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Table 1 Uncertainty of sky irradiance based on comparison between \(f^{{{\text{obs}}}}\) and \(f^{{{\text{gf}}}}\)

From: Rapid, accurate computation of narrow-band sky radiance in the 940 nm gas absorption region using the correlated k-distribution method for sun-photometer observations

Wavelength

Num. of data

Standard deviation

315 nm

127

\(5.0\times {10}^{-3}\)

340 nm

117

\(3.0\times {10}^{-3}\)

380 nm

104

\(1.9\times {10}^{-3}\)

400 nm

122

\(2.7\times {10}^{-3}\)

500 nm

119

\(2.9\times {10}^{-3}\)

675 nm

114

\(4.1\times {10}^{-3}\)

870 nm

135

\(6.5\times {10}^{-3}\)

1020 nm

105

\(4.3\times {10}^{-3}\)

940 nm

110

\(4.3\times {10}^{-3}\)

1627 nm

56

\(4.8\times {10}^{-3}\)

2200 nm

57

\(4.4 \times 10^{ - 3}\)