光谱学与光谱分析
光譜學與光譜分析
광보학여광보분석
SPECTROSCOPY AND SPECTRAL ANALYSIS
2013年
12期
3432-3436
,共5页
郝爱花%胡炳樑%白加光%李立波%于涛%李思远
郝愛花%鬍炳樑%白加光%李立波%于濤%李思遠
학애화%호병량%백가광%리립파%우도%리사원
大视场%宽谱段%高分辨率%紫外%成像光谱仪
大視場%寬譜段%高分辨率%紫外%成像光譜儀
대시장%관보단%고분변솔%자외%성상광보의
Large field of view%Wide spectrum%High resolution%Ultraviolet%Imaging spectrometer
紫外-可见光(200~500 nm )成像光谱仪是空间遥感的重要组成部分,本文基于机载紫外-可见成像光谱仪的特殊性和实际应用要求,提出了一种采用面阵CCD的摆扫式成像光谱仪,这样既克服了传统线阵CCD摆扫式成像光谱仪空间分辨率低的缺点,同时又弥补了推扫式成像光谱仪视场范围有限的缺点,能够满足大视场、宽谱段、高分辨率成像光谱仪的应用要求;此外,考虑400~500 nm波段中200~250 nm波段二级光谱的影响和<290 nm的短波区和>310 nm的长波区两个波段相差3个数量级的辐射波动,采用了分波段、分系统的方式独立进行消杂光光谱成像。在系统结构设计方面,本着高性能、低成本的设计理念,选用了两镜同心系统作为望远系统,Czerny-T urner平面光栅结构作为成像光谱仪系统的光学设计方案;设计了一种不使用任何辅助光学元件,全部采用球面镜结构的成像光谱仪。整个系统结构简单、紧凑,性能优良,可行性好。全谱段、全视场调制传递函数值在0.6以上。
紫外-可見光(200~500 nm )成像光譜儀是空間遙感的重要組成部分,本文基于機載紫外-可見成像光譜儀的特殊性和實際應用要求,提齣瞭一種採用麵陣CCD的襬掃式成像光譜儀,這樣既剋服瞭傳統線陣CCD襬掃式成像光譜儀空間分辨率低的缺點,同時又瀰補瞭推掃式成像光譜儀視場範圍有限的缺點,能夠滿足大視場、寬譜段、高分辨率成像光譜儀的應用要求;此外,攷慮400~500 nm波段中200~250 nm波段二級光譜的影響和<290 nm的短波區和>310 nm的長波區兩箇波段相差3箇數量級的輻射波動,採用瞭分波段、分繫統的方式獨立進行消雜光光譜成像。在繫統結構設計方麵,本著高性能、低成本的設計理唸,選用瞭兩鏡同心繫統作為望遠繫統,Czerny-T urner平麵光柵結構作為成像光譜儀繫統的光學設計方案;設計瞭一種不使用任何輔助光學元件,全部採用毬麵鏡結構的成像光譜儀。整箇繫統結構簡單、緊湊,性能優良,可行性好。全譜段、全視場調製傳遞函數值在0.6以上。
자외-가견광(200~500 nm )성상광보의시공간요감적중요조성부분,본문기우궤재자외-가견성상광보의적특수성화실제응용요구,제출료일충채용면진CCD적파소식성상광보의,저양기극복료전통선진CCD파소식성상광보의공간분변솔저적결점,동시우미보료추소식성상광보의시장범위유한적결점,능구만족대시장、관보단、고분변솔성상광보의적응용요구;차외,고필400~500 nm파단중200~250 nm파단이급광보적영향화<290 nm적단파구화>310 nm적장파구량개파단상차3개수량급적복사파동,채용료분파단、분계통적방식독립진행소잡광광보성상。재계통결구설계방면,본착고성능、저성본적설계이념,선용료량경동심계통작위망원계통,Czerny-T urner평면광책결구작위성상광보의계통적광학설계방안;설계료일충불사용임하보조광학원건,전부채용구면경결구적성상광보의。정개계통결구간단、긴주,성능우량,가행성호。전보단、전시장조제전체함수치재0.6이상。
The ultraviolet-visible (UV-Vis 200~500 nm) imaging spectrometer is an important part of space remote sensing . Based on special requirements and practical application of the airborne UV-VIS spectrometer ,a kind of scanning imaging spec-trometer using area array CCD is proposed ,which can meet the application requirements of large field of view ,wide spectrum and high resolution .It overcomes low spatial resolution of traditional line array CCD scanning imaging spectrometer ,and limited field of view of the pushbroom imaging spectrometer .In addition ,dual channel was designed to reduce stray light .400~500 nm band includes two order spectrum for 200~250 nm band ,and variation of radiance from earth between the shorter wavelength (<290 nm) and the longer wavelength (>310 nm) is above three orders of magnitude .In the structure design of the system , the imaging spectrometer is composed of a two-mirror concentric telescope and two Czerny-Turner plane grating imaging spec-trometers .The whole system doesn’t use any additional optical elements in addition to spherical mirrors .The whole system has the advantage of simple structure ,excellent performance ,and very good feasibility .The modulation transfer function value of full spectrum and full field of view is above 0.6 .