The vertical structure of the quasi‐biennial oscillation: Observations and theory

20Citations
Citations of this article
11Readers
Mendeley users who have this article in their library.

This article is free to access.

Abstract

Rocketsonde observations of the zonal wind over Ascension Island (8°S) were analysed to obtain the amplitude and phase of the quasi‐biennial oscillation (QBO) in the height range 25–58 km. It was found that the amplitude peaked at about 30km and decreased rapidly above 40km. In fact, above 45 km there is no clear evidence that a QBO actually exists.A number of simulations using the Holton‐Lindzen model of the QBO were performed. It was found that when the waves in the model were damped with Dickinson's (1973) Newtonian cooling, the simulated QBO extended to higher levels than actually observed. However, when the wavelength‐dependent cooling rates of Fels(1981) were used, a fairly realistic vertical structure resulted. © Taylor & Francis Group, LLC.

Cite

CITATION STYLE

APA

Hamilton, K. (1981). The vertical structure of the quasi‐biennial oscillation: Observations and theory. Atmosphere - Ocean, 19(3), 236–250. https://doi.org/10.1080/07055900.1981.9649111

Register to see more suggestions

Mendeley helps you to discover research relevant for your work.

Already have an account?

Save time finding and organizing research with Mendeley

Sign up for free