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风云静止气象卫星的图像导航和大气运动矢量(特邀)

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本文介绍了风云静止气象卫星图像配准定位和大气运动矢量的算法。图像配准和定位统称图像导航,是图像观测的重要步骤。图像导航的数学模型须要在每一个观测瞬间,获得卫星的位置以及从卫星指向观测目标物的矢量。风云二号是自旋稳定卫星,它用图像上地球影像中心位置的时间序列求解卫星的姿态,并对图像进行定位。风云四号是三轴稳定卫星,存在影响卫星对地观测光路指向的因素。所以风云四号卫星的观测和图像定位,通过更加密切的星地协同操作实现。在连续的图像上追踪云的运动,获得大气运动矢量。大气运动矢量所在的高度,是用物理方法确定的。从密实云上行的辐射,主要来自云。把云的温度与数值预报模式中各个高度层面上的温度相匹配,得到云的高度。从半透明的薄云上行的辐射,一部分来自云体,其余部分来自云下的背景。云的半透明程度主要和云的密实程度有关,所以在窗区和半透明通道的卫星测值之间,存在线性相关关系。据此可以更加准确地计算出云的半透明程度,以及在云的高度上大气的温度。半透明云高度计算方法的改善,提高了大气运动矢量的精度。
Image Navigation and Atmospheric Motion Vectors for FY Geosynchronous Meteorological Satellites(Invited)
Significance Geosynchronous meteorological satellites,operating at an altitude of 35800 km above the equator,frequently capture images of the Earth disk.The successive image derives atmospheric motion vectors.They have been monitoring various weather systems continuously and are indispensable tools for precise weather forecasting.Our study shows image navigation and atmospheric motion vector algorithms for FY geosynchronous meteorological satellites.Progress The geosynchronous satellite takes Earth observation pixel by pixel.The observation pixels are assembled to form images.The image assembling contains two major components:image registration and image navigation.Image registration refers to the process of ensuring that each pixel within an image is correctly aligned with its nominal Earth location within a specified accuracy,which measures pointing stability.Image navigation involves determining the location of each pixel within an image in terms of Earth latitude and longitude,which measures absolute pointing accuracy.Both image registration and navigation are critical steps in image assembling,impacting all subsequent data processing procedures and product quality.Due to the satellite's considerable distance from Earth,the accuracy of attitude determination significantly affects image navigation quality.Precise image navigation requires accurate measurement of the position and the attitude of the satellite at any observation time.The FY-2 satellite has a spin-stabilized attitude.The Earth position within the image is used to determine the attitude of the satellite.The time series of the satellite orientation relative to the centerline of the Earth disk provides information on the attitude parameter in the north-south direction.The angle between the sun and the Earth serves as a reference for aligning the Earth observation pixels position in the scan line together with the attitude parameter in the east-west direction.The solution to the image navigation model requires the parameters to be well-defined,measured,transformed,and applied within appropriate coordinate systems while maintaining correct astronomical relationships.The FY-4 satellite,on the other hand,is three-axis stabilized.The additional moving equipment causes uneven shifts of the satellite.Moreover,the satellite is heated at the side facing the sun which makes uneven temperature distribution in the spacecraft with diurnal variation.Both factors affect the orientation of the observation vectors.Thus,the operation of the image registration and navigation for FY-4 rely on the interactions between the satellite and the ground system more closely.The star positions are used to determine the attitude of the satellite.Using previous observation,the ground system estimates future positions of the stars and possible observation vector orientation errors caused by uneven heating.Those parameters are transmitted to the satellite,which then adjusts its attitude to maintain stability and compensate for observation vector deviations.Tracing clouds and other features in the successive images provides an estimation of the scene's displacements,which represent atmospheric motion vectors.The height of the wind vector is determined with a physical method.For opaque clouds,the infrared window brightness temperature reflects the upwelling radiation energy from the cloud.The cloud level is identified at the height where the feature brightness temperature fits the forecast model temperature.For semi-transparent clouds,a part of the energy is from the cloud,the other part is from the background under the cloud.Since the semi-transparent status is only related to cloud density,not related to the observation wavelengths.In the cloudy region,there is a linear relationship between observations from the window and absorption channels.By using observations from both the window and absorption channels,the portions of upwelling radiation energy from the cloud and from the background are well estimated.This approach needs the locations of both the cloudy and the cloud-free pixels,and the upwelling energy from those locations.Based on the moving status of the pixels during the feature tracing stage,the cloudy and the cloud-free pixels are well separated.The upwelling radiation energy from the under cloud background is estimated with data from the nearest cloud-free pixels.This algorithm provides a more accurate estimation of semi-transparent cloud heights.Conclusions and Prospects By using algorithms introduced in our study achieve more accurate observation,navigation,and wind derivation.For both FY-2 and FY-4,all the parameters are produced automatically and routinely without any manual operation.The accuracy of image navigation reaches pixel level.The image navigation accuracy approaches pixel level.The accuracy and distribution of the atmospheric vectors are also improved.Meteorological satellite data processing involves a long chain including many steps simulating the radiation transmission process from the observation objective to the sensor.A deep understanding and the precise expression of the real situation in the data processing algorithm ensure better product quality.

geosynchronous meteorological satelliteimage registrationimage navigationatmospheric motion vector

许健民、陆风、杨磊、张晓虎、曹赟、张其松、商建

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中国气象局国家卫星气象中心,北京 100081

静止气象卫星 图像配准 图像定位 大气运动矢量

国家自然科学基金国家自然科学基金国家重点研发计划资助国家重点研发计划资助

40275007402750362021YFB39004002021YFB3900402

2024

光学学报
中国光学学会 中国科学院上海光学精密机械研究所

光学学报

CSTPCD北大核心
影响因子:1.931
ISSN:0253-2239
年,卷(期):2024.44(18)