Tidal periodicities in observations of the OH(6-2) emission from Mawson, Antarctica.

被引：2
|
作者：
Greet, PA
Dyson, PL
机构：
[1] Australian Antarctic Div, Kingston, Tas 7050, Australia
[2] La Trobe Univ, Sch Phys, Bundoora, Vic 3083, Australia
来源：
MESOPAUSE AND EXTRA-TERRESTRIAL INFLUENCES ON THE OZONE LAYER | 1999年 / 24卷 / 05期
基金：
澳大利亚研究理事会;
关键词：
D O I：
10.1016/S0273-1177(99)00204-5
中图分类号：
V [航空、航天];
学科分类号：
08 ; 0825 ;
摘要：
High-resolution Fabry-Perot spectrometer observations of the OH (6-2) Q(1)(1) line, lambda 834.460 nm, have been made at Mawson, Antarctica on a limited campaign basis since 1993. In August 1995, some data were obtained on 14 days in a 15 day period. Periodicities have been identified using the Lomb-Scargle technique. The most significant periodicity in the zonal wind and the meridional wind and intensity is at twelve hours. These results are compared with other measurements and a model of high latitude semidiurnal tidal oscillations. (C) 1999 COSPAR. Published by Elsevier Science Ltd.
引用
收藏
页码：579 / 582
页数：4
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