the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
A study of optical scattering modelling for mixed phase Polar Stratospheric Clouds
Abstract. Scattering codes are used to study the optical properties of Polar Stratospheric Clouds (PSC). Backscattering and extinction can be computed with available scattering codes once the particle size distribution (PSD) is known and a suitable refractive index is assumed. However, PSCs often appear as external mixtures of Supercooled Ternary Solution (STS) droplets, solid Nitric Acid Trihydrate (NAT) and possibly ice particles, making questionable the assumption of a single refractive index and a single morphology to model the scattarers. Here we consider a set of fifteen coincident measurements of PSC above McMurdo Station, Antarctica, by ground-based lidar and balloon-borne Optical Particle Counters (OPC), and in situ observations taken by a laser backscattersonde and an OPC during four balloon stratospheric flights from Kiruna, Sweden. This unique dataset of microphysical and optical observations allows to test the performances of optical scattering models when both spherical and aspherical scatterers of different composition and, possibly, shapes are present.
Here we consider particles as STS if their radius is below a certain threshold value Rth and NAT or possibly ice if above it. The refractive indices are assumed known from the literature. Mie scattering is used for the STS, assumed spherical, while scattering from NAT particles, considered as spheroids of different Aspect Ratio (AR), is treated with T-Matrix results where applicable, and of geometric-optics-integral-equation approach where the particle size parameter is too large to allow for a convergence of the T matrix method. The parameters Rth and AR of our model are chosen to provide the best match with the observed optical backscattering and depolarization. The comparison of the calculations with the measures is satisfactory for the backscattering but not so for the depolarization, and possible causes are discussed. The results of this work help to understand the limits of the application of these scattering theories in modeling the optical response of particles of different composition and morphology.
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Notice on discussion status
The requested preprint has a corresponding peer-reviewed final revised paper. You are encouraged to refer to the final revised version.
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Preprint
(3299 KB)
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The requested preprint has a corresponding peer-reviewed final revised paper. You are encouraged to refer to the final revised version.
- Preprint
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- Final revised paper
Journal article(s) based on this preprint
Interactive discussion
Status: closed
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RC1: 'Reviewer 1', Darrel Baumgardner, 21 Nov 2022
The comment was uploaded in the form of a supplement: https://egusphere.copernicus.org/preprints/2022/egusphere-2022-972/egusphere-2022-972-RC1-supplement.pdf
- AC1: 'Reply on RC1', Francesco Cairo, 10 Jan 2023
- AC3: 'Reply on RC1', Francesco Cairo, 10 Jan 2023
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RC2: 'Comment on egusphere-2022-972', Cynthia Twohy, 22 Nov 2022
The comment was uploaded in the form of a supplement: https://egusphere.copernicus.org/preprints/2022/egusphere-2022-972/egusphere-2022-972-RC2-supplement.pdf
- AC2: 'Reply on RC2', Francesco Cairo, 10 Jan 2023
Interactive discussion
Status: closed
-
RC1: 'Reviewer 1', Darrel Baumgardner, 21 Nov 2022
The comment was uploaded in the form of a supplement: https://egusphere.copernicus.org/preprints/2022/egusphere-2022-972/egusphere-2022-972-RC1-supplement.pdf
- AC1: 'Reply on RC1', Francesco Cairo, 10 Jan 2023
- AC3: 'Reply on RC1', Francesco Cairo, 10 Jan 2023
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RC2: 'Comment on egusphere-2022-972', Cynthia Twohy, 22 Nov 2022
The comment was uploaded in the form of a supplement: https://egusphere.copernicus.org/preprints/2022/egusphere-2022-972/egusphere-2022-972-RC2-supplement.pdf
- AC2: 'Reply on RC2', Francesco Cairo, 10 Jan 2023
Peer review completion
Journal article(s) based on this preprint
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Terry Deshler
Luca Di Liberto
Andrea Scoccione
Marcel Snels
The requested preprint has a corresponding peer-reviewed final revised paper. You are encouraged to refer to the final revised version.
- Preprint
(3299 KB) - Metadata XML