Klaus Pfeilsticker

Abstract: Ajavon, Ayité-Lo Université de Lomé Togo Andersen, Stephen O. Environmental Protection Agency USA Austin, John NOAA Geophysical Fluid Dynamics Laboratory USA Bais, Alkiviadis F. Aristotle University of Thessaloniki Greece Baldwin, Mark NorthWest Research Associates, Inc. USA Beig, Gufran Indian Institute of Tropical Meteorology India Björn, Lars Olof Lund University Sweden Bodeker, Greg National Institute of Water & Atmospheric Research New Zealand Braathen, Geir World Meteorological Organization Switzerland Burrows, John University of Bremen Germany Chanin, Marie-Lise Service d'Aeronomie du CNRS France Chipperfield, Martyn University of Leeds UK Clerbaux, Catherine Service d'Aeronomie du CNRS France Cunnold, Derek Georgia Institute of Technology USA Dameris, Martin German Aerospace Center (DLR) Institut für Physik der Atmosphäre Germany

TL;DR: In this article, the most significant sources of error are identified as the wavelength calibration of several of the absorption cross sections fitted and of the measured spectra themselves, the wavelength region of the fitting, the temperature dependence of the O3 absorption cross section, failure to adequately account for the so-called I0 effect, inadequate offset correction, and inadequate measurement of the individual instrument slit functions.

TL;DR: In this article, a Monte Carlo atmospheric radiative transfer model is presented to support the interpretation of UV/vis/near-IR spectroscopic measurements of scattered Sun light in the atmosphere.

TL;DR: Observation implies that the WD |0>f|4>b band is located at 749.5 nanometers, with a full width at half maximum of ∼19.4 wave numbers, and that its band strength ranges between 1.23 × 10–22 and 5.25 × 10-22 centimeters per molecule.