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On radiative heating due to polar stratospheric clouds

Jean-Pierre Blanchet
- 11 Sep 1985 - 
- Vol. 37, pp 197-209
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TLDR
In this paper, a simple parameterization of optical properties of polar stratospheric clouds is presented for inclusion into broad band radiation models, where the authors show that the radiative effect appears more sensitive to the distribution of cloud than to the strength of the surface temperature inversion.
Abstract
Recent satellite observations of polar stratospheric clouds (PSCs) and the theoretical explanation of their formation brought up questions on the radiative effects of those thin clouds. Optical parameters are calculated for selected stages of the cloud development and for wavelengths between I and 40 μn. Radiative transfer calculations yield absolute values of heating rates of about 0.03 K/day for the thickest polar stratospheric clouds observed by the SAM II satellite. The top portion of the cloud is characterized by cooling of the order of 0.01 K/day while thr lower and denser part of the cloud may experience either cooling or warming depending on the thermal structure and on the vertical distribution of clouds in the troposphere. Due to the correlation between cold stratosphere and warm troposphere, the radiative effect appears more sensitive to the distribution of cloud than to the strength of the surface temperature inversion. Unlike most tropospheric cases and under favorable conditions, the growth of cloud particles may reach equilibrium not only by depletion of ambient moisture but also by thermal equilibrium. The hypothetical fully developed cloud would lead to absolute values of the heating rates of the order of 1 K/day. The maximum warming is found in the wings of the I5 μm CO 2 band and extends up to 24 μm, while some cooling occurs at the upper end of the thermal spectrum. A simple parameterization of optical properties of PSCs is presented for inclusion into broad band radiation models. DOI: 10.1111/j.1600-0889.1985.tb00069.x

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Journal ArticleDOI

The mystery of the Antarctic Ozone “Hole”

TL;DR: In this paper, the authors reviewed observations of the total ozone column and its vertical profile over Antarctica, and the current status of the evidence supporting various theories of the behavior of ozone in the Antarctic is summarized.
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The Arctic polar stratospheric cloud aerosol: Aircraft measurements of reactive nitrogen, total water, and particles

TL;DR: In situ aircraft measurements in the lower stratosphere are used to investigate the reactive nitrogen, NO(y), total water, and particle components of the polar stratospheric cloud (PSC) aerosol in the Arctic as discussed by the authors.
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Total ozone, ozone vertical distributions, and stratospheric temperatures at South Pole, Antarctica, in 1986 and 1987

TL;DR: Ozone and temperatures measured in 1986 and 1987 at South Pole, Antarctica, are compared, with emphasis on observations made at the time of formation of the Antarctica ozone hole.
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Radiative effects of polar stratospheric clouds

TL;DR: In this paper, radiative transfer calculations for polar stratospheric clouds (PSCs) using newly acquired PSC properties and polar atmospheric data are performed for PSC radiative effects depend strongly on upwelling thermal radiation and vary from infrared heating over warm polar surfaces such as oceans, to cooling over cold surfaces, such as the Antarctic plateau.
Journal ArticleDOI

Radiative effects of polar stratospheric clouds during the Airborne Antarctic Ozone Experiment and the Airborne Arctic Stratospheric Expedition

TL;DR: In this article, the radiative effects of polar stratospheric clouds during the Airborne Antarctic Ozone Experiment (AAOE) and the airborne Arctic Stratospheric Expedition (AASE) were studied.
References
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TL;DR: Extinction coefficients k(lambda) for water at 25 degrees C were determined through a broad spectral region by manually smoothing a point by point graph of k( lambda) vs wavelength lambda that was plotted for data obtained from a review of the scientific literature on the optical constants of water.
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TL;DR: The latest edition of the AFGL atmospheric absorption line parameters compilation for the seven most active infrared terrestrial absorbers is described and the sources of the absorption parameters are summarized.
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Random Lorentz band model with exponential-tailed S-1 line-intensity distribution function

TL;DR: In this article, the growth curves calculated for Lorentz lines were used for molecular spectra representation using growth curves for the 1.1/s line intensity distribution function, and the growth curve was calculated for the 2.5/2.
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