Abstract

Abstract. This paper is an overview of the progress in sky radiometer technology and the development of the network called SKYNET. It is found that the technology has produced useful on-site calibration methods, retrieval algorithms, and data analyses from sky radiometer observations of aerosol, cloud, water vapor, and ozone. A formula was proposed for estimating the accuracy of the sky radiometer calibration constant F0 using the improved Langley (IL) method, which was found to be a good approximation to observed monthly mean uncertainty in F0, around 0.5 % to 2.4 % at the Tokyo and Rome sites and smaller values of around 0.3 % to 0.5 % at the mountain sites at Mt. Saraswati and Davos. A new cross IL (XIL) method was also developed to correct an underestimation by the IL method in cases with large aerosol retrieval errors. The root-mean-square difference (RMSD) in aerosol optical thickness (AOT) comparisons with other networks took values of less than 0.02 for λ≥500 nm and a larger value of about 0.03 for shorter wavelengths in city areas and smaller values of less than 0.01 in mountain comparisons. Accuracies of single-scattering albedo (SSA) and size distribution retrievals are affected by the propagation of errors in measurement, calibrations for direct solar and diffuse sky radiation, ground albedo, cloud screening, and the version of the analysis software called the Skyrad pack. SSA values from SKYNET were up to 0.07 larger than those from AERONET, and the major error sources were identified as an underestimation of solid viewing angle (SVA) and cloud contamination. Correction of these known error factors reduced the SSA difference to less than 0.03. Retrievals of other atmospheric constituents by the sky radiometer were also reviewed. Retrieval accuracies were found to be about 0.2 cm for precipitable water vapor amount and 13 DU (Dobson Unit) for column ozone amount. Retrieved cloud optical properties still showed large deviations from validation data, suggesting a need to study the causes of the differences. It is important that these recent studies on improvements presented in the present paper are introduced into the existing operational systems and future systems of the International SKYNET Data Center.

Highlights

  • A sun–sky radiometer is a narrow-band filter photometer able to perform measurements of direct solar and diffuse sky radiation at selected wavelengths and at several scattering angles

  • An estimate of the retrieval accuracy of F0 is given by Eq (10) for the improved Langley (IL) method, which can serve as an approximation of observed monthly mean uncertainty in F0 as 0.5 % to 2.4 % at the Tokyo and Rome sites and smaller values of around 0.3 % to 0.5 % at the mountain sites of Mt

  • These values are consistent with root-mean-square difference (RMSD) values, in the aerosol optical thickness (AOT) comparisons with other networks, of less than 0.02 for λ ≥ 500 nm and a larger value of about 0.03 for shorter wavelengths in city areas and smaller values of less than 0.01 in mountain comparisons

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Summary

Introduction

A sun–sky radiometer is a narrow-band filter photometer able to perform measurements of direct solar and diffuse sky radiation at selected wavelengths and at several scattering angles. Diffuse sky irradiance in the circumsolar or solar aureole region was measured by the pyranometer to correct for the atmospheric effects in the measured solar constant (Abbot and Aldrich, 1916) This method was used by Kalitin (1930), Fesenkov (1933), and PyaskovskayaFesenkova (1957) (Terez and Terez, 2003). Networks of radiometers have been developed to utilize sun and sky measurement data for various applications, such as satellite remote sensing validation, air pollution monitoring, and the study of the climate effects of atmospheric constituents, as overviewed by Holben et al (2001). Of and issues with SKYNET to provide better information for the community

Sun and sky measurements from the sky radiometer
Radiometric calibration of the direct solar irradiance measurements
Sky radiance calibration for the sky radiometer
Method a SL
Retrievals of parameters for atmospheric constituents
Method
Findings
Conclusions
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