Wave interactions and baroclinic chaos: A paradigm for long timescale variability in planetary atmospheres
Baroclinic instability is the principal mode of non-axisymmetric flow in the large-scale atmospheric circulation at mid-latitudes, and is responsible for oganising the structure and behaviour of major weather systems. This instability can also be fruitfully studied in the laboratory under controlled...
Main Authors: | Read, P, Collins, M, Fruh, W, Lewis, SR, Lovegrove, A |
---|---|
Format: | Conference item |
Published: |
1998
|
Similar Items
-
Baroclinic wave transitions in the Martian atmosphere
by: Collins, M, et al.
Published: (1996) -
Wave interactions and the transition to chaos of baroclinic waves in a thermally driven rotating annulus
by: Fruh, W, et al.
Published: (1997) -
Sloping convection: A paradigm for large-scale waves and eddies in planetary atmospheres?
by: Hide, R, et al.
Published: (1994) -
Baroclinic and barotropic instabilities in planetary atmospheres: energetics, equilibration and adjustment
by: Read, P, et al.
Published: (2020) -
APPLICATIONS OF SINGULAR SYSTEMS-ANALYSIS TO BAROCLINIC CHAOS
by: Read, P
Published: (1992)