The KNMI Large Ensemble Time Slice (KNMI-LENTIS)
Large-ensemble modelling has become an increasingly popular approach to studying the mean climate and the climate system’s internal variability in response to external forcing. Here we present the Royal Netherlands Meteorological Institute (KNMI) Large Ensemble Time Slice (KNMI–LENTIS): a new large...
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ftcopernicus:oai:publications.copernicus.org:egusphere108124 2023-09-05T13:13:07+02:00 The KNMI Large Ensemble Time Slice (KNMI-LENTIS) Muntjewerf, Laura Bintanja, Richard Reerink, Thomas Wiel, Karin 2023-08-11 application/pdf https://doi.org/10.5194/egusphere-2022-1378 https://egusphere.copernicus.org/preprints/2023/egusphere-2022-1378/ eng eng doi:10.5194/egusphere-2022-1378 https://egusphere.copernicus.org/preprints/2023/egusphere-2022-1378/ eISSN: Text 2023 ftcopernicus https://doi.org/10.5194/egusphere-2022-1378 2023-08-14T16:24:22Z Large-ensemble modelling has become an increasingly popular approach to studying the mean climate and the climate system’s internal variability in response to external forcing. Here we present the Royal Netherlands Meteorological Institute (KNMI) Large Ensemble Time Slice (KNMI–LENTIS): a new large ensemble produced with the re-tuned version of the global climate model EC-Earth3. The ensemble consists of two distinct time slices of 10 years each: a present-day time slice and a +2 K warmer future time slice relative to the present day. The initial conditions for the ensemble members are generated with a combination of micro- and macro-perturbations. The 10-year length of a single time slice is assumed to be too short to show a significant forced climate change signal, and the ensemble size of 1600 years (160 × 10 years) is assumed to be sufficient to sample the full distribution of climate variability. The time slice approach makes it possible to study extreme events on sub-daily timescales as well as events that span multiple years such as multi-year droughts and preconditioned compound events. KNMI–LENTIS is therefore uniquely suited to study internal variability and extreme events both at a given climate state and resulting from forced changes due to external radiative forcing. A unique feature of this ensemble is the high temporal output frequency of the surface water balance and surface energy balance variables, which are stored in 3-hourly intervals, allowing for detailed studies into extreme events. The large ensemble is particularly geared towards research in the land–atmosphere domain. EC-Earth3 has a considerable warm bias in the Southern Ocean and over Antarctica. Hence, users of KNMI–LENTIS are advised to make in-depth comparisons with observational or reanalysis data, especially if their studies focus on ocean processes, on locations in the Southern Hemisphere, or on teleconnections involving both hemispheres. In this paper, we will give some examples to demonstrate the added value of KNMI–LENTIS for ... Text Antarc* Antarctica Southern Ocean Copernicus Publications: E-Journals Southern Ocean |
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Copernicus Publications: E-Journals |
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English |
description |
Large-ensemble modelling has become an increasingly popular approach to studying the mean climate and the climate system’s internal variability in response to external forcing. Here we present the Royal Netherlands Meteorological Institute (KNMI) Large Ensemble Time Slice (KNMI–LENTIS): a new large ensemble produced with the re-tuned version of the global climate model EC-Earth3. The ensemble consists of two distinct time slices of 10 years each: a present-day time slice and a +2 K warmer future time slice relative to the present day. The initial conditions for the ensemble members are generated with a combination of micro- and macro-perturbations. The 10-year length of a single time slice is assumed to be too short to show a significant forced climate change signal, and the ensemble size of 1600 years (160 × 10 years) is assumed to be sufficient to sample the full distribution of climate variability. The time slice approach makes it possible to study extreme events on sub-daily timescales as well as events that span multiple years such as multi-year droughts and preconditioned compound events. KNMI–LENTIS is therefore uniquely suited to study internal variability and extreme events both at a given climate state and resulting from forced changes due to external radiative forcing. A unique feature of this ensemble is the high temporal output frequency of the surface water balance and surface energy balance variables, which are stored in 3-hourly intervals, allowing for detailed studies into extreme events. The large ensemble is particularly geared towards research in the land–atmosphere domain. EC-Earth3 has a considerable warm bias in the Southern Ocean and over Antarctica. Hence, users of KNMI–LENTIS are advised to make in-depth comparisons with observational or reanalysis data, especially if their studies focus on ocean processes, on locations in the Southern Hemisphere, or on teleconnections involving both hemispheres. In this paper, we will give some examples to demonstrate the added value of KNMI–LENTIS for ... |
format |
Text |
author |
Muntjewerf, Laura Bintanja, Richard Reerink, Thomas Wiel, Karin |
spellingShingle |
Muntjewerf, Laura Bintanja, Richard Reerink, Thomas Wiel, Karin The KNMI Large Ensemble Time Slice (KNMI-LENTIS) |
author_facet |
Muntjewerf, Laura Bintanja, Richard Reerink, Thomas Wiel, Karin |
author_sort |
Muntjewerf, Laura |
title |
The KNMI Large Ensemble Time Slice (KNMI-LENTIS) |
title_short |
The KNMI Large Ensemble Time Slice (KNMI-LENTIS) |
title_full |
The KNMI Large Ensemble Time Slice (KNMI-LENTIS) |
title_fullStr |
The KNMI Large Ensemble Time Slice (KNMI-LENTIS) |
title_full_unstemmed |
The KNMI Large Ensemble Time Slice (KNMI-LENTIS) |
title_sort |
knmi large ensemble time slice (knmi-lentis) |
publishDate |
2023 |
url |
https://doi.org/10.5194/egusphere-2022-1378 https://egusphere.copernicus.org/preprints/2023/egusphere-2022-1378/ |
geographic |
Southern Ocean |
geographic_facet |
Southern Ocean |
genre |
Antarc* Antarctica Southern Ocean |
genre_facet |
Antarc* Antarctica Southern Ocean |
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eISSN: |
op_relation |
doi:10.5194/egusphere-2022-1378 https://egusphere.copernicus.org/preprints/2023/egusphere-2022-1378/ |
op_doi |
https://doi.org/10.5194/egusphere-2022-1378 |
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1776203528103002112 |