Introducing Ice Nucleating Particles functionality into the Unified Model and its impact on the Southern Ocean short-wave radiation biases

Insufficient reflection of short-wave radiation especially over the Southern Ocean region is still a leading issue in many present-day global climate models. One of the potential reasons for this observed bias is an inadequate representation of clouds. In a previous study, we modified the cloud micr...

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Main Authors: Varma, Vidya, Morgenstern, Olaf, Furtado, Kalli, Field, Paul, Williams, Jonny
Format: Text
Language:English
Published: 2021
Subjects:
Online Access:https://doi.org/10.5194/acp-2021-438
https://acp.copernicus.org/preprints/acp-2021-438/
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spelling ftcopernicus:oai:publications.copernicus.org:acpd94860 2023-05-15T18:24:35+02:00 Introducing Ice Nucleating Particles functionality into the Unified Model and its impact on the Southern Ocean short-wave radiation biases Varma, Vidya Morgenstern, Olaf Furtado, Kalli Field, Paul Williams, Jonny 2021-06-11 application/pdf https://doi.org/10.5194/acp-2021-438 https://acp.copernicus.org/preprints/acp-2021-438/ eng eng doi:10.5194/acp-2021-438 https://acp.copernicus.org/preprints/acp-2021-438/ eISSN: 1680-7324 Text 2021 ftcopernicus https://doi.org/10.5194/acp-2021-438 2021-06-14T16:22:13Z Insufficient reflection of short-wave radiation especially over the Southern Ocean region is still a leading issue in many present-day global climate models. One of the potential reasons for this observed bias is an inadequate representation of clouds. In a previous study, we modified the cloud micro-physics scheme in the Unified Model and showed that choosing a more realistic value for the capacitance or shape parameter of atmospheric ice-crystals, in better agreement with theory and observations, benefits the simulation of short-wave radiation over the Southern Ocean by brightening the clouds. However, attempts to modify the cloud phase by directly adjusting the micro-physics process rates like capacitance tend to affect both the hemispheres symmetrically whereas we seek to brighten only the high-latitude Southern Hemisphere clouds. In this study we implement a simple prognostic parametrisation whereby the heterogeneous ice nucleation temperature is made to vary three-dimensionally as a function of the mineral dust distribution in the model. As a result, those regions with less dust number density would have lower nucleation temperature compared to the default global value of −10 °C. By using mineral dust as an indicator for ice nucleating particles in the model, this parametrisation thus captures the impact of ice nucleating particles on the cloud distribution due to its general paucity over the Southern Ocean region. This approach thus improves the physics of the model with minimal complexity. Text Southern Ocean Copernicus Publications: E-Journals Southern Ocean
institution Open Polar
collection Copernicus Publications: E-Journals
op_collection_id ftcopernicus
language English
description Insufficient reflection of short-wave radiation especially over the Southern Ocean region is still a leading issue in many present-day global climate models. One of the potential reasons for this observed bias is an inadequate representation of clouds. In a previous study, we modified the cloud micro-physics scheme in the Unified Model and showed that choosing a more realistic value for the capacitance or shape parameter of atmospheric ice-crystals, in better agreement with theory and observations, benefits the simulation of short-wave radiation over the Southern Ocean by brightening the clouds. However, attempts to modify the cloud phase by directly adjusting the micro-physics process rates like capacitance tend to affect both the hemispheres symmetrically whereas we seek to brighten only the high-latitude Southern Hemisphere clouds. In this study we implement a simple prognostic parametrisation whereby the heterogeneous ice nucleation temperature is made to vary three-dimensionally as a function of the mineral dust distribution in the model. As a result, those regions with less dust number density would have lower nucleation temperature compared to the default global value of −10 °C. By using mineral dust as an indicator for ice nucleating particles in the model, this parametrisation thus captures the impact of ice nucleating particles on the cloud distribution due to its general paucity over the Southern Ocean region. This approach thus improves the physics of the model with minimal complexity.
format Text
author Varma, Vidya
Morgenstern, Olaf
Furtado, Kalli
Field, Paul
Williams, Jonny
spellingShingle Varma, Vidya
Morgenstern, Olaf
Furtado, Kalli
Field, Paul
Williams, Jonny
Introducing Ice Nucleating Particles functionality into the Unified Model and its impact on the Southern Ocean short-wave radiation biases
author_facet Varma, Vidya
Morgenstern, Olaf
Furtado, Kalli
Field, Paul
Williams, Jonny
author_sort Varma, Vidya
title Introducing Ice Nucleating Particles functionality into the Unified Model and its impact on the Southern Ocean short-wave radiation biases
title_short Introducing Ice Nucleating Particles functionality into the Unified Model and its impact on the Southern Ocean short-wave radiation biases
title_full Introducing Ice Nucleating Particles functionality into the Unified Model and its impact on the Southern Ocean short-wave radiation biases
title_fullStr Introducing Ice Nucleating Particles functionality into the Unified Model and its impact on the Southern Ocean short-wave radiation biases
title_full_unstemmed Introducing Ice Nucleating Particles functionality into the Unified Model and its impact on the Southern Ocean short-wave radiation biases
title_sort introducing ice nucleating particles functionality into the unified model and its impact on the southern ocean short-wave radiation biases
publishDate 2021
url https://doi.org/10.5194/acp-2021-438
https://acp.copernicus.org/preprints/acp-2021-438/
geographic Southern Ocean
geographic_facet Southern Ocean
genre Southern Ocean
genre_facet Southern Ocean
op_source eISSN: 1680-7324
op_relation doi:10.5194/acp-2021-438
https://acp.copernicus.org/preprints/acp-2021-438/
op_doi https://doi.org/10.5194/acp-2021-438
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