On the correction of temperatures derived from meteor wind radars due to geomagnetic activity

C. M. Hall, M. G. Johnsen
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Abstract

Abstract Radars used to observe meteor trails in the mesosphere deliver information on winds and temperature. Use of these radars is becoming a standard method for determining mesospheric dynamics and temperatures worldwide due to relatively low costs and ease of deployment. However, recent studies have revealed that temperatures may be overestimated in conditions such as high geomagnetic activity. The effect is thought to be most prevalent at high latitude, although this is not yet proven. Here, we demonstrate how temperatures might be corrected for geomagnetic effects; the demonstration is for a particular geographic location (Svalbard, 78°N, 16°E) because it is local geomagnetic disturbances that affects local temperature measurements, therefore requiring co-located instruments. We see that summer temperatures require a correction (reduction) of a few Kelvin, but winter estimates are more accurate.
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地磁活动对流星风雷达温度的校正
用于观测中间层流星轨迹的雷达提供有关风和温度的信息。由于成本相对较低且易于部署,使用这些雷达正在成为全球范围内确定中间层动力学和温度的标准方法。然而,最近的研究表明,在高地磁活动等条件下,温度可能被高估了。这种效应被认为在高纬度地区最为普遍,尽管这一点尚未得到证实。在这里,我们演示了如何根据地磁效应对温度进行校正;该演示是针对一个特定的地理位置(Svalbard, 78°N, 16°E),因为它是局部地磁干扰,影响局部温度测量,因此需要同时放置仪器。我们看到夏天的温度需要修正(降低)几个开尔文,但冬天的估计更准确。
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