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首页> 外文期刊>Journal of atmospheric and solar-terrestrial physics >Seasonal variation of the auroral E-region neutral wind for different solar activities
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Seasonal variation of the auroral E-region neutral wind for different solar activities

机译:不同太阳活动的极光E区中性风的季节变化

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Seasonal variations in the auroral E-region neutral wind for different solar activity periods are studied. This work is based on neutral wind data obtained over 56 days between 95-119 km altitude under geomagnetic quiet conditions (A_p<16) during one solar cycle by the European Incoherent Scatter radar located in northern Scandinavia. In general, the meridional mean wind shifts northward, and the zonal mean wind increases in eastward amplitude from winter to summer. The zonal mean wind blows eastward in the middle and lower E-region for each season and for each solar condition except for the equinox, where the zonal mean wind blows westward at and below 104 km. Solar activity dependence of the mean wind exists during the winter and equinox seasons, while in summer it is less prominent. Under high solar activity conditions, the altitude profiles of the horizontal mean winds in winter and the equinoxes tend to resemble those in summer. The horizontal diurnal tide is less sensitive to solar activity except during summer when the meridional amplitude increases by approx 10 m s~(-1) and the corresponding phase shifts to a later time period (1-2 h) during high solar activity. Seasonal dependence of the semidiurnal tide is complex, but is found to vary with solar activity. Under low solar activity conditions the horizontal semidiurnal amplitude shows seasonal dependence except at upper E-region heights, while under high solar activity conditions it becomes less sensitive to seasonal effects (except for the meridional component above 107 km). Comparisons of mean winds with LF and UARS observations are made, and the driving forces for the horizontal mean winds are discussed for various conditions.
机译:研究了不同太阳活动时期的极光E区中性风的季节性变化。这项工作是基于位于北欧斯堪的纳维亚半岛的欧洲非相干散射雷达在一个太阳周期内,在地磁安静条件下(A_p <16)在95-119 km高度之间的56天中空风数据获得的。通常,子午平均风向北移动,纬向平均风从冬季到夏季向东增加。除春分点外,每个季节和每种太阳条件,纬向平均风在中部和下部E区向东吹,春分线在104 km及以下向东吹。平均风对太阳活动的依赖性在冬季和春分季节存在,而在夏季则不那么明显。在高太阳活动条件下,冬季水平平均风的高度剖面和夏季的春分点往往类似于夏季。除了在夏季,子午线幅值增加约10 m s〜(-1),并且在高太阳活动期间相应的相移移至较晚的时间段(1-2 h)以外,水平日潮对太阳活动的敏感性较小。半昼夜潮的季节依赖性很复杂,但是发现随太阳活动而变化。在低太阳活动条件下,水平半日振幅显示出季节依赖性,除了在较高的E区高度处;而在高太阳活动条件下,其对季节影响变得不那么敏感(除了107 km以上的子午分量)。用LF和UARS观测值比较了平均风,并讨论了各种条件下水平平均风的驱动力。

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