Forward and inverse kinetic energy cascades in Jupiter’s turbulent weather layer
Jupiter’s turbulent weather layer contains phenomena of many different sizes, from local storms up to the Great Red Spot and banded jets. The global circulation is driven by complex interactions with (as yet uncertain) small scale processes. We have calculated structure functions and kinetic energy...
Main Authors: | Young, R, Read, P |
---|---|
Format: | Journal article |
Language: | English |
Published: |
Nature Publishing Group
2017
|
Similar Items
-
The turbulent dynamics of Jupiter’s and Saturn’s weather layers: order out of chaos?
by: Read, PL, et al.
Published: (2020) -
Simulating Jupiter's weather layer. Part II: Passive ammonia and water cycles
by: Young, R, et al.
Published: (2018) -
GCM representation of turbulence on Jupiter
by: Zuchowski, L, et al.
Published: (2007) -
The dynamics of Jupiter’s and Saturn’s weather layers: a synthesis after Cassini and Juno
by: Read, P
Published: (2024) -
Simulating Jupiter’s weather layer. Part I: Jet spin-up in a dry atmosphere
by: Young, R, et al.
Published: (2018)