太阳光度计校准的极端方法

Hikmat Hamid Asadov, I. Chobanzade
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引用次数: 0

摘要

太阳光度计是目前测量大气气溶胶光学厚度和大气水汽总量的主要气象仪器之一。这些装置在功能上也适用于估算大气中臭氧的总量,这证实了太阳光度计对气象科学的重要性。目前,基于这种设备的气溶胶测量网络正在各地建立。太阳光度计正常工作的最重要条件是对该设备进行准确校准。本文致力于开发一种新的太阳光度计校准方法,该方法几乎完全消除了大气气溶胶不稳定性的影响。结果表明,太阳光度计的总标定误差由两部分组成:(a)大气气溶胶不稳定性引起的误差;(b)兰利图几何构造误差。第一个组件实际上被认为无法用现有方法恢复,第二个组件可以使用先前提出的计算方法消除。所开发的极端校准太阳光度计的方法不需要在几个小时内构建兰利图,在此期间,大气气溶胶由于其可变性,在校准结果中引入了重大误差。从而消除了经典Langley方法的主要缺点。通过形成一个额外的信息指标和进一步研究这个新引入的指标的极值,可以达到提高校准精度的效果。给出了提高精度效果的定量指标。作为一个例子,尽管所提出的方法的实施时间较长,但当大气光学厚度小于0.1时,当该指标在Langley方法的实施过程中不稳定10%时,可以消除2.74%的气溶胶误差。给出了器件的功能光学方案和实现校准方法的算法。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
EXTREME METHOD FOR SOLAR PHOTOMETERS CALIBRATION
Solar photometers are currently one of the main meteorological instruments with which the optical thickness of atmospheric aerosol and the total amount of water vapor in the atmosphere can be measured. These devices are also functionally suitable for estimating the total amount of ozone in the atmosphere, which confirms the importance of solar photometers for meteorological science. At present, aerosol measurement networks based on such devices are being built everywhere. The most important condition for the normal functioning of a solar photometer is the accurate calibration of this device. The article is devoted to the development of a new method of calibration of solar photometers, in which the influence of atmospheric aerosol instability is almost completely eliminated. It is shown that the total calibration error of solar photometers consists of two components: (a) the error caused by the instability of atmospheric aerosol; (b) the error of the geometric construction of the Langley diagram. The first of these components is practically considered unrecoverable by existing methods, and the second can be eliminated using previously proposed computational methods. The developed extreme method of calibration of solar photometers eliminates the need to construct a Langley diagram for several hours, during which the atmospheric aerosol, due to its variability, introduces a significant error in the calibration result. Thus, the main drawback of the classical Langley method is eliminated. The effect of increasing the accuracy of calibration is achieved by forming an additional informative indicator and further investigation of the extremum of this newly introduced indicator. Quantitative indicators of the achieved effect of increasing accuracy are given. As an example, it is shown that despite some high duration of implementation of the proposed method, it becomes possible to eliminate the aerosol error of 2.74 % that occurs when the optical thickness of the atmosphere is less than 0.1, and when this indicator is unstable by 10 percent during the implementation of the Langley method. The functional optical scheme of the device and the algorithm for implementing the proposed calibration method are given.
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