Thesis
Modelling of equatorial wave motions in the middle atmosphere
- Abstract:
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A three-dimensional mechanistic model of the middle atmosphere is used to model various classes of equatorial wave motions that are observed in the atmosphere. These waves are thought to be largely responsible for the forcing of the quasi-biennial oscillation (QBO) in the tropical lower stratosphere. By generating a combination of different classes of equatorial waves in the model, an oscillation which has many similarities to the observed QBO is produced in the model.
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Authors
Bibliographic Details
- Publication date:
- 1998
- Type of award:
- DPhil
- Level of award:
- Doctoral
- Awarding institution:
- University of Oxford
- Source identifiers:
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603838917
Item Description
- Language:
- English
- Subjects:
- UUID:
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uuid:9ae75869-a15b-465e-af64-c608cca8b34c
- Local pid:
- td:603838917
- Deposit date:
- 2015-02-04
Terms of use
- Copyright holder:
- Drysdale, E
- Copyright date:
- 1998
- Notes:
- This thesis was digitised thanks to the generosity of Dr Leonard Polonsky
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