The Lorenz energy cycle: trends and the impact of modes of climate variability

The atmospheric circulation is driven by heat transport from the tropics to the polar regions, embedding energy conversions between available potential and kinetic energy through various mechanisms. The processes of energy transformations related to the dynamics of the atmosphere can be quantitative...

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Autores principales: Qiyun Ma, Valerio Lembo, Christian L.E. Franzke
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Publicado: Taylor & Francis Group 2021
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spelling oai:doaj.org-article:e4a8d838b8a64a37b15bd182ee9ae6432021-12-01T14:40:58ZThe Lorenz energy cycle: trends and the impact of modes of climate variability1600-087010.1080/16000870.2021.1900033https://doaj.org/article/e4a8d838b8a64a37b15bd182ee9ae6432021-01-01T00:00:00Zhttp://dx.doi.org/10.1080/16000870.2021.1900033https://doaj.org/toc/1600-0870The atmospheric circulation is driven by heat transport from the tropics to the polar regions, embedding energy conversions between available potential and kinetic energy through various mechanisms. The processes of energy transformations related to the dynamics of the atmosphere can be quantitatively investigated through the Lorenz energy cycle formalism. Here we examine these variations and the impacts of modes of climate variability on the Lorenz energy cycle by using reanalysis data from the Japanese Meteorological Agency (JRA-55). We show that the atmospheric circulation is overall becoming more energetic and efficient. For instance, we find a statistically significant trend in the eddy available potential energy, especially in the transient eddy available potential energy in the Southern Hemisphere. We find significant trends in the conversion rates between zonal available potential and kinetic energy, consistent with an expansion of the Hadley cell, and in the conversion rates between eddy available potential and kinetic energy, suggesting an increase in mid-latitudinal baroclinic instability. We also show that planetary-scale waves dominate the stationary eddy energy, while synoptic-scale waves dominate the transient eddy energy with a significant increasing trend. Our results suggest that interannual variability of the Lorenz energy cycle is determined by modes of climate variability. We find that significant global and hemispheric energy fluctuations are caused by the El Nino-Southern Oscillation, the Arctic Oscillation, the Southern Annular Mode, and the meridional temperature gradient over the Southern Hemisphere.Qiyun MaValerio LemboChristian L.E. FranzkeTaylor & Francis Grouparticlelorenz energy cycleclimate variabilitytrendsOceanographyGC1-1581Meteorology. ClimatologyQC851-999ENTellus: Series A, Dynamic Meteorology and Oceanography, Vol 73, Iss 1, Pp 1-15 (2021)
institution DOAJ
collection DOAJ
language EN
topic lorenz energy cycle
climate variability
trends
Oceanography
GC1-1581
Meteorology. Climatology
QC851-999
spellingShingle lorenz energy cycle
climate variability
trends
Oceanography
GC1-1581
Meteorology. Climatology
QC851-999
Qiyun Ma
Valerio Lembo
Christian L.E. Franzke
The Lorenz energy cycle: trends and the impact of modes of climate variability
description The atmospheric circulation is driven by heat transport from the tropics to the polar regions, embedding energy conversions between available potential and kinetic energy through various mechanisms. The processes of energy transformations related to the dynamics of the atmosphere can be quantitatively investigated through the Lorenz energy cycle formalism. Here we examine these variations and the impacts of modes of climate variability on the Lorenz energy cycle by using reanalysis data from the Japanese Meteorological Agency (JRA-55). We show that the atmospheric circulation is overall becoming more energetic and efficient. For instance, we find a statistically significant trend in the eddy available potential energy, especially in the transient eddy available potential energy in the Southern Hemisphere. We find significant trends in the conversion rates between zonal available potential and kinetic energy, consistent with an expansion of the Hadley cell, and in the conversion rates between eddy available potential and kinetic energy, suggesting an increase in mid-latitudinal baroclinic instability. We also show that planetary-scale waves dominate the stationary eddy energy, while synoptic-scale waves dominate the transient eddy energy with a significant increasing trend. Our results suggest that interannual variability of the Lorenz energy cycle is determined by modes of climate variability. We find that significant global and hemispheric energy fluctuations are caused by the El Nino-Southern Oscillation, the Arctic Oscillation, the Southern Annular Mode, and the meridional temperature gradient over the Southern Hemisphere.
format article
author Qiyun Ma
Valerio Lembo
Christian L.E. Franzke
author_facet Qiyun Ma
Valerio Lembo
Christian L.E. Franzke
author_sort Qiyun Ma
title The Lorenz energy cycle: trends and the impact of modes of climate variability
title_short The Lorenz energy cycle: trends and the impact of modes of climate variability
title_full The Lorenz energy cycle: trends and the impact of modes of climate variability
title_fullStr The Lorenz energy cycle: trends and the impact of modes of climate variability
title_full_unstemmed The Lorenz energy cycle: trends and the impact of modes of climate variability
title_sort lorenz energy cycle: trends and the impact of modes of climate variability
publisher Taylor & Francis Group
publishDate 2021
url https://doaj.org/article/e4a8d838b8a64a37b15bd182ee9ae643
work_keys_str_mv AT qiyunma thelorenzenergycycletrendsandtheimpactofmodesofclimatevariability
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