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: | , , , , |
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| Format: | Conference item |
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1998
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