EGU23-6254
https://doi.org/10.5194/egusphere-egu23-6254
EGU General Assembly 2023
© Author(s) 2023. This work is distributed under
the Creative Commons Attribution 4.0 License.

Spectral Resolution of the Oceans Lorenz Energy Cycle

Jan Niklas Dettmer
Jan Niklas Dettmer
  • Universität Hamburg, Institut für Meereskunde, Germany (jan.niklas.dettmer@gmail.com)

Eddy kinetic energy (EKE) and the conversion terms of the Lorenz energy cycle are estimated from an eddy-resolving global ocean model and resolved spectrally per horizontal wavenumber. The baroclinic conversion term (BC) exhibits a dipolar structure, where it is a source for EKE at scales close to the first baroclinic Rossby radius and a sink for EKE at larger scales close to the Rhines scale. The geographical and vertical distributions of the BC term are explored. It is found that in the ocean interior negative BC is limited to regions poleward of approximately 30° north and south. It is suggested that the cause for this distribution is the transfer of eddy energy to Rossby waves and zonal jets equatorward of 30°. It removes eddy energy before it cascades up to the scale where negative BC takes place. Equatorward of 30° the existence of a closed energy loop is suggested. Positive BC produces EKE which cascades upscale where it is converted to available eddy potential energy (EAPE) by negative BC, which cascades downscale again. The sink of EKE partly balances the EKE produced by baroclinic instability. The energy loop traps a certain amount of energy. Finally, the baroclinic conversion term is explored further in idealized model setups. The goal of the idealized setups is to test the robustness of the diagnostic methods and gain physical understanding of the negative baroclinic conversion.

How to cite: Dettmer, J. N.: Spectral Resolution of the Oceans Lorenz Energy Cycle, EGU General Assembly 2023, Vienna, Austria, 24–28 Apr 2023, EGU23-6254, https://doi.org/10.5194/egusphere-egu23-6254, 2023.