The Quasi 16-day Waves in the Mesosphere and Lower Thermosphere at Wuhan
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摘要: 利用武汉流星雷达2002年2月20日至2003年11月10日的观测数据,研究了武汉上空中间层低热层(MLT)中的准16日波,即周期范围在12-20天的行星波.分析结果表明,16日波的纬向成分通常比经向成分要强.(1)在2002年和2003年,波振幅最强都出现在当年的秋季(约9月10日-10月10日).Lomb-Scargle(L-S)谱分析得到振幅最大值约为16m/s.2002年夏季出现了同年次最强的波动,但2003年没有发现这一现象.两年的冬季都没有出现强的16日波.(2)2002年,在86-98km处波动较强,最大振幅(约16m/s)出现在90km、94km处而2003年低高度的波动要比较高高度的波动强.武汉上空MLT中,秋季的16日波是能量上传的波动,即它的源在较低的大气层.2002年夏季的波动的能量是下行的,波源可能在南半球.Abstract: Data observed by the Wuhan meteor radar(20 February 2002-10 November 2003) have been used to study the quasi 16-day oscillations in the mesosphere and lower thermosphere(MLT),which is a type of planetary wave with period ranges from 12 to 20 days.The results show that the zonal components are generally stronger than the meridional components.(1) In the year of 2002 and 2003,the largest amplitudes appear in early autumn(10 September-10 October) when the zonal background winds are eastward.The largest amplitude value derived from the Lomb-Scargle(L-S) periodograms is about 16 m/s.A second maximum appears in the summer of 2002,but not in the summer of 2003.There are no strong wave activities in the winter months of both years.(2) In 2002,the 16 day waves are strong from 86 to 98km with the maximum at about 90km to 94km,but they are strong at lower altitudes in 2003.The energy of the 16-day wave propagates upward in autumn,which means the wave originate from lower atmosphere,but the direction of wave energy propagation is downward in summer of 2002,which means the 16-day waves may propagate from the southern hemisphere.
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Key words:
- Meteor radar /
- Mesosphere and lower thermosphere /
- The 16-day waves
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