地球信息科学学报
地毬信息科學學報
지구신식과학학보
GEO-INFORMATION SCIENCE
2015年
2期
229-235
,共7页
何永健%张娅琳%邱新法%曹芸
何永健%張婭琳%邱新法%曹蕓
하영건%장아림%구신법%조예
ASTER%云顶高度%云迹风%云顶高度解算方法
ASTER%雲頂高度%雲跡風%雲頂高度解算方法
ASTER%운정고도%운적풍%운정고도해산방법
ASTER%cloud-top height%cloud winds%cloud-top height calculation
云顶高度是天气预报、天气监测的重要因子,准确的云顶高度对提高天气分析和数值预报的质量,具有重要的科学意义。立体几何法是公认云顶高度解算精度较高的方法,目前,普遍采用卫星-球心-投影云-真云的平面和球面三角几何关系,以及影像匹配技术解算云顶高度,由于采用了理想椭球体和重投影技术,以及对云移动考虑不足,因此误差较大。本文将数字摄影测量理论与遥感技术相结合,首次将摄影测量共线方程用于云顶高度解算。本文利用ASTER影像,依据相关系数法解求云迹风,并将其引入到摄影测量共线方程中,建立了ASTER影像的云顶高度解算模型,进行了未考虑和考虑风速的云顶高度解算,通过地面点计算,本文解算误差为2个像元(30 m)左右,经与MISR云顶高度产品对比分析,认为该模型解算的考虑风速的云顶高度精度优于MISR解算结果。
雲頂高度是天氣預報、天氣鑑測的重要因子,準確的雲頂高度對提高天氣分析和數值預報的質量,具有重要的科學意義。立體幾何法是公認雲頂高度解算精度較高的方法,目前,普遍採用衛星-毬心-投影雲-真雲的平麵和毬麵三角幾何關繫,以及影像匹配技術解算雲頂高度,由于採用瞭理想橢毬體和重投影技術,以及對雲移動攷慮不足,因此誤差較大。本文將數字攝影測量理論與遙感技術相結閤,首次將攝影測量共線方程用于雲頂高度解算。本文利用ASTER影像,依據相關繫數法解求雲跡風,併將其引入到攝影測量共線方程中,建立瞭ASTER影像的雲頂高度解算模型,進行瞭未攷慮和攷慮風速的雲頂高度解算,通過地麵點計算,本文解算誤差為2箇像元(30 m)左右,經與MISR雲頂高度產品對比分析,認為該模型解算的攷慮風速的雲頂高度精度優于MISR解算結果。
운정고도시천기예보、천기감측적중요인자,준학적운정고도대제고천기분석화수치예보적질량,구유중요적과학의의。입체궤하법시공인운정고도해산정도교고적방법,목전,보편채용위성-구심-투영운-진운적평면화구면삼각궤하관계,이급영상필배기술해산운정고도,유우채용료이상타구체화중투영기술,이급대운이동고필불족,인차오차교대。본문장수자섭영측량이론여요감기술상결합,수차장섭영측량공선방정용우운정고도해산。본문이용ASTER영상,의거상관계수법해구운적풍,병장기인입도섭영측량공선방정중,건립료ASTER영상적운정고도해산모형,진행료미고필화고필풍속적운정고도해산,통과지면점계산,본문해산오차위2개상원(30 m)좌우,경여MISR운정고도산품대비분석,인위해모형해산적고필풍속적운정고도정도우우MISR해산결과。
Cloud-top height is an important factor in weather forecasting and monitoring. Accurate cloud-top height has important scientific significance for improving the quality of both weather analyses and numerical weather prediction. The geometric method to calculate cloud-top height using stereo image pair obtained from meteorological satellites has been recognized as providing relatively high precision, and has practical impor-tance. However, this method does not fully consider cloud movement and typically assumes ideal ellipsoids in theory. Thus, the calculated cloud-top height still has a relatively large error in practice. In this study, cloud-movement speed was introduced into the collinearity equation of photogrammetry. We established a model to cal-culate the cloud-top height from the ASTER images (3B and 3N) with digital photogrammetry and remote sens-ing technology. Firstly, we created a stereo pair from ASTER images obtained on 25th September 2012. Then, the cloud-movement speed was calculated through matching cloud points. Finally, the cloud-top heights with and without consideration of wind speed were both calculated. Compared with ground control points, the model error is determined to be within two pixels (about 30 meter). We further compared our results with MISR products, and found that the cloud-top height determined without using wind speed is consistent with the height obtained from MISR, the difference between them is about 300 meters. Our cloud-top height determined with wind speed considered, however is about 1400 meters higher than that of MISR without wind considered. Marchand and Naud had identified in their research that the cloud-top height obtained from MISR is about 1000 meters lower than Lidar observation. This implies that our results with consideration of wind speed are closer to the Lidar ob-servations. Due to the fact that our method for determining cloud-top height is dependent on the cloud moving speed, and the results with wind speed included have led to a good estimation of cloud-top height, we conclude that the wind speed should be included in algorithms for cloud-top height determination.