Sensitivity of modeled snow grain size retrievals to solar geometry, snow particle asphericity, and snowpack impurities

Snow grain size is an important metric to determine snow age and metamorphism, but it is difficult to measure. The effective grain size can be derived from spaceborne and airborne radiance measurements due to strong attenuation of near-infrared energy by ice. Consequently, a snow grain size inversio...

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Bibliographic Details
Published in:The Cryosphere
Main Authors: Z. Fair, M. Flanner, A. Schneider, S. M. Skiles
Format: Article in Journal/Newspaper
Language:English
Published: Copernicus Publications 2022
Subjects:
geo
Online Access:https://doi.org/10.5194/tc-16-3801-2022
https://tc.copernicus.org/articles/16/3801/2022/tc-16-3801-2022.pdf
https://doaj.org/article/f7e0bf78fc084ee1aec59dc281b5c0b9
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record_format openpolar
spelling fttriple:oai:gotriple.eu:oai:doaj.org/article:f7e0bf78fc084ee1aec59dc281b5c0b9 2023-05-15T18:32:18+02:00 Sensitivity of modeled snow grain size retrievals to solar geometry, snow particle asphericity, and snowpack impurities Z. Fair M. Flanner A. Schneider S. M. Skiles 2022-09-01 https://doi.org/10.5194/tc-16-3801-2022 https://tc.copernicus.org/articles/16/3801/2022/tc-16-3801-2022.pdf https://doaj.org/article/f7e0bf78fc084ee1aec59dc281b5c0b9 en eng Copernicus Publications doi:10.5194/tc-16-3801-2022 1994-0416 1994-0424 https://tc.copernicus.org/articles/16/3801/2022/tc-16-3801-2022.pdf https://doaj.org/article/f7e0bf78fc084ee1aec59dc281b5c0b9 undefined The Cryosphere, Vol 16, Pp 3801-3814 (2022) geo envir Journal Article https://vocabularies.coar-repositories.org/resource_types/c_6501/ 2022 fttriple https://doi.org/10.5194/tc-16-3801-2022 2023-01-22T18:11:43Z Snow grain size is an important metric to determine snow age and metamorphism, but it is difficult to measure. The effective grain size can be derived from spaceborne and airborne radiance measurements due to strong attenuation of near-infrared energy by ice. Consequently, a snow grain size inversion technique that uses hyperspectral radiances and exploits variations in the 1.03 µm ice absorption feature was previously developed for use with airborne imaging spectroscopy. Previous studies have since demonstrated the effectiveness of the technique, though there has yet to be a quantitative assessment of the retrieval sensitivity to snowpack impurities, ice particle shape, or solar geometry. In this study, we use the Snow, Ice, and Aerosol Radiative (SNICAR) model and a Monte Carlo photon tracking model to examine the sensitivity of snow grain size retrievals to changes in dust and black carbon content, anisotropic reflectance, changes in solar illumination angle (θ0), and scattering asymmetry parameter (g) associated with different particle shapes. Our results show that changes in these variables can produce large grain size errors, especially when the effective grain size exceeds 500 µm. Dust content of 1000 ppm induces errors exceeding 800 µm, with the highest biases associated with small particles. Aspherical ice particles and perturbed solar zenith angles produce maximum biases of ∼540 µm and ∼400 µm, respectively, when spherical snow grains and θ0=60∘ are assumed in the generation of the retrieval calibration curve. Retrievals become highly sensitive to viewing angle when reflectance is anisotropic, with biases exceeding 1000 µm in extreme cases. Overall, we show that a more detailed understanding of snowpack state and solar geometry improves the precision when determining snow grain size through hyperspectral remote sensing. Article in Journal/Newspaper The Cryosphere Unknown The Cryosphere 16 9 3801 3814
institution Open Polar
collection Unknown
op_collection_id fttriple
language English
topic geo
envir
spellingShingle geo
envir
Z. Fair
M. Flanner
A. Schneider
S. M. Skiles
Sensitivity of modeled snow grain size retrievals to solar geometry, snow particle asphericity, and snowpack impurities
topic_facet geo
envir
description Snow grain size is an important metric to determine snow age and metamorphism, but it is difficult to measure. The effective grain size can be derived from spaceborne and airborne radiance measurements due to strong attenuation of near-infrared energy by ice. Consequently, a snow grain size inversion technique that uses hyperspectral radiances and exploits variations in the 1.03 µm ice absorption feature was previously developed for use with airborne imaging spectroscopy. Previous studies have since demonstrated the effectiveness of the technique, though there has yet to be a quantitative assessment of the retrieval sensitivity to snowpack impurities, ice particle shape, or solar geometry. In this study, we use the Snow, Ice, and Aerosol Radiative (SNICAR) model and a Monte Carlo photon tracking model to examine the sensitivity of snow grain size retrievals to changes in dust and black carbon content, anisotropic reflectance, changes in solar illumination angle (θ0), and scattering asymmetry parameter (g) associated with different particle shapes. Our results show that changes in these variables can produce large grain size errors, especially when the effective grain size exceeds 500 µm. Dust content of 1000 ppm induces errors exceeding 800 µm, with the highest biases associated with small particles. Aspherical ice particles and perturbed solar zenith angles produce maximum biases of ∼540 µm and ∼400 µm, respectively, when spherical snow grains and θ0=60∘ are assumed in the generation of the retrieval calibration curve. Retrievals become highly sensitive to viewing angle when reflectance is anisotropic, with biases exceeding 1000 µm in extreme cases. Overall, we show that a more detailed understanding of snowpack state and solar geometry improves the precision when determining snow grain size through hyperspectral remote sensing.
format Article in Journal/Newspaper
author Z. Fair
M. Flanner
A. Schneider
S. M. Skiles
author_facet Z. Fair
M. Flanner
A. Schneider
S. M. Skiles
author_sort Z. Fair
title Sensitivity of modeled snow grain size retrievals to solar geometry, snow particle asphericity, and snowpack impurities
title_short Sensitivity of modeled snow grain size retrievals to solar geometry, snow particle asphericity, and snowpack impurities
title_full Sensitivity of modeled snow grain size retrievals to solar geometry, snow particle asphericity, and snowpack impurities
title_fullStr Sensitivity of modeled snow grain size retrievals to solar geometry, snow particle asphericity, and snowpack impurities
title_full_unstemmed Sensitivity of modeled snow grain size retrievals to solar geometry, snow particle asphericity, and snowpack impurities
title_sort sensitivity of modeled snow grain size retrievals to solar geometry, snow particle asphericity, and snowpack impurities
publisher Copernicus Publications
publishDate 2022
url https://doi.org/10.5194/tc-16-3801-2022
https://tc.copernicus.org/articles/16/3801/2022/tc-16-3801-2022.pdf
https://doaj.org/article/f7e0bf78fc084ee1aec59dc281b5c0b9
genre The Cryosphere
genre_facet The Cryosphere
op_source The Cryosphere, Vol 16, Pp 3801-3814 (2022)
op_relation doi:10.5194/tc-16-3801-2022
1994-0416
1994-0424
https://tc.copernicus.org/articles/16/3801/2022/tc-16-3801-2022.pdf
https://doaj.org/article/f7e0bf78fc084ee1aec59dc281b5c0b9
op_rights undefined
op_doi https://doi.org/10.5194/tc-16-3801-2022
container_title The Cryosphere
container_volume 16
container_issue 9
container_start_page 3801
op_container_end_page 3814
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