光电工程
光電工程
광전공정
OPTO-ELECTRONIC ENGINEERING
2013年
4期
45-51
,共7页
王东鹤%王喜军%何昕%魏仲慧%张磊
王東鶴%王喜軍%何昕%魏仲慧%張磊
왕동학%왕희군%하흔%위중혜%장뢰
光波%大气折射%分层%精密修正
光波%大氣摺射%分層%精密脩正
광파%대기절사%분층%정밀수정
light waves%atmospheric refraction%stratification%precision correction
准确获取光学测量中目标的角度是实现高精度的靶场光学测量的关键之一,而大气折射是影响最终计算目标角度的重要因素,需采用适当的方法计算得到目标的准确角度值.本文以分层处理为出发点,对影响大气折射率的主要因素气压、气温、湿度分别采用气压分层模型,气温分层模型,湿度分层模型,以大气折射率模型和接近靶场实际的大气实测数据为基础,根据斯涅耳折射定律和大气光路方程,建立了一种基于分层处理的光波大气折射精密修正方法.利用实际的星体观测实验数据对文中方法和常用的其它方法进行了比较,将处理得到的数据与星体真值进行比较;另外利用实际的靶场测量数据进行了对比处理,两种实验结果都能够说明本文中的分层处理方法可以实现更高精度的修正,可以最终提高光测设备的测量精度.
準確穫取光學測量中目標的角度是實現高精度的靶場光學測量的關鍵之一,而大氣摺射是影響最終計算目標角度的重要因素,需採用適噹的方法計算得到目標的準確角度值.本文以分層處理為齣髮點,對影響大氣摺射率的主要因素氣壓、氣溫、濕度分彆採用氣壓分層模型,氣溫分層模型,濕度分層模型,以大氣摺射率模型和接近靶場實際的大氣實測數據為基礎,根據斯涅耳摺射定律和大氣光路方程,建立瞭一種基于分層處理的光波大氣摺射精密脩正方法.利用實際的星體觀測實驗數據對文中方法和常用的其它方法進行瞭比較,將處理得到的數據與星體真值進行比較;另外利用實際的靶場測量數據進行瞭對比處理,兩種實驗結果都能夠說明本文中的分層處理方法可以實現更高精度的脩正,可以最終提高光測設備的測量精度.
준학획취광학측량중목표적각도시실현고정도적파장광학측량적관건지일,이대기절사시영향최종계산목표각도적중요인소,수채용괄당적방법계산득도목표적준학각도치.본문이분층처리위출발점,대영향대기절사솔적주요인소기압、기온、습도분별채용기압분층모형,기온분층모형,습도분층모형,이대기절사솔모형화접근파장실제적대기실측수거위기출,근거사열이절사정률화대기광로방정,건립료일충기우분층처리적광파대기절사정밀수정방법.이용실제적성체관측실험수거대문중방법화상용적기타방법진행료비교,장처리득도적수거여성체진치진행비교;령외이용실제적파장측량수거진행료대비처리,량충실험결과도능구설명본문중적분층처리방법가이실현경고정도적수정,가이최종제고광측설비적측량정도.
@@@@To accurately obtain the optical measurement of the angle of the target is one of the keys to achieve high-precision result in optical measurement applications. The atmospheric refraction is an important factor to affect the final calculation of the target angle, so appropriate method should be used to calculate the accurate angle of the target. Main factors affecting the atmospheric refractive index:pressure, temperature and humidity are processed separately with the hierarchical model, the temperature stratification model and humidity hierarchical model. Based on atmospheric refractive index model and actual measured data, according to Snell's law of refraction and atmospheric optical path equation, a precision correction method based on hierarchical processing of the light waves of atmospheric refraction is established. The method of this paper and other methods commonly used are compared with the data of stars observed. Additionally, the actual range measurement data is used to compare different methods. Results of both the experiments show that method of this paper can achieve more precise correction and ultimately improve the measurement accuracy of optical measurement equipments.