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Some observations on the role of planetary waves in determining the spring time ozone distribution in the Antarctic

 

作者: S. Chandra,   R. D. McPeters,  

 

期刊: Geophysical Research Letters  (WILEY Available online 1986)
卷期: Volume 13, issue 12  

页码: 1224-1227

 

ISSN:0094-8276

 

年代: 1986

 

DOI:10.1029/GL013i012p01224

 

数据来源: WILEY

 

摘要:

Ozone measurements from 1970 to 1984 from the Nimbus 4 backscattered ultraviolet (BUV) and the Nimbus 7 solar backscattered ultraviolet (SBUV) spectrometers show significant decrease in total ozone only after 1979. The downward trend is most apparent in October south of 70°S in the longitude zone 0° to 30°W where planetary wave activity is weak. Outside this longitude region, the trend in total Ozone is much smaller due to strong interannual variability of wave activity. This paper gives a phenomenological description of ozone depletion in the Antarctic region based on vertical advection and transient planetary wav

 

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