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Atmospheric Chemistry and Physics An interactive open-access journal of the European Geosciences Union
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Given the time and location of a point on the Earth's surface, we explain how to compute the wavelength-dependent obscuration fraction during solar eclipses. We restore the top-of-atmosphere reflectances and the Absorbing Aerosol Index in the partial Moon shadow during the eclipses on 26 December 2019 and 21 June 2020 measured by TROPOMI. This correction method resolves eclipse anomalies and allows for studying the effect of solar eclipses on the composition of the Earth's atmosphere from space.
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https://doi.org/10.5194/acp-2020-1172
https://doi.org/10.5194/acp-2020-1172

  18 Dec 2020

18 Dec 2020

Review status: this preprint is currently under review for the journal ACP.

Restoring the top-of-atmosphere reflectance during solar eclipses: a proof of concept with the UV Absorbing Aerosol Index measured by TROPOMI

Victor Trees1,2, Ping Wang1, and Piet Stammes1 Victor Trees et al.
  • 1Royal Netherlands Meteorological Institute (KNMI), De Bilt, The Netherlands
  • 2Delft University of Technology, Delft, The Netherlands

Abstract. Solar eclipses reduce the measured top-of-atmosphere (TOA) reflectances as derived by Earth observation satellites, because the solar irradiance that is used to compute these reflectances is commonly measured before the start of the eclipse. Consequently, air quality products that are derived from these spectra, such as the ultraviolet (UV) Absorbing Aerosol Index (AAI), are distorted or undefined in the shadow of the Moon. The availability of air quality satellite data in the penumbral and antumbral shadow during solar eclipses, however, may be of particular interest to users studying solar eclipses and their effect on the Earth's atmosphere. Given the time and location of a point on the Earth's surface, we explain how to compute the eclipse obscuration fraction taking into account wavelength dependent solar limb darkening. With the calculated obscuration fractions, we restore the TOA reflectances and the AAI in the penumbral shadow during the annular solar eclipses on 26 December 2019 and 21 June 2020 measured by the TROPOMI/S5P instrument. We verify the calculated obscuration with the observed obscuration using an uneclipsed orbit. In the corrected products, the signature of the Moon shadow disappeared. Not taking into account solar limb darkening, however, would result in a maximum underestimation of the obscuration fraction of 0.06 at 380 nm on 26 December 2019, and in a maximum Moon shadow signature in the AAI of 6.7 points increase. We find that the Moon shadow anomaly in the uncorrected AAI is caused by a reduction of the measured reflectance at 380 nm, rather than a color change of the measured light. We restore common AAI features such as the sunglint and desert dust, and we confirm the restored AAI feature on 21 June 2020 at the Taklamakan desert by measurements of the GOME-2C satellite instrument on the same day but outside the Moon shadow. We conclude that the correction method of this paper can be used to detect real AAI rising phenomena and has the potential to restore any other product that is derived from TOA reflectance spectra. This would resolve the solar eclipse anomalies in satellite air quality measurements in the penumbra and antumbra, and would allow for studying the effect of the eclipse obscuration on the composition of the Earth's atmosphere from space.

Victor Trees et al.

 
Status: open (until 12 Feb 2021)
Status: open (until 12 Feb 2021)
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Victor Trees et al.

Victor Trees et al.

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Short summary
Given the time and location of a point on the Earth's surface, we explain how to compute the wavelength-dependent obscuration fraction during solar eclipses. We restore the top-of-atmosphere reflectances and the Absorbing Aerosol Index in the partial Moon shadow during the eclipses on 26 December 2019 and 21 June 2020 measured by TROPOMI. This correction method resolves eclipse anomalies and allows for studying the effect of solar eclipses on the composition of the Earth's atmosphere from space.
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