Kolhapur (16.8oN, 74.2 e)上空中层和低层热层平均风的变率研究

Q4 Computer Science
G.P. Naniwadekar, S. Gurubaran, A.P. Jadhav, R. Ghodpage, P. Patil, D. Burud
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引用次数: 0

摘要

我们利用位于印度Kolhapur(16.8°N,74.2°E)的部分反射雷达站(MF–雷达)的观测结果,对78–98公里高度范围内的中层风进行了研究。本研究使用了该雷达在1.98 MHz下运行时获得的2014-2019年期间的连续风廓线。为了描述中层和低热层(MLT)区域的风的行为,我们使用了提供一小时平均水平风速的风数据。详细介绍了上述时期MLT区域纬向(东西)和经向(南北)分量的季节、年度和年际变化,以及平均运动的气候学。观测到90公里以下的纬向风,在至点期间向东流动,在春分时向西流动,显示出强烈的半年振荡(SAO)。当超过90公里时,年振荡(AO)占主导地位。在平均经向风中观测到年振荡(AO),冬季向极地运动,其余季节向赤道运动。在更高的海拔(92公里以上),极地运动减弱,向赤道方向的气流变强。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Studies on the variability of mean winds in the mesosphere and lower thermosphere region (MLT) over Kolhapur (16.8oN, 74.2oE)
We present the study of mesospheric winds in the 78–98 km height range using observations by a partial reflection radar station (MF–radar) situated at Kolhapur (16.8° N, 74.2° E), India. The sequential wind profiles over the period of 2014–2019 obtained from this radar operated at 1.98 MHz are used for this study. To delineate the behaviour of the winds in the mesosphere and lower thermosphere (MLT) region, we use wind data providing horizontal wind velocities averaged for an hour. Details of the seasonal, annual, and inter-annual variations and also the climatology of mean motion in zonal (East-West) and meridional (North-South) components in the MLT region over the aforementioned period are presented. The zonal wind below 90 km has been observed with eastward flow for the period of solstices and westward flow at equinoxes, showing strong semi-annual oscillations (SAO). While above 90 km, annual oscillations (AO) are seen to be dominant. Annual oscillations (AO) are observed in the mean meridional wind, with poleward motion during winter and equatorward motion during the remaining seasons. At higher altitudes (above 92 km), the poleward motion weakens and the equatorward wind flow becomes strong.
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来源期刊
测绘地理信息
测绘地理信息 Earth and Planetary Sciences-Earth-Surface Processes
CiteScore
0.20
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4458
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