Preprints
https://doi.org/10.5194/egusphere-2024-3141
https://doi.org/10.5194/egusphere-2024-3141
07 Nov 2024
 | 07 Nov 2024
Status: this preprint is open for discussion.

Evaluating sensitivity of optical snow grain size retrievals to radiative transfer models, shape parameters, and inversion techniques

James W. Dillon, Christopher P. Donahue, Evan N. Schehrer, and Kevin D. Hammonds

Abstract. The near-infrared (NIR) albedo of snow is controlled by optical snow grain size (ropt). Therefore, characterizing the spatial and temporal variability in ropt at the snow surface is critical for understanding melt timing and magnitude for water availability, and Earth’s energy budget towards future climates. While numerous studies have demonstrated estimates of ropt via optical instruments that span scales from in situ to satellites, they leverage differing retrieval techniques, radiative transfer models, and modeled snow grain shapes. Variation in these factors cause tremendous uncertainty in ropt retrievals, yet a thorough evaluation has yet to be conducted. To address this knowledge gap we conducted a laboratory bidirectional reflectance study, using NIR hyperspectral imaging (NIR-HSI) to retrieve grain size metrics for a wide variety of snow microstructures and evaluate them against micro-CT benchmarks. Towards enhanced ropt retrieval accuracy, we sought to determine 1) the optimal modeled snow grain shape, 2) the best-performing radiative transfer model, and 3) variability associated with retrieval techniques, spanning broadband, narrowband, multispectral, and hyperspectral approaches. Our results for optimizing grain shape parameters align with existing studies for the TARTES model, and we offer first recommendations for the SNICAR model. The retrieval technique also displayed considerable variation with the hyperspectral residual method performing best. Multispectral and single-band techniques were comparable to their hyperspectral counterparts at times, but this was attributed to the idealized laboratory conditions and high instrument signal-to-noise ratio. Following shape-optimization, the SNICAR and TARTES models produced the best results (median absolute error of 15.6–17.4 %, depending on technique), outperforming the AART model and the Random Mixture model. Towards a more direct comparison with albedo estimate error, we also evaluated the square root of ropt retrievals; median absolute error values ranged from 7.9–26.2 % depending on model and technique, with most pairings resulting in values < 15 %. Our results demonstrate that the accuracy of ropt retrievals is highly sensitive to the choice of retrieval technique, radiative transfer model, and grain shape parameters. To minimize error, each of these factors should be carefully selected in the context of the specific measurement. As NIR-HSI instruments and other NIR detectors become increasingly affordable and their resolution improve, the findings presented here provide guidance for improved ropt and snow albedo mapping across ground-based, aerial, and satellite platforms.

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James W. Dillon, Christopher P. Donahue, Evan N. Schehrer, and Kevin D. Hammonds

Status: open (until 19 Dec 2024)

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James W. Dillon, Christopher P. Donahue, Evan N. Schehrer, and Kevin D. Hammonds
James W. Dillon, Christopher P. Donahue, Evan N. Schehrer, and Kevin D. Hammonds

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Short summary
The optical grain size of snow controls albedo, playing a key role in Earth's energy balance. This parameter varies substantially in time and space, and thus accurate estimates are vital. Reflectance measurements can be used to map grain size, although results differ considerably depending on the algorithm and model used during retrieval. We perform a novel laboratory comparison to determine the optimal model, shape parameters, and retrieval algorithm for accurately estimating grain size.