Articles | Volume 20, issue 4
Atmos. Chem. Phys., 20, 1961–1976, 2020
Atmos. Chem. Phys., 20, 1961–1976, 2020

Research article 21 Feb 2020

Research article | 21 Feb 2020

Accurate 3-D radiative transfer simulation of spectral solar irradiance during the total solar eclipse of 21 August 2017

Paul Ockenfuß et al.


Interactive discussion

Status: closed
Status: closed
AC: Author comment | RC: Referee comment | SC: Short comment | EC: Editor comment
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Peer-review completion

AR: Author's response | RR: Referee report | ED: Editor decision
AR by Paul Ockenfuss on behalf of the Authors (23 Dec 2019)  Author's response    Manuscript
ED: Publish as is (11 Jan 2020) by Stelios Kazadzis
Short summary
We model solar radiation as it would be measured on the Earth's surface in the core shadow of a total solar eclipse. Subsequently, we compare our results to observations during the total eclipse 2017 for ultraviolet, visible and near-infrared wavelengths. Moreover, we analyze the effect of the surface reflectance, the ozone profile, aerosol and the topography and give a visualization of the prevailing photons paths in the atmosphere during the eclipse.
Final-revised paper