Garrison L M, Doda D D, Green A E
Appl Opt. 1979 Mar 15;18(6):850-5. doi: 10.1364/AO.18.000850.
A method has been developed to determine total ozone from multispectral measurements of the direct solar irradiance. The total ozone is determined by a least squares fit to the spectrum between 290 nm and 380 nm. The aerosol extinction is accounted for by expanding it in a power series in wavelength; use of the linear term proved adequate. A mobile laboratory incorporating a sky scanner has been developed and used to obtain data to verify the method. Sun tracking, wavelength setting of the double monochromator, and data acquisition are under control of a minicomputer. Results obtained at Wallops Island, Virginia, and Palestine, Texas, agree well with simultaneous Dobson and Canterbury spectrometer and balloon ECC ozonesonde values. The wavelength calibration of the monochromator and the values for the normalized ozone absorption are the most important factors in an accurate determination of total ozone.
已开发出一种通过对太阳直接辐照度进行多光谱测量来测定总臭氧量的方法。总臭氧量通过对290纳米至380纳米光谱进行最小二乘法拟合来确定。气溶胶消光通过在波长上展开为幂级数来考虑;结果表明使用线性项就足够了。已开发出一个配备天空扫描仪的移动实验室,并用于获取数据以验证该方法。太阳跟踪、双单色仪的波长设置以及数据采集均由一台小型计算机控制。在弗吉尼亚州的瓦勒普斯岛和得克萨斯州的巴勒斯坦所获得的结果与同时使用多布森光谱仪、坎特伯雷光谱仪以及气球电子俘获探测器臭氧探空仪测得的值吻合良好。单色仪的波长校准以及归一化臭氧吸收值是准确测定总臭氧量的最重要因素。