Microstructure representation of snow in coupled snowpack and microwave emission models

This is the first study to encompass a wide range of coupled snow evolution and microwave emission models in a common modelling framework in order to generalise the link between snowpack microstructure predicted by the snow evolution models and microstructure required to reproduce observations of br...

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Published in:The Cryosphere
Main Authors: Sandells, Melody, Essery, Richard, Rutter, Nick, Wake, Leanne, Leppänen, Leena, Lemmetyinen, Juha
Format: Text
Language:English
Published: 2018
Subjects:
Online Access:https://doi.org/10.5194/tc-11-229-2017
https://tc.copernicus.org/articles/11/229/2017/
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author Sandells, Melody
Essery, Richard
Rutter, Nick
Wake, Leanne
Leppänen, Leena
Lemmetyinen, Juha
author_facet Sandells, Melody
Essery, Richard
Rutter, Nick
Wake, Leanne
Leppänen, Leena
Lemmetyinen, Juha
author_sort Sandells, Melody
collection Copernicus Publications: E-Journals
container_issue 1
container_start_page 229
container_title The Cryosphere
container_volume 11
description This is the first study to encompass a wide range of coupled snow evolution and microwave emission models in a common modelling framework in order to generalise the link between snowpack microstructure predicted by the snow evolution models and microstructure required to reproduce observations of brightness temperature as simulated by snow emission models. Brightness temperatures at 18.7 and 36.5 GHz were simulated by 1323 ensemble members, formed from 63 Jules Investigation Model snowpack simulations, three microstructure evolution functions, and seven microwave emission model configurations. Two years of meteorological data from the Sodankylä Arctic Research Centre, Finland, were used to drive the model over the 2011–2012 and 2012–2013 winter periods. Comparisons between simulated snow grain diameters and field measurements with an IceCube instrument showed that the evolution functions from SNTHERM simulated snow grain diameters that were too large (mean error 0.12 to 0.16 mm), whereas MOSES and SNICAR microstructure evolution functions simulated grain diameters that were too small (mean error −0.16 to −0.24 mm for MOSES and −0.14 to −0.18 mm for SNICAR). No model (HUT, MEMLS, or DMRT-ML) provided a consistently good fit across all frequencies and polarisations. The smallest absolute values of mean bias in brightness temperature over a season for a particular frequency and polarisation ranged from 0.7 to 6.9 K. Optimal scaling factors for the snow microstructure were presented to compare compatibility between snowpack model microstructure and emission model microstructure. Scale factors ranged between 0.3 for the SNTHERM–empirical MEMLS model combination (2011–2012) and 3.3 for DMRT-ML in conjunction with MOSES microstructure (2012–2013). Differences in scale factors between microstructure models were generally greater than the differences between microwave emission models, suggesting that more accurate simulations in coupled snowpack–microwave model systems will be achieved primarily through improvements in the snowpack microstructure representation, followed by improvements in the emission models. Other snowpack parameterisations in the snowpack model, mainly densification, led to a mean brightness temperature difference of 11 K at 36.5 GHz H-pol and 18 K at V-pol when the Jules Investigation Model ensemble was applied to the MOSES microstructure and empirical MEMLS emission model for the 2011–2012 season. The impact of snowpack parameterisation increases as the microwave scattering increases. Consistency between snowpack microstructure and microwave emission models, and the choice of snowpack densification algorithms should be considered in the design of snow mass retrieval systems and microwave data assimilation systems.
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spelling ftcopernicus:oai:publications.copernicus.org:tc53801 2025-01-16T20:52:01+00:00 Microstructure representation of snow in coupled snowpack and microwave emission models Sandells, Melody Essery, Richard Rutter, Nick Wake, Leanne Leppänen, Leena Lemmetyinen, Juha 2018-09-27 application/pdf https://doi.org/10.5194/tc-11-229-2017 https://tc.copernicus.org/articles/11/229/2017/ eng eng doi:10.5194/tc-11-229-2017 https://tc.copernicus.org/articles/11/229/2017/ eISSN: 1994-0424 Text 2018 ftcopernicus https://doi.org/10.5194/tc-11-229-2017 2020-07-20T16:23:51Z This is the first study to encompass a wide range of coupled snow evolution and microwave emission models in a common modelling framework in order to generalise the link between snowpack microstructure predicted by the snow evolution models and microstructure required to reproduce observations of brightness temperature as simulated by snow emission models. Brightness temperatures at 18.7 and 36.5 GHz were simulated by 1323 ensemble members, formed from 63 Jules Investigation Model snowpack simulations, three microstructure evolution functions, and seven microwave emission model configurations. Two years of meteorological data from the Sodankylä Arctic Research Centre, Finland, were used to drive the model over the 2011–2012 and 2012–2013 winter periods. Comparisons between simulated snow grain diameters and field measurements with an IceCube instrument showed that the evolution functions from SNTHERM simulated snow grain diameters that were too large (mean error 0.12 to 0.16 mm), whereas MOSES and SNICAR microstructure evolution functions simulated grain diameters that were too small (mean error −0.16 to −0.24 mm for MOSES and −0.14 to −0.18 mm for SNICAR). No model (HUT, MEMLS, or DMRT-ML) provided a consistently good fit across all frequencies and polarisations. The smallest absolute values of mean bias in brightness temperature over a season for a particular frequency and polarisation ranged from 0.7 to 6.9 K. Optimal scaling factors for the snow microstructure were presented to compare compatibility between snowpack model microstructure and emission model microstructure. Scale factors ranged between 0.3 for the SNTHERM–empirical MEMLS model combination (2011–2012) and 3.3 for DMRT-ML in conjunction with MOSES microstructure (2012–2013). Differences in scale factors between microstructure models were generally greater than the differences between microwave emission models, suggesting that more accurate simulations in coupled snowpack–microwave model systems will be achieved primarily through improvements in the snowpack microstructure representation, followed by improvements in the emission models. Other snowpack parameterisations in the snowpack model, mainly densification, led to a mean brightness temperature difference of 11 K at 36.5 GHz H-pol and 18 K at V-pol when the Jules Investigation Model ensemble was applied to the MOSES microstructure and empirical MEMLS emission model for the 2011–2012 season. The impact of snowpack parameterisation increases as the microwave scattering increases. Consistency between snowpack microstructure and microwave emission models, and the choice of snowpack densification algorithms should be considered in the design of snow mass retrieval systems and microwave data assimilation systems. Text Arctic Sodankylä Copernicus Publications: E-Journals Arctic Jules ENVELOPE(140.917,140.917,-66.742,-66.742) Moses ENVELOPE(-99.183,-99.183,-74.550,-74.550) Sodankylä ENVELOPE(26.600,26.600,67.417,67.417) The Cryosphere 11 1 229 246
spellingShingle Sandells, Melody
Essery, Richard
Rutter, Nick
Wake, Leanne
Leppänen, Leena
Lemmetyinen, Juha
Microstructure representation of snow in coupled snowpack and microwave emission models
title Microstructure representation of snow in coupled snowpack and microwave emission models
title_full Microstructure representation of snow in coupled snowpack and microwave emission models
title_fullStr Microstructure representation of snow in coupled snowpack and microwave emission models
title_full_unstemmed Microstructure representation of snow in coupled snowpack and microwave emission models
title_short Microstructure representation of snow in coupled snowpack and microwave emission models
title_sort microstructure representation of snow in coupled snowpack and microwave emission models
url https://doi.org/10.5194/tc-11-229-2017
https://tc.copernicus.org/articles/11/229/2017/