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Atmospheric Measurement Techniques An interactive open-access journal of the European Geosciences Union
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Volume 5, issue 8 | Copyright
Atmos. Meas. Tech., 5, 2013-2024, 2012
https://doi.org/10.5194/amt-5-2013-2012
© Author(s) 2012. This work is distributed under
the Creative Commons Attribution 3.0 License.

Research article 21 Aug 2012

Research article | 21 Aug 2012

Calibration of an all-sky camera for obtaining sky radiance at three wavelengths

R. Román1, M. Antón2,3, A. Cazorla2,3,*, A. de Miguel1, F. J. Olmo2,3, J. Bilbao1, and L. Alados-Arboledas2,3 R. Román et al.
  • 1Laboratorio de Atmósfera y Energía, Departamento de Física Aplicada, Universidad de Valladolid, C/ Dr. Mergelina s/n, 47005 Valladolid, Spain
  • 2Centro Andaluz de Medio Ambiente (CEAMA), Av. del Mediterráneo s/n, 18006 Granada, Spain
  • 3Departamento de Física Aplicada, Universidad de Granada, Campus de Fuentenueva s/n, 18071 Granada, Spain
  • *now at: Department of Chemistry and Biochemistry, University of California, San Diego, 9500 Gilman Drive La Jolla, California 92093, USA

Abstract. This paper proposes a method to obtain spectral sky radiances, at three wavelengths (464, 534 and 626 nm), from hemispherical sky images. Images are registered with the All-Sky Imager installed at the Andalusian Center for Environmental Research (CEAMA) in Granada (Spain). The methodology followed in this work for the absolute calibration in radiance of this instrument is based on the comparison of its output measurements with modelled sky radiances derived from the LibRadtran/UVSPEC radiative transfer code under cloud-free conditions. Previously, in order to check the goodness of the simulated radiances, these are compared with experimental values recorded by a CIMEL sunphotometer. In general, modelled radiances are in agreement with experimental data, showing mean differences lower than 20% except for the pixels located next to the Sun position that show larger errors.

The relationship between the output signal of the All-Sky Imager and the modelled sky radiances provides a calibration matrix for each image. The variability of the matrix coefficients is analyzed, showing no significant changes along a period of 5 months. Therefore, a unique calibration matrix per channel is obtained for all selected images (a total of 705 images per channel). Camera radiances are compared with CIMEL radiances, finding mean absolute differences between 2% and 15% except for pixels near to the Sun and high scattering angles. We apply these calibration matrices to three images in order to study the sky radiance distributions for three different sky conditions: cloudless, overcast and partially cloudy. Horizon brightening under cloudless conditions has been observed together with the enhancement effect of individual clouds on sky radiance.

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