2008
DOI: 10.1007/s11207-008-9187-7
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The High-Resolution Solar Reference Spectrum between 250 and 550 nm and its Application to Measurements with the Ozone Monitoring Instrument

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Cited by 72 publications
(90 citation statements)
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“…Since EPIC does not measure solar irradiance, we use a high-resolution solar irradiance spectrum, S(λ) (Dobber et al, 2008), as a reference solar spectrum. The reference spectrum is convolved with EPIC's filter transmission functions T M (λ) (Fig.…”
Section: Calibrationmentioning
confidence: 99%
“…Since EPIC does not measure solar irradiance, we use a high-resolution solar irradiance spectrum, S(λ) (Dobber et al, 2008), as a reference solar spectrum. The reference spectrum is convolved with EPIC's filter transmission functions T M (λ) (Fig.…”
Section: Calibrationmentioning
confidence: 99%
“…Next, the following equation is used for the DOAS fit: Bogumil et al (2000) at 220 K. I R (λ) was calculated using as input the expressions given in Chance and Spurr (1997), numbers given in Burrows et al (1996) and the high-resolution solar irradiance provided by Dobber et al (2008). The Raman spectrum was then calculated by convolving the solar spectrum with the rotational Raman lines and the OMI slit function and divided by the convoluted solar spectrum.…”
Section: Doas Fitmentioning
confidence: 99%
“…First, a high-resolution oversampled solar atlas that is convolved to the OMI instrument line shape (Dobber et al, 2008b) is interpolated onto both the reference and radiance spectra wavelength grids (F λ(REF) and F λ(ES) respectively) using cubic spline interpolation. The ratio of these interpolated spectra is then multiplied by the intensity of the solar irradiance, which therefore gives the desired interpolation.…”
Section: Retrieval Using Omi L1b Spectral Datamentioning
confidence: 99%