Arctic Climate Response to European Radiative Forcing: A Deep Learning Approach

Heterogeneous radiative forcing in mid-latitudes, such as that exerted by aerosols, has been found to affect the Arctic climate, though the mechanisms remain debated. In this study, we leverage Deep Learning (DL) techniques to explore the complex response of the Arctic climate system to local radiat...

Full description

Bibliographic Details
Main Authors: Mehrdad, Sina, Handorf, Dörthe, Höschel, Ines, Karami, Khalil, Quaas, Johannes, Dipu, Sudhakar, Jacobi, Christoph
Format: Text
Language:English
Published: 2024
Subjects:
Online Access:https://doi.org/10.5194/egusphere-2023-3033
https://egusphere.copernicus.org/preprints/2024/egusphere-2023-3033/
id ftcopernicus:oai:publications.copernicus.org:egusphere117038
record_format openpolar
spelling ftcopernicus:oai:publications.copernicus.org:egusphere117038 2024-09-15T18:16:11+00:00 Arctic Climate Response to European Radiative Forcing: A Deep Learning Approach Mehrdad, Sina Handorf, Dörthe Höschel, Ines Karami, Khalil Quaas, Johannes Dipu, Sudhakar Jacobi, Christoph 2024-01-18 application/pdf https://doi.org/10.5194/egusphere-2023-3033 https://egusphere.copernicus.org/preprints/2024/egusphere-2023-3033/ eng eng doi:10.5194/egusphere-2023-3033 https://egusphere.copernicus.org/preprints/2024/egusphere-2023-3033/ eISSN: Text 2024 ftcopernicus https://doi.org/10.5194/egusphere-2023-3033 2024-08-28T05:24:15Z Heterogeneous radiative forcing in mid-latitudes, such as that exerted by aerosols, has been found to affect the Arctic climate, though the mechanisms remain debated. In this study, we leverage Deep Learning (DL) techniques to explore the complex response of the Arctic climate system to local radiative forcing over Europe. We conducted sensitivity experiments using the Max Planck Institute Earth System Model (MPI-ESM1.2) coupled with atmosphere-ocean–land surface components. Utilizing a DL-based clustering method, we classify atmospheric circulation patterns in a lower-dimensional space, focusing on Poleward Moist Static Energy Transport (PMSET) as our primary parameter. We developed a novel method to analyze the circulation patterns' contributions to various climatic parameter anomalies. Our findings indicate that the negative forcing over Europe alters existing circulation patterns and their occurrence frequency without introducing new ones. Specifically, we identify changes in a circulation pattern with a high-pressure system over Scandinavia as a key driver for reduced Sea Ice Concentration (SIC) in the Barents-Kara Sea during autumn. This circulation pattern also influences middle atmospheric dynamics, although its contribution is relatively minor compared to other circulation patterns that resemble the phases of the North Atlantic Oscillation (NAO). Our multidimensional approach combines DL algorithms and human expertise to offer a novel analytical tool that could have broader applications in climate science. Text Kara Sea North Atlantic North Atlantic oscillation Sea ice Copernicus Publications: E-Journals
institution Open Polar
collection Copernicus Publications: E-Journals
op_collection_id ftcopernicus
language English
description Heterogeneous radiative forcing in mid-latitudes, such as that exerted by aerosols, has been found to affect the Arctic climate, though the mechanisms remain debated. In this study, we leverage Deep Learning (DL) techniques to explore the complex response of the Arctic climate system to local radiative forcing over Europe. We conducted sensitivity experiments using the Max Planck Institute Earth System Model (MPI-ESM1.2) coupled with atmosphere-ocean–land surface components. Utilizing a DL-based clustering method, we classify atmospheric circulation patterns in a lower-dimensional space, focusing on Poleward Moist Static Energy Transport (PMSET) as our primary parameter. We developed a novel method to analyze the circulation patterns' contributions to various climatic parameter anomalies. Our findings indicate that the negative forcing over Europe alters existing circulation patterns and their occurrence frequency without introducing new ones. Specifically, we identify changes in a circulation pattern with a high-pressure system over Scandinavia as a key driver for reduced Sea Ice Concentration (SIC) in the Barents-Kara Sea during autumn. This circulation pattern also influences middle atmospheric dynamics, although its contribution is relatively minor compared to other circulation patterns that resemble the phases of the North Atlantic Oscillation (NAO). Our multidimensional approach combines DL algorithms and human expertise to offer a novel analytical tool that could have broader applications in climate science.
format Text
author Mehrdad, Sina
Handorf, Dörthe
Höschel, Ines
Karami, Khalil
Quaas, Johannes
Dipu, Sudhakar
Jacobi, Christoph
spellingShingle Mehrdad, Sina
Handorf, Dörthe
Höschel, Ines
Karami, Khalil
Quaas, Johannes
Dipu, Sudhakar
Jacobi, Christoph
Arctic Climate Response to European Radiative Forcing: A Deep Learning Approach
author_facet Mehrdad, Sina
Handorf, Dörthe
Höschel, Ines
Karami, Khalil
Quaas, Johannes
Dipu, Sudhakar
Jacobi, Christoph
author_sort Mehrdad, Sina
title Arctic Climate Response to European Radiative Forcing: A Deep Learning Approach
title_short Arctic Climate Response to European Radiative Forcing: A Deep Learning Approach
title_full Arctic Climate Response to European Radiative Forcing: A Deep Learning Approach
title_fullStr Arctic Climate Response to European Radiative Forcing: A Deep Learning Approach
title_full_unstemmed Arctic Climate Response to European Radiative Forcing: A Deep Learning Approach
title_sort arctic climate response to european radiative forcing: a deep learning approach
publishDate 2024
url https://doi.org/10.5194/egusphere-2023-3033
https://egusphere.copernicus.org/preprints/2024/egusphere-2023-3033/
genre Kara Sea
North Atlantic
North Atlantic oscillation
Sea ice
genre_facet Kara Sea
North Atlantic
North Atlantic oscillation
Sea ice
op_source eISSN:
op_relation doi:10.5194/egusphere-2023-3033
https://egusphere.copernicus.org/preprints/2024/egusphere-2023-3033/
op_doi https://doi.org/10.5194/egusphere-2023-3033
_version_ 1810454199504207872