Revealing the Intensity of Turbulent Energy Transfer in Planetary Atmospheres-Reference-Cited by-同舟云学术

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Revealing the Intensity of Turbulent Energy Transfer in Planetary Atmospheres

Published:2020-12-08 Issue:23 Volume:47 Page:
ISSN:0094-8276
Container-title:Geophysical Research Letters
language:en
Short-container-title:Geophys. Res. Lett.

Author:

Cabanes Simon¹^ORCID,Espa Stefania¹^ORCID,Galperin Boris²^ORCID,Young Roland M. B.³^ORCID,Read Peter L.⁴^ORCID

Affiliation:

1. DICEA Sapienza Universitá di Roma Rome Italy

2. College of Marine Science University of South Florida St. Petersburg FL USA

3. Department of Physics and National Space Science and Technology Center UAE University Al Ain United Arab Emirates

4. Atmospheric, Oceanic and Planetary Physics, Department of Physics University of Oxford Oxford UK

Funder

Seventh Framework Programme

Publisher

American Geophysical Union (AGU)

Subject

General Earth and Planetary Sciences,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1029/2020GL088685

Reference40 articles.

1. Geostrophic Turbulence in the Frequency–Wavenumber Domain: Eddy-Driven Low-Frequency Variability*

2. A New Formulation of the Spectral Energy Budget of the Atmosphere, with Application to Two High-Resolution General Circulation Models

3. Homogeneous and Isotropic Turbulence on the Sphere

4. Evidence for the double cascade scenario in two-dimensional turbulence

5. Global climate modeling of Saturn's atmosphere. Part III: Global statistical picture of zonostrophic turbulence in high-resolution 3D-turbulent simulations

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