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
点击下载:
PDF
(323KB)
返 回