光谱学与光谱分析
光譜學與光譜分析
광보학여광보분석
SPECTROSCOPY AND SPECTRAL ANALYSIS
2014年
3期
609-613
,共5页
刘恩超%李新%张艳娜%李文伟%郑小兵
劉恩超%李新%張豔娜%李文偉%鄭小兵
류은초%리신%장염나%리문위%정소병
辐照度仪%Fèry棱镜%音圈电机%陷阱探测器%光学厚度
輻照度儀%Fèry稜鏡%音圈電機%陷阱探測器%光學厚度
복조도의%Fèry릉경%음권전궤%함정탐측기%광학후도
Irradiance-meter%Fèry prism%Voice coil actuator%Trap detector%Optical depth
为了实现对太阳辐射的绝对测量和大气特性的精确反演,研制了光谱覆盖范围在0.4~1.0μm的高精度太阳光谱辐照度仪。太阳辐照度仪采用Fèry棱镜实现入射太阳光的色散,闭环控制光谱扫描机构的方法实现光谱扫描。论文详细介绍了太阳辐照度仪光谱扫描测量部分的设计。给出了Fèry棱镜的设计要求,实现单一元件完成光谱色散;利用陷阱探测器进行光谱采集,保证了测量精度;结合探测器的性能参数,说明了温控的需求和方法;介绍了光谱扫描结构的设计方法,实现了精确的波长定位;给出了音圈电机的参数、稳定性和供电要求,实现了0.025%的波长定位误差。开展室外观测实验,实现了0.4~1.0μm波段的太阳细分光谱扫描测量,并分别与可见-短波红外光谱仪和自动太阳光度计(C E318)进行了对比。结果表明,辐照度仪的光谱扫描测量结果的吸收峰波长值吻合,与C E318全天测量数据的相对偏差小于0.13%,可见波段的光学厚度的相对偏差小于2%,近红外波段的相对偏差小于4%。
為瞭實現對太暘輻射的絕對測量和大氣特性的精確反縯,研製瞭光譜覆蓋範圍在0.4~1.0μm的高精度太暘光譜輻照度儀。太暘輻照度儀採用Fèry稜鏡實現入射太暘光的色散,閉環控製光譜掃描機構的方法實現光譜掃描。論文詳細介紹瞭太暘輻照度儀光譜掃描測量部分的設計。給齣瞭Fèry稜鏡的設計要求,實現單一元件完成光譜色散;利用陷阱探測器進行光譜採集,保證瞭測量精度;結閤探測器的性能參數,說明瞭溫控的需求和方法;介紹瞭光譜掃描結構的設計方法,實現瞭精確的波長定位;給齣瞭音圈電機的參數、穩定性和供電要求,實現瞭0.025%的波長定位誤差。開展室外觀測實驗,實現瞭0.4~1.0μm波段的太暘細分光譜掃描測量,併分彆與可見-短波紅外光譜儀和自動太暘光度計(C E318)進行瞭對比。結果錶明,輻照度儀的光譜掃描測量結果的吸收峰波長值吻閤,與C E318全天測量數據的相對偏差小于0.13%,可見波段的光學厚度的相對偏差小于2%,近紅外波段的相對偏差小于4%。
위료실현대태양복사적절대측량화대기특성적정학반연,연제료광보복개범위재0.4~1.0μm적고정도태양광보복조도의。태양복조도의채용Fèry릉경실현입사태양광적색산,폐배공제광보소묘궤구적방법실현광보소묘。논문상세개소료태양복조도의광보소묘측량부분적설계。급출료Fèry릉경적설계요구,실현단일원건완성광보색산;이용함정탐측기진행광보채집,보증료측량정도;결합탐측기적성능삼수,설명료온공적수구화방법;개소료광보소묘결구적설계방법,실현료정학적파장정위;급출료음권전궤적삼수、은정성화공전요구,실현료0.025%적파장정위오차。개전실외관측실험,실현료0.4~1.0μm파단적태양세분광보소묘측량,병분별여가견-단파홍외광보의화자동태양광도계(C E318)진행료대비。결과표명,복조도의적광보소묘측량결과적흡수봉파장치문합,여C E318전천측량수거적상대편차소우0.13%,가견파단적광학후도적상대편차소우2%,근홍외파단적상대편차소우4%。
In order to measure the radiation of the sun absolutely and retrieve the characterization of the atmosphere precisely ,a high-precision solar spectral irradiance meter working in 0.4~1.0 μm band was developed .A Fèry prism was employed to dis-perse the incident sunlight and a closed-loop control method was adopted for spectral scanning in this solar irradiance meter .The design of spectral scanning measurement was depicted in detail .The design requirements of Fèry prism were given and spectral dispersion was achieved by single element .The trap detectors were used to ensure precise spectral measurement .According to the parameters of the trap detectors ,the demands and method of temperature control were introduced .The design of spectral scanning structure was introduced ,and wavelengths were positioned accurately .The requirements for parameters ,stability and power supply of voice coil actuator were given and the wavelength position error of 0.025% was achieved .Spectral scanning measurement of 0.4~1.0 μm was accomplished in outdoor experiments .A comparison was carried out with visible-short wave infrared spectrometer and auto-sunphotometer (CE318 ) . Results indicate that absorption peak locations of spectral scanning measurement of irradiance meter are correct ,and the relative deviation from CE318 measurements is less than 0.13% for all day , and the relative deviation of optical depth in visible and near infrared band is less than 2% and 5% ,respectively .