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首页> 外文期刊>Journal of Geophysical Research, D. Atmospheres: JGR >Long‐term observations of the wind field in the Antarctic and Arctic mesosphere and lower‐thermosphere at conjugate latitudes
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Long‐term observations of the wind field in the Antarctic and Arctic mesosphere and lower‐thermosphere at conjugate latitudes

机译:长期观测的风场南极和北极中间层在共轭纬度低量热大气层

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摘要

Mean winds, semidiurnal and diurnal tides, and trends and long‐period oscillations spanning a solar cycle (from early 1999 through June 2010) measured by medium frequency (MF) radars at conjugate Antarctic and Arctic latitudes (Syowa, Antarctica, 69°S, 39.6°E, and Andenes, Norway, 69.3°N, 16°E) are described and compared. Zonal mean winds are stronger and more uniform from year to year over the Antarctic, with a stronger eastward winter jet spanning the range of altitudes presented (70 to 96 km). The summer westward jet is also stronger and maximizes at higher altitudes over the Antarctic than over the Arctic. The eastward winter jet over the Arctic, while generally weaker, exhibits a localized maximum in late winter at ~2 to 3 year intervals. Meridional mean winds likewise achieve somewhat stronger maxima at higher altitudes over the Antarctic than over the Arctic. Semidiurnal tide amplitudes are typically somewhat larger over the Antarctic and similar in the two components, with maxima at ~85 km or above and narrow responses that tend to cluster from ~February to May and ~September to November over the Antarctic and from ~December to February and ~June to September over the Arctic. Zonal diurnal tide amplitudes are quite similar between the sites, with maxima extending from ~70 to 90 km and slightly stronger over the Antarctic. Meridional diurnal amplitudes display more significant growth with altitude, achieve stronger maxima at the highest altitudes presented, and typically exhibit a single and narrow maximum during December to February over the Antarctic and double maxima from ~May to September over the Arctic. Also discussed are trends and long‐period oscillations over a solar cycle observed in these mean and tidal wind fields.
机译:意思是风,半日、全日潮和趋势和长期周期振荡生成一个太阳活动周期(从1999年初到2010年6月)衡量中频(MF)雷达共轭南极和北极高纬度地区(Syowa南极洲,69°S, 39.6°E,然后,挪威,69.3°N, 16°E)并对其优缺点进行了比较。风是更强大和更均匀每年在南极,更强东冬天飞机跨越的范围海拔(70到96公里)。西飞机也越来越最大化南极上空的高海拔地区北极。虽然普遍较弱,展品本地化在冬末最大间隔~ 2到3年。子午意味着风同样实现在高海拔的最大值南极北极上空。振幅通常更大了南极和类似的两个组件,maxima ~ 85公里或以上和狭窄的反应倾向于从2 ~ 5月和集群~ 9月至11月在南极12月~ 2月~ 6月到9月在北极。网站之间非常相似,最大值吗扩展从70 ~ 90公里,略强在南极。显示更重要的增长与高度,实现更强的最大值在最高海拔,并给出了典型的单一和展览狭窄的最大12月到2月期间南极和双maxima ~ 59月在北极。在一个太阳能趋势和长期周期振荡在这些的意思是风和潮汐循环观察字段。

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