fields, so it is one of the key goals of satellite remote sensing detection. .

大气颗粒物卫星遥感探测已有几十年的发展历程,历经单通道探测、多通道探测、强度探测、偏振探测、多角度探测等多项技术的建立和完善。代表性的大气颗粒物探测卫星传感器包括:Aqua卫星上的MODIS传感器具有可见光至短波红外探测通道,发展了较成熟的气溶胶暗目标反演算法和深蓝反演算法;搭载在Terra卫星上的MISR传感器能够实现目标像元多个角度下的观测,相应发展了适配其多角度他探测的气溶胶反演算法;CALIPSO卫星搭载了主动激光雷达CALIOP,通过接收回波信号获得气溶胶垂直方向的信息;静止卫星以凝视方式探测地球特定区域,能够获取高时相的区域气溶胶监测结果,代表性传感器包括韩国的GOCI/COMS、日本的AHI/HIMAWARI-8,以及我国高分系列的PMS/GF-4。Atmospheric particulate matter satellite remote sensing detection has been developed for decades, and has undergone the establishment and improvement of many technologies such as single-channel detection, multi-channel detection, intensity detection, polarization detection, and multi-angle detection. Representative atmospheric particulate matter detection satellite sensors include: the MODIS sensor on the Aqua satellite has a visible light to short-wave infrared detection channel, and a relatively mature aerosol dark target retrieval algorithm and deep blue retrieval algorithm have been developed; the MISR sensor mounted on the Terra satellite It can realize the observation of the target pixel from multiple angles, and the aerosol inversion algorithm adapted to its multi-angle detection has been developed accordingly; the CALIPSO satellite is equipped with the active lidar CALIOP, and the information of the vertical direction of the aerosol is obtained by receiving the echo signal. ; Geostationary satellites detect specific areas of the earth by staring, and can obtain high-phase regional aerosol monitoring results. Representative sensors include GOCI/COMS in South Korea, AHI/HIMAWARI-8 in Japan, and PMS/GF in my country's high score series. -4.

上述卫星传感器的一个共同的局限是观测维度相对较少,因此仅能获得气溶胶光学厚度参数,而对其他的关键参数例如吸收性、粒径尺度等大气颗粒物物理特性的探测能力则尚未形成较成熟的技术方法。法国PARASOL卫星上搭载的POLDER-3传感器具有多角度、多波段、强度、偏振探测能力,被认为是目前气溶胶探测能力最强、最全面也是最有效的星载探测方式,得到了研究人员的广泛关注。A common limitation of the above satellite sensors is that the observation dimension is relatively small, so only the aerosol optical depth parameter can be obtained, and the detection ability of other key parameters such as absorption, particle size and other physical properties of atmospheric particles has not yet been developed. Proven technical approach. The POLDER-3 sensor mounted on the French PARASOL satellite has multi-angle, multi-band, intensity, and polarization detection capabilities. It is considered to be the most powerful, comprehensive and effective spaceborne detection method for aerosol detection. extensive attention.

2018年5月我国发射了高分辨率对地观测系统中的高分五号卫星,其上搭载了可见光-短波红外高光谱相机、全谱段光谱成像仪两个对地观测传感器,以及多角度偏振成像仪、大气环境红外甚高光谱分辨率探测仪、大气主要温室气体监测仪、大气痕量气体差分吸收光谱仪四个先进大气观测载荷,是我国高分卫星系列中的环境监测旗舰卫星。其中,多角度偏振成像仪(Directional Polarization Camera, DPC)是我国首个具有多谱段(覆盖可见光至近红外)、多角度(9-12个角度成像)、偏振(探测3个偏振分量)的星载宽视场成像仪(幅宽1850公里),具有探测气溶胶、云、水汽等大气成分信息的专用探测通道,同时兼顾陆地和海洋环境的探测能力。DPC通过在沿轨方向连续高速成像,实现目标像元最多12个角度下的偏振和强度辐射信息探测,同时通过滤光片及偏振片轮的转动和耦合获得不同光谱通道上的偏振和强度辐射信号。中国发射的DPC/GF-5与法国POLDER-3传感器采用相似的先进探测机制,具有光谱、角度、强度、偏振多个维度的高精度探测能力,并且空间分辨率达到3.3 km,比POLDER-3分辨率(6*7 km)高出1倍,能够满足城市尺度精细化大气探测、区域污染传输通道监测等重要应用对大气产品高空间分辨率的要求。In May 2018, my country launched the Gaofen-5 satellite in the high-resolution earth observation system. It is equipped with a visible light-shortwave infrared hyperspectral camera, a full-spectrum spectral imager, two earth observation sensors, and a multi-angle. Polarization Imager, Atmospheric Environment Infrared Very High Spectral Resolution Detector, Atmospheric Main Greenhouse Gas Monitor, Atmospheric Trace Gas Differential Absorption Spectrometer Four advanced atmospheric observation payloads are the flagship satellites for environmental monitoring in my country's high-resolution satellite series. Among them, the Directional Polarization Camera (DPC) is the first satellite in my country with multi-spectral (covering visible light to near-infrared), multi-angle (9-12 angle imaging), and polarization (detecting 3 polarization components). The carrier wide field of view imager (width 1850 kilometers) has a dedicated detection channel for detecting atmospheric composition information such as aerosols, clouds, and water vapor, and takes into account the detection capabilities of terrestrial and marine environments. DPC realizes the detection of polarization and intensity radiation information at a maximum of 12 angles of the target pixel through continuous high-speed imaging along the track, and obtains polarization and intensity radiation on different spectral channels through the rotation and coupling of the filter and the polarizer wheel. Signal. The DPC/GF-5 launched by China adopts a similar advanced detection mechanism to the French POLDER-3 sensor. It has high-precision detection capabilities in multiple dimensions of spectrum, angle, intensity, and polarization, and has a spatial resolution of 3.3 km, which is higher than that of POLDER-3. The resolution (6*7 km) is 1 times higher, which can meet the high spatial resolution requirements of atmospheric products for important applications such as urban-scale refined atmospheric detection and regional pollution transmission channel monitoring.

但是,目前的数据用于大气参数定量反演时,效果并不理想。However, when the current data is used for quantitative inversion of atmospheric parameters, the effect is not ideal.

发明内容SUMMARY OF THE INVENTION

经研究发现,DPC与POLDER-3/PARASOL类似,在标准化数据产品(L1级)生产时,将多个观测角度的辐射和偏振观测数据,依据对地观测顺序进行了裁切、调整和拼接,以保证更完整的观测信息集中在排序靠前的观测角度(同一景成像的数据观测角相同)中,提高数据的连续性和可读性。但也由此带来一个问题,即对应的一幅遥感图像实际上并不是某个角度下传感器成像时“同时”获取的一景影像,而是多个角度下观测数据依据一定规则进行裁切和拼接之后的结果。这种方式会导致在图像中的裁切接边处出现错位,主要表现为对应的观测天顶角、观测方位角,以及强度和偏振辐射等具有角度变化特性的观测量,其数值产生较大的跳动。在涉及到影像的空间域处理时,这种数据组织形式不利于定量反演,特别是对于观测几何较为敏感的气溶胶参数反演,可能导致反演结果出现空间不连续的异常条带。因此,需对DPC及类似传感器的L1级数据产品进行重新处理,恢复传感器拍摄时“同时”成像的单景数据,以提升卫星遥感数据定量化反演和处理的精度。The study found that DPC is similar to POLDER-3/PARASOL. During the production of standardized data products (L1 level), the radiation and polarization observation data of multiple observation angles were cut, adjusted and spliced according to the order of earth observation. In order to ensure that more complete observation information is concentrated in the observation angles that are ranked first (the data observation angles of the same scene imaging are the same), the continuity and readability of the data are improved. But this also brings a problem, that is, a corresponding remote sensing image is not actually a scene image obtained by the sensor at a certain angle, but the observation data from multiple angles is cropped according to certain rules. and the result after splicing. This method will lead to misalignment at the cropped edge in the image, which is mainly manifested in the corresponding observation zenith angle, observation azimuth angle, and observational quantities with angular variation characteristics such as intensity and polarized radiation. beating. When it comes to the spatial domain processing of images, this form of data organization is not conducive to quantitative inversion, especially for the inversion of aerosol parameters that are sensitive to observation geometry, which may lead to spatially discontinuous abnormal bands in the inversion results. Therefore, it is necessary to reprocess the L1-level data products of DPC and similar sensors to restore the single-scene data imaged by the sensor "simultaneously" during shooting, so as to improve the accuracy of quantitative inversion and processing of satellite remote sensing data.

目前,尚未见有针对此类载荷的多角度数据重组匹配方法和技术的研究或报道。迫切需要发展一种面向国产多角度偏振卫星应用需求的多角度遥感数据重组匹配方法,为提高大气参数定量化反演精度提供重要的数据基础。At present, there is no research or report on the method and technology of multi-angle data reorganization and matching for such payloads. There is an urgent need to develop a multi-angle remote sensing data recombination and matching method for the application requirements of domestic multi-angle polarization satellites, which provides an important data basis for improving the quantitative inversion accuracy of atmospheric parameters.

本发明的目的是提供一种提高大气参数定量反演准确性的多角度偏振卫星的数据预处理方法;具体技术方案为:The object of the present invention is to provide a data preprocessing method for multi-angle polarization satellites that improves the accuracy of quantitative inversion of atmospheric parameters; the specific technical scheme is:

一种多角度偏振卫星的数据预处理方法,包括以下步骤:A data preprocessing method for a multi-angle polarization satellite, comprising the following steps:

1)读取整轨数据中的观测角度个数信息,判断有效的总行数和总列数,将获取的整轨卫星数据进行分割得到初始分块;1) Read the number of observation angles in the entire orbit data, determine the effective total number of rows and columns, and divide the obtained orbit satellite data to obtain initial blocks;

2)判断所述初始分块中是否存在至少一列完整的数据列;如果存在,作为待处理数据块,执行步骤4)2) Determine whether there is at least one complete data column in the initial block; if there is, as a data block to be processed, go to step 4)

3)将初始分块按行进行分割,分割为若干存在至少一列完整的数据列的子块;所述子块作为待处理数据块;3) The initial block is divided by row, and divided into several sub-blocks with at least one complete data column; the sub-blocks are used as the data blocks to be processed;

4)提取所述待处理数据块中的观测数据;4) Extract the observation data in the data block to be processed;

5)从所述完整的数据列中一个端点为起点向另一端点依次进行遍历,当前点作为参考像元,下一个点作为待处理像元,构成参考像元-待处理像元对;所有参考像元-待处理像元对组成参考列邻近像元对数据集;5) From one end point in the complete data column as the starting point to the other end point, the current point is used as the reference pixel, and the next point is used as the to-be-processed pixel to form a reference pixel-to-be-processed pixel pair; all Reference pixel-to-be-processed pixel pair constitutes a reference column adjacent pixel pair dataset;

6)以所述完整的数据列中每个点为起点,向左依次进行遍历,当前点作为参考像元,下一个点作为待处理像元,构成参考像元-待处理像元对;所有参考像元-待处理像元对组成左邻近像元对数据集;向右依次遍历,采用相同方法组成右邻近像元对数据集;6) Take each point in the complete data column as the starting point, and traverse to the left in turn, the current point is used as the reference pixel, and the next point is used as the pixel to be processed, forming a reference pixel-to-be-processed pixel pair; all The reference pixel-to-be-processed pixel pair constitutes a left adjacent pixel pair dataset; traverse to the right in turn, and use the same method to form a right adjacent pixel pair dataset;

7)将参考像元所有观测角度的数据与待处理像元当前观测角度的数据采用公式(1)和公式(2)计算,判断构成的每个所述参考像元-待处理像元对是否匹配;7) Calculate the data of all observation angles of the reference pixel and the data of the current observation angle of the pixel to be processed using formula (1) and formula (2), and determine whether each of the reference pixel-to-be-processed pixel pairs is formed. match;

δz=VZAref,i-VZAtest (1);δz=VZA ref,i -VZA test (1);

δa=VAAref,i-VAAtest (2);δa=VAAref ,i - VAAtest (2);

其中,δz为观测天顶角差值,i为观测角度序号,VZAref,i为参考像元的第i个观测天顶角,VZAtest为待处理像元当前观测角度的观测天顶角,δa为观测方位角差值,VAAref,i为参考像元的第i个观测方位角,VAAtest为待处理像元当前观测角度的观测方位角;Among them, δz is the observation zenith angle difference, i is the observation angle serial number, VZA ref,i is the ith observation zenith angle of the reference pixel, VZA test is the observation zenith angle of the current observation angle of the pixel to be processed, δa is the observation azimuth difference, VAA ref,i is the ith observation azimuth of the reference pixel, and VAA test is the observation azimuth of the current observation angle of the pixel to be processed;

δz小于观测天顶角阈值Tz且δa小于观测方位角Ta;则判断为匹配,进入步骤9);If δz is smaller than the observation zenith angle threshold Tz and δa is smaller than the observation azimuth angle Ta; then it is judged to be a match and go to step 9);

否则,判断为不匹配;进入步骤8)Otherwise, it is judged that it does not match; go to step 8)

8)选取待处理像元的下一个观测角度的数据与参考像元通过步骤7)进行匹配,直至匹配;8) Select the data of the next observation angle of the pixel to be processed and match the reference pixel through step 7) until it matches;

9)该待处理像元作为参考像元,匹配的观测角度作为参考像元的起始观测角度;9) The pixel to be processed is used as the reference pixel, and the matching observation angle is used as the starting observation angle of the reference pixel;

10)采用步骤7)相同的方法处理所述参考列邻近像元对数据集、所述左邻近像元对数据集和所述右邻近像元对数据集,直至数据集中所有的参考像元-待处理像元对完成匹配;10) Use the same method as step 7) to process the reference column adjacent pixel pair dataset, the left adjacent pixel pair dataset and the right adjacent pixel pair dataset until all reference pixels in the dataset- The pixel pair to be processed is matched;

11)将经匹配处理的所有参考像元的各观测角度对应的观测数据代替原数据,完成多角度定序重组。11) Replace the original data with the observation data corresponding to each observation angle of all reference pixels that have been matched and complete the multi-angle sequence reorganization.

进一步,所述Tz的范围为0.5-1.0°;Ta的范围为1.0-2.0°。Further, the range of Tz is 0.5-1.0°; the range of Ta is 1.0-2.0°.

进一步,所述观测数据包括地理坐标域信息和各波段、各角度的数据域信息。Further, the observation data includes geographic coordinate domain information and data domain information of each band and each angle.

进一步,所述地理坐标域信息包括地表高程、海陆掩膜、经纬度、格网行列号。Further, the geographic coordinate domain information includes surface elevation, sea and land mask, longitude and latitude, and grid row and column numbers.

进一步,所述数据域信息包括辐射亮度、偏振Stokes分量、观测几何。Further, the data domain information includes radiance, polarization Stokes component, and observation geometry.

进一步,还包括以下步骤:Further, the following steps are also included:

12) 根据待处理像元的起始观测角度序号AnS和有效观测角度数N,计算观测角度移动次序步长:12) According to the starting observation angle sequence number AnS and the effective observation angle number N of the pixel to be processed, calculate the observation angle moving order step size:

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将起始观测角度序号AnS及以后的数据与起始观测角度序号AnS以前的数据换位,对数据进行重组,计算参考像元和待处理像元各观测角度下VZA和VAA的总体差值,判断是否所有观测角度均已满足匹配:Transpose the data of the starting observation angle serial number AnS and later with the data before the starting observation angle serial number AnS, reorganize the data, and calculate the overall difference between VZA and VAA at each observation angle of the reference pixel and the pixel to be processed. Determine whether all observation angles have been matched:

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其中,i表示观测角度序号(共N个),下标ref和test分别表示参考像元和待处理像元,Tz为观测天顶角阈值和Ta为观测方位角阈值;Among them, i represents the observation angle serial number (N in total), the subscripts ref and test represent the reference pixel and the pixel to be processed, respectively, Tz is the observation zenith angle threshold and Ta is the observation azimuth angle threshold;

如果满足,则数据校核成功;如果不满足,则对新的数据进行步骤1)至步骤12)的处理;发现并剔除异常数据所在的观测角度。If it is satisfied, the data verification is successful; if it is not satisfied, the new data is processed from step 1) to step 12); the observation angle where the abnormal data is found and eliminated.

本发明通过对数据进行标准行数的数据分块,组成参考像元和待处理像元对,逐像元定序重组及调整等步骤对卫星数据进行处理;该种多角度数据重组匹配方法有效、稳定,处理结果能够满足大气参数定量反演的数据基础需求。The invention processes the satellite data by dividing the data into blocks with a standard number of rows, forming a pair of reference pixels and pixels to be processed, and sorting, reorganizing and adjusting pixel by pixel; the multi-angle data reorganization and matching method is effective , stable, and the processing results can meet the data basis requirements for quantitative inversion of atmospheric parameters.

附图说明Description of drawings

图1为本发明提出的多角度数据重组匹配方法流程;Fig. 1 is the multi-angle data reorganization and matching method process flow proposed by the present invention;

图2为实施例中根据参考像元选择需要进一步进行数据分块的过程示意图;2 is a schematic diagram of the process of further performing data segmentation according to the selection of reference pixels in the embodiment;

图3为实施例中经过标准行数数据分块的DPC/GF-5的L1级数据影像(670 nm波段、第一个观测角度的Stokes矢量I、Q、U,以及观测天顶角、观测方位角);Figure 3 is the L1-level data image of DPC/GF-5 with standard line number data blocks in the embodiment (670 nm band, Stokes vectors I, Q, U of the first observation angle, and observation zenith angle, observation Azimuth);

图4为实施例中经过多角度数据重组匹配后的影像数据(670 nm波段、第一个观测角度的Stokes矢量I、Q、U,以及观测天顶角、观测方位角)。Figure 4 shows the image data after multi-angle data recombination and matching in the embodiment (670 nm band, Stokes vectors I, Q, U of the first observation angle, and observation zenith angle and observation azimuth).

具体实施方式Detailed ways

下面利用实施例对本发明进行更全面的说明。本发明可以体现为多种不同形式,并不应理解为局限于这里叙述的示例性实施例。The present invention will be more fully described below by means of examples. The present invention may be embodied in many different forms and should not be construed as limited to the exemplary embodiments set forth herein.

以国产多角度偏振卫星传感器DPC/GF-5实际观测数据为例,描述本发明的具体实施方式。本发明采用的实施例数据是DPC/GF-5观测数据(数据时间:2019年5月5日,数据空间范围:中国东部地区);根据本发明的方法利用计算机对数据进行处理。本发明方法技术流程图见图1。Taking the actual observation data of the domestic multi-angle polarization satellite sensor DPC/GF-5 as an example, the specific implementation of the present invention is described. The example data used in the present invention is DPC/GF-5 observation data (data time: May 5, 2019, data space range: Eastern China); the data is processed by a computer according to the method of the present invention. The technical flow chart of the method of the present invention is shown in FIG. 1 .

(1)整轨影像数据分块(1) The whole track image data is divided into blocks

首先,读取整轨数据中的观测角度个数信息,通过无效值或填充值判断该轨数据的有效总行数和总列数。其次,设定标准分块行数(可根据计算机处理性能设定),按照设定值对整轨数据进行逐波段、逐角度的分块处理。DPC/GF-5实施例数据采用标准行数(500行)进行数据分块的部分示例结果见图3,包括670 nm波段偏振Stokes矢量I670、Q670、U670、观测天顶角VZA、观测方位角VAA。First, read the observation angle number information in the entire track data, and judge the valid total number of rows and columns of the track data through invalid values or fill values. Secondly, set the standard block number (which can be set according to the processing performance of the computer), and perform block-by-band and angle-by-angle block processing on the entire track data according to the set value. Figure 3 shows some examples of the data of the DPC/GF-5 example using the standard number of lines (500 lines) to block the data, including the polarization Stokes vectors I670, Q670, U670 in the 670 nm band, the observation zenith angle VZA, and the observation azimuth angle. VAA.

传统数据分块处理完成上述步骤即可,但对于本发明需要最终实现的多角度数据重组这一目标,分块后的影像还可能面临多种不利情况,特别是高纬度地区(接近南北极)的影像易出现不规则形状,例如影像存在尖角边缘、影像长宽比过大导致边缘处出现多列无效数据等,需要进一步进行针对性的处理。在标准行数分块的基础上,本发明的一个创新之处在于根据后续参考像元选择的需要进一步进行分块处理,避免数据重组时参考像元出现无效结果。判断初步分块后的各数据块是否满足参考像元选择的要求,即分块后的影像至少存在一个完整的数据列,该列中所有的像元均为有效数据。注意到DPC/GF-5实施例分块数据中不存在完整的数据列,因此需继续对该数据块进行分块处理,根据数据块实际情况,采用二分法进一步按行分块,满足上、下两个子块中均至少存在一列完整的数据列。DPC/GF-5实施例数据进一步进行数据分块的过程示意图见图2。当然,也可以根据需要进行三分或更多的按行分割。分割后,参考列尽量靠近所有完整列的中部。The traditional data block processing can complete the above steps, but for the goal of multi-angle data reorganization that the present invention needs to finally achieve, the image after block may also face various unfavorable situations, especially in high latitude areas (close to the North and South Pole) The images are prone to irregular shapes, such as sharp edges in the images, and multiple columns of invalid data appearing at the edges due to an excessively large aspect ratio of the images, which requires further targeted processing. On the basis of the standard row number block, an innovation of the present invention is that the block processing is further performed according to the need of subsequent reference pixel selection, so as to avoid invalid results of the reference pixel during data reorganization. It is judged whether each data block after preliminary segmentation meets the requirements of reference pixel selection, that is, there is at least one complete data column in the divided image, and all the pixels in this column are valid data. It is noted that there is no complete data column in the block data of the DPC/GF-5 embodiment, so it is necessary to continue to perform block processing on the data block. At least one complete column of data exists in the next two sub-blocks. Figure 2 shows a schematic diagram of the process of further dividing the data in the DPC/GF-5 embodiment into data blocks. Of course, three or more row-wise splits can also be performed as needed. After splitting, the reference column is as close as possible to the middle of all complete columns.

最后,根据上述分块结果提取相应的观测数据,包括各波段、各角度的辐射亮度、偏振Stokes分量、观测几何等数据域信息,以及地表高程、海陆掩膜、经纬度、格网行列号等地理坐标域信息。最后,按照原L1级整轨数据文件存储格式,将上述提取的分块数据信息写入新的分块数据文件,完成数据分块处理。Finally, the corresponding observation data are extracted according to the above block results, including data domain information such as radiance of each band and angle, polarization Stokes component, observation geometry, etc. Coordinate field information. Finally, according to the original L1 level full track data file storage format, the above-mentioned extracted block data information is written into a new block data file to complete the data block processing.

(2)分块数据参考像元选择(2) Block data reference pixel selection

本发明提出的多角度数据重组匹配的核心思路是为分块影像中每个像元建立一一对应的参考像元—待处理像元对,将待处理像元的多角度排序按照参考像元进行调整。除影像边缘外,每个像元既是参考像元又是待处理像元,某像元的多角度次序由其参考像元决定,同时也决定了下一个待处理像元的多角度次序。因此,分块数据参考像元的正确选择是本发明实现的重要先决条件。该步骤需要解决的核心问题是如何为影像中每个像元确定其参考像元。The core idea of multi-angle data reorganization and matching proposed by the present invention is to establish a one-to-one corresponding reference pixel-to-be-processed pixel pair for each pixel in the segmented image, and to sort the multi-angle order of the to-be-processed pixels according to the reference pixel make adjustments. Except for the image edge, each pixel is both a reference pixel and a pixel to be processed. The multi-angle order of a pixel is determined by its reference pixel, and it also determines the multi-angle order of the next pixel to be processed. Therefore, the correct selection of the reference pixels of the block data is an important prerequisite for the realization of the present invention. The core problem to be solved in this step is how to determine the reference cell for each cell in the image.

传统上对于遥感图像进行逐像元遍历的方法一般有两种。一种是从角点起始沿纵、横两个方向进行遍历,但由于DPC/GF-5此类载荷特殊的成像方式和数据投影特点,分块后的影像数据并非标准矩形或正方形,而是近似平行四边形或梯形的四边形,这种方法会遇到大量的无效数据情况而导致处理失效。另一种是从影像中间任意选择像元起始进行上下左右四个方向的遍历,遇无效值判定为到达影像边缘而终止,这种方法虽然能够建立所有像元的参考像元—待处理像元对,但会使后续多角度重组处理更为复杂和易错,且计算量较大。为解决这一难题,本发明创新性提出了一种基于“点”(参考像元)—“列”(参考数据列)—“行”(每一行)双循环的参考像元遍历方法。首先,根据分块数据确定起始参考像元seed。由于前述分块步骤中需满足至少存在一列完整数据列的分块策略,起始参考像元从满足该要求的所有列{Ci}中进行选择,一般取{Ci}的中间列(Cm)的最底行(Rb)的像元,作为起始参考像元seed(行号为Rb,列号为Cm)。之后,从seed开始向上逐像元对邻近像元进行遍历,构建Cm列每一行像元的参考像元—待处理像元对,即(Rb, Cm)ßà(Rb-1, Cm)、(Rb-1, Cm)ßà(Rb-2, Cm)、…,依次类推。之后,以参考数据列Cm的每一行像元为参考,分别向左和向右逐像元遍历,构建相应的参考像元—待处理像元对,即(Rb, Cm)ßà(Rb, Cm-1)和(Rb, Cm)ßà(Rb, Cm+1)、(Rb-1, Cm)ßà(Rb-1, Cm-1)和(Rb-1, Cm)ßà(Rb-1, Cm+1)、…,依次类推。最后,建立该数据块中所有像元的参考像元—待处理像元的对应关系,形成邻近像元对数据集。Traditionally, there are two methods for traversing remote sensing images pixel by pixel. One is to traverse vertically and horizontally from the corner point. However, due to the special imaging method and data projection characteristics of such loads as DPC/GF-5, the divided image data is not a standard rectangle or square, but It is a quadrilateral that approximates a parallelogram or trapezoid. This method will encounter a large number of invalid data conditions and cause processing failure. The other is to randomly select a pixel in the middle of the image to traverse in four directions, up, down, left, and right. In case of an invalid value, it is determined to reach the edge of the image and terminate. Although this method can establish a reference pixel for all pixels—the image to be processed However, it will make the subsequent multi-angle recombination processing more complicated and error-prone, and the amount of calculation is large. To solve this problem, the present invention innovatively proposes a reference pixel traversal method based on a double cycle of "point" (reference pixel) - "column" (reference data column) - "row" (each row). First, the starting reference pixel seed is determined according to the block data. Since the segmentation strategy that at least one complete data column exists in the foregoing segmentation step needs to be satisfied, the starting reference pixel is selected from all columns {C i } that satisfy this requirement, and generally the middle column (C i } of {C i } is selected. m ) of the bottom row (R b ) of the cell, as the starting reference cell seed (row number R b , column number C m ). After that, traverse the adjacent pixels from the seed upwards pixel by pixel, and construct the reference pixel-to-be-processed pixel pair for each row of cells in column C m , namely (R b , C m )ßà(R b -1, C m ), (R b -1, C m )ßà(R b -2, C m ), … and so on. After that, take each row of pixels in the reference data column C m as a reference, traverse left and right pixel by pixel, and construct the corresponding reference pixel-to-be-processed pixel pair, namely (R b , C m )ßà( R b , C m -1) and (R b , C m )ßà(R b , C m +1), (R b -1, C m )ßà(R b -1, C m -1) and ( R b -1, C m )ßà(R b -1, C m +1), … and so on. Finally, the corresponding relationship between the reference pixel and the pixel to be processed of all the pixels in the data block is established, and the adjacent pixel pair dataset is formed.

(3)邻近像元观测角度匹配(3) Matching of observation angles of adjacent pixels

形成邻近像元对数据集后,对每一组参考像元—待处理像元进行观测角度匹配,其目的是找到待处理像元的起始观测角度序号(与参考像元一致),从而为后续多角度数据定序重组处理提供初始值。DPC/GF-5传感器在同一个观测角度下成像时,观测天顶角VZA变化很小,而经过前述裁切和拼接后,在拼接边缘处(非同一观测角度下成像)会发生明显跳变,因此可以通过设定观测天顶角的跳变阈值来判断是否为同一观测角度下成像。然而,DPC/GF-5数据每个像元有9-12个观测角度,VZA按照由大到小再到大的变化顺序,基本呈现以天底方向VZA为最小值的前视、后视对称变化分布,仅依靠观测天顶角数值难以进行正确匹配。After the adjacent pixel pair dataset is formed, the observation angle matching is performed for each group of reference pixels-to-be-processed pixels. Subsequent multi-angle data reordering processing provides initial values. When the DPC/GF-5 sensor is imaged at the same observation angle, the observed zenith angle VZA changes very little, but after the aforementioned cropping and splicing, there will be obvious jumps at the edge of the splicing (imaging at different observation angles) , so it can be determined whether the imaging is under the same observation angle by setting the jump threshold of the observation zenith angle. However, each pixel of the DPC/GF-5 data has 9-12 observation angles, and the VZA basically presents front-sight and rear-sight symmetry with the nadir direction VZA as the minimum value according to the order of change from large to small and then large. Variation distribution, it is difficult to correctly match only relying on the observed zenith angle value.

本发明提出了一种新的技术思路解决上述问题,在观测天顶角判识匹配的基础上加入了观测方位角进行辅助判识。首先,根据分块数据中观测天顶角VZA和观测方位角VAA数值变化规律,设定VZA和VAA的跳变阈值Tz和Ta,即参考像元和待处理像元之间VZA差异小于Tz且VAA差异小于Ta时,判定待处理像元与参考像元为同观测角度成像,未发生裁切和拼接。之后,再将参考像元其他观测角度下的VZA和VAA与待处理像元第一个观测角度下VZA和VAA进行匹配(即未发生跳变)的情况,并根据匹配情况进行如下处理:j如果只存在一个匹配结果,则该匹配角度即为待处理像元的起始观测角度AnS;k如果存在超过一个匹配结果,则选择δz和δa总体较小的匹配角度作为待处理像元的起始观测角度AnS;l如果不存在匹配结果,说明与参考像元相比,与待处理像元第一个观测角度不是同一个观测角度,改变待处理像元的观测角度重复上述步骤继续判断,参考像元各观测角度下的VZA和VAA是否存在与待处理像元第二个观测角度下VZA和VAA匹配,以查找待处理像元的起始观测角度。匹配成功后,待处理像元的数据替换下一个参考像元-待处理像元对中参考像元的数据,进行匹配。匹配时,先进行参考列邻近像元对数据集中所有参考像元-待处理像元对的匹配;再以处理后的参考列数据为基准,分别对所述左邻近像元对数据集和所述右邻近像元对数据集中的所有参考像元-待处理像元对进行处理。最终,建立每一个待处理像元的起始观测角度序号,用于后续逐像元定序重组。跳变计算公式为:The present invention proposes a new technical idea to solve the above-mentioned problems, and adds the observation azimuth angle to assist in the identification on the basis of the identification and matching of the observation zenith angle. First, according to the variation law of the observed zenith angle VZA and the observed azimuth angle VAA in the block data, the jump thresholds Tz and Ta of VZA and VAA are set, that is, the VZA difference between the reference pixel and the pixel to be processed is less than Tz and When the VAA difference is less than Ta, it is determined that the pixel to be processed and the reference pixel are imaged at the same observation angle, and no cropping and splicing occur. After that, match the VZA and VAA at other observation angles of the reference pixel with the VZA and VAA at the first observation angle of the pixel to be processed (that is, there is no jump), and perform the following processing according to the matching situation: j If there is only one matching result, the matching angle is the starting observation angle AnS of the pixel to be processed; if there is more than one matching result k, the matching angle with the overall smaller δz and δa is selected as the starting point of the pixel to be processed. If there is no matching result, it means that compared with the reference pixel, it is not the same observation angle as the first observation angle of the pixel to be processed. Change the observation angle of the pixel to be processed and repeat the above steps to continue the judgment. Check whether the VZA and VAA at each observation angle of the reference pixel match the VZA and VAA at the second observation angle of the pixel to be processed, so as to find the starting observation angle of the pixel to be processed. After the matching is successful, the data of the pixel to be processed replaces the data of the reference pixel in the next reference pixel-to-be-processed pixel pair for matching. When matching, firstly perform the matching of all reference pixel-to-be-processed pixel pairs in the reference column adjacent pixel pair dataset; All reference-to-be-processed cell pairs in the dataset are processed by the right neighbor cell pair described above. Finally, the initial observation angle sequence number of each pixel to be processed is established, which is used for subsequent pixel-by-pixel sequence reorganization. The jump calculation formula is:

δz=VZAref,i-VZAtest (1);δz=VZA ref,i -VZA test (1);

δa=VAAref,i-VAAtest (2);δa=VAAref ,i - VAAtest (2);

(4)逐像元多角度数据定序重组(4) Pixel-by-pixel multi-angle data sequencing and reorganization

确定待处理像元的起始观测角度序号后,即可按照观测天顶角和观测方位角变化规律,顺次对各角度下的数据进行重组。然而,由于有些像元的个别观测角度有所缺失,仅进行顺序重组会导致该缺失角度之后的各角度出现顺次错位。因此,本发明在实际数据处理过程中,采用逐次重组、匹配检测的策略,即每次重组之后进行匹配检测,对剩余尚未匹配的观测角度进行重新处理,发现并剔除异常数据所在的观测角度,直至完成所有有效观测角度的匹配。具体步骤如下:After the initial observation angle serial number of the pixel to be processed is determined, the data at each angle can be reorganized in sequence according to the change rule of the observation zenith angle and the observation azimuth angle. However, due to the missing individual viewing angles for some cells, just doing a sequential reorganization would result in a sequential misalignment of the angles following the missing angle. Therefore, in the actual data processing process of the present invention, the strategy of successive reorganization and matching detection is adopted, that is, matching detection is performed after each reorganization, the remaining unmatched observation angles are reprocessed, and the observation angles where abnormal data are located are found and eliminated. Until all valid observation angles are matched. Specific steps are as follows:

首先,根据待处理像元的起始观测角度序号AnS和有效观测角度数N,计算观测角度移动次序步长:First, according to the initial observation angle sequence number AnS and the effective observation angle number N of the pixel to be processed, calculate the observation angle moving order step size:

Figure 147663DEST_PATH_IMAGE001
Figure 147663DEST_PATH_IMAGE001

将待处理像元的第AnS个观测角度至最后一个观测角度,挪至新数据的前L+1个角度,待处理像元的前AnS-1个角度顺次挪至新数据的第L+2至最后一个角度,完成第一次重组。之后,通过计算参考像元和待处理像元各观测角度下VZA和VAA的总体差值,判断是否所有观测角度均已满足匹配:Move the AnSth observation angle of the pixel to be processed to the last observation angle, move it to the first L+1 angle of the new data, and move the first AnS-1 angle of the pixel to be processed to the L+th angle of the new data. 2 to the last angle to complete the first reorganization. After that, by calculating the overall difference between VZA and VAA at each observation angle of the reference pixel and the pixel to be processed, it is judged whether all the observation angles have satisfied the matching:

Figure 540467DEST_PATH_IMAGE002
Figure 540467DEST_PATH_IMAGE002

Figure 595011DEST_PATH_IMAGE003
Figure 595011DEST_PATH_IMAGE003

其中,i表示观测角度序号(共N个),下标ref和test分别表示参考像元和待处理像元,Tz为观测天顶角阈值和Ta为观测方位角阈值。Among them, i represents the observation angle serial number (N in total), the subscripts ref and test represent the reference pixel and the pixel to be processed, respectively, T z is the observation zenith angle threshold and T a is the observation azimuth threshold.

若仍存在不匹配的观测角度,则进一步根据阈值筛选尚未完成匹配的观测角度,将其中第一个作为新的起始观测角度序号,并重复上述步骤,直至待处理像元的所有观测角度均与参考像元匹配,满足式(4)和式(5),并输出待处理像元观测角度次序调整数组。所述Tz的范围最好为0.5-1.0°;Ta的范围为1.0-2.0°。阈值太低,无法保证完全匹配;阈值太高,计算的耗时会急剧增加。If there are still unmatched observation angles, further filter the unmatched observation angles according to the threshold, take the first one as the new starting observation angle serial number, and repeat the above steps until all the observation angles of the pixel to be processed are Match with the reference pixel, satisfy formula (4) and formula (5), and output the observation angle order adjustment array of the pixel to be processed. The range of Tz is preferably 0.5-1.0°; the range of Ta is 1.0-2.0°. If the threshold is too low, a complete match cannot be guaranteed; if the threshold is too high, the computation time will increase dramatically.

最后,按照该调序数组,将待处理像元各观测角度下的多波段强度辐射、偏振Stokes矢量、观测天顶角、观测方位角、太阳天顶角、太阳方位角等重新写入新的数据文件,完成多角度定序重组。DPC/GF-5实施例分块数据经过逐像元多角度定序重组后的结果见图4,可以看出,原始L1级数据(图3)中因裁切和拼接导致的Stokes矢量I、Q、U影像的跳变已经得到校正,观测天顶角和观测方位角条带已复原为传感器成像时的影像,变化规律符合物理场景,说明本发明提出的多角度数据重组匹配方法有效、稳定,能够满足大气参数定量反演的数据基础需求。Finally, according to the ordered array, rewrite the multi-band intensity radiation, polarization Stokes vector, observation zenith angle, observation azimuth, solar zenith angle, solar azimuth, etc. under each observation angle of the pixel to be processed into a new Data files, complete multi-angle sequencing and reorganization. Figure 4 shows the results of the multi-angle sequencing and reorganization of the block data in the DPC/GF-5 embodiment. It can be seen that the Stokes vector I, The jumps of the Q and U images have been corrected, the observation zenith angle and the observation azimuth angle strips have been restored to the images of the sensor imaging, and the change law conforms to the physical scene, indicating that the multi-angle data reorganization and matching method proposed by the present invention is effective and stable. , which can meet the data base requirements for quantitative inversion of atmospheric parameters.

上述示例只是用于说明本发明,除此之外,还有多种不同的实施方式,而这些实施方式都是本领域技术人员在领悟本发明思想后能够想到的,故,在此不再一一列举。The above examples are only used to illustrate the present invention. In addition, there are many different implementations, and these implementations can be thought of by those skilled in the art after comprehending the idea of the present invention. Therefore, they are not repeated here. an enumeration.

Claims (6)

1. A data preprocessing method for a multi-angle polarized satellite is characterized by comprising the following steps:
1) reading observation angle number information in the whole-orbit data, judging effective total line number and total column number, and segmenting the acquired whole-orbit satellite data to obtain initial blocks;
2) judging whether at least one complete data column exists in the initial block; if yes, as the data block to be processed, executing the step 4)
3) Dividing the initial block into a plurality of sub-blocks with at least one complete data column; the sub-blocks are used as data blocks to be processed;
4) extracting observation data in the data block to be processed;
5) traversing from one end point in the complete data column as a starting point to the other end point in sequence, wherein the current point is used as a reference pixel and the next point is used as a pixel to be processed to form a reference pixel-pixel to be processed pair; all reference pixel-pixel pairs to be processed form a reference column adjacent pixel pair data set;
6) Traversing each point in the complete data column serving as a starting point in sequence leftwards, wherein the current point serves as a reference pixel and the next point serves as a pixel to be processed to form a reference pixel-pixel to be processed pair; all reference pixel-to-be-processed pixel pairs form a left adjacent pixel pair data set; traversing sequentially to the right, and forming a right adjacent pixel pair data set by adopting the same method;
7) calculating the data of all observation angles of the reference pixel and the data of the current observation angle of the pixel to be processed by adopting a formula (1) and a formula (2), and judging whether each formed reference pixel-pixel to be processed pair is matched;
δz=VZAref,i-VZAtest (1);
δa=VAAref,i-VAAtest (2);
wherein, delta z is the difference value of the observation zenith angle, i is the serial number of the observation angle, VZAref,iIs the ith observation of the reference pixelZenith angle, VZAtestThe observation zenith angle of the current observation angle of the pixel to be processed is delta a, the difference value of the observation azimuth angle is VAAref,iIs the i-th observation azimuth, VAA, of the reference pixeltestThe observation azimuth angle of the current observation angle of the pixel to be processed is obtained;
δ z is smaller than the observation zenith angle threshold Tz and δ a is smaller than the observation azimuth angle Ta; judging the matching and entering the step 9);
otherwise, judging as mismatching; entering step 8)
8) Selecting data of a next observation angle of the pixel to be processed and the reference pixel, and matching the data and the reference pixel in the step 7) until the data and the reference pixel are matched;
9) The pixel to be processed is used as a reference pixel, and the matched observation angle is used as an initial observation angle of the reference pixel;
10) processing the reference column adjacent pixel pair data set, the left adjacent pixel pair data set and the right adjacent pixel pair data set by adopting the same method in the step 7) until all reference pixel-to-be-processed pixel pairs in the data sets are matched;
11) and replacing the observation data corresponding to each observation angle of all the reference pixels subjected to matching processing with the original data to finish multi-angle sequencing recombination.
2. The method for pre-processing data for a multi-angle polarized satellite of claim 1, wherein Tz ranges from 0.5 to 1.0 °; ta ranges from 1.0 to 2.0 deg.
3. The method for pre-processing data of a multi-angle polarized satellite according to claim 1, wherein the observation data comprises geographical coordinate domain information and data domain information for each wave band and each angle.
4. The method for preprocessing data of a multi-angle polarized satellite of claim 3, wherein the geographic coordinate domain information comprises surface elevation, sea-land mask, latitude and longitude, grid row and column number.
5. The method for data pre-processing of a multi-angle polarized satellite of claim 3, wherein the data domain information comprises radiance, polarized Stokes components, observation geometry.
6. The method for pre-processing data for a multi-angle polarized satellite of claim 1, further comprising the steps of:
12) calculating the step length of the movement sequence of the observation angle according to the initial observation angle sequence number AnS and the effective observation angle number N of the pixel to be processed:
Figure DEST_PATH_IMAGE001
the data of the initial observation angle sequence number AnS and the subsequent data are transposed with the data of the initial observation angle sequence number AnS, the data are recombined, the overall difference value of VZA and VAA under each observation angle of the reference pixel and the pixel to be processed is calculated, and whether all the observation angles meet the matching condition is judged:
Figure 626431DEST_PATH_IMAGE002
Figure DEST_PATH_IMAGE003
wherein i represents an observation angle sequence number; the number of the observation angles is N, subscripts ref and test respectively represent a reference pixel and a pixel to be processed, Tz is an observation zenith angle threshold value and Ta is an observation azimuth angle threshold value;
if yes, the data check is successful; if not, processing the new data from the step 1) to the step 12); and finding and eliminating the observation angle of the abnormal data.
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