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Thermal conditions for PMC existence derived from Odin/OSIRIS and TIMED/SABER data

机译:来自Odin / OSIRIS和TIMED / SABER数据的PMC存在的热条件

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We study a relationship between Polar Mesospheric Cloud (PMC) brightness and coincident mesospheric Kinetic Temperatures (KT) measured by two satellite instruments, the Optical Spectrograph and Infrared Imager System and Sounding of the Atmosphere using Broadband Emission Radiometry respectively. Two fifteen-day periods in July 2002 and 2003 have been analyzed. For coincidences <= 3 hours and <= 200 km PMCs with a peak at 82-84 km were observed for the mean KT in this height range <= 142 K. Bright PMCs, at least twice brighter than the seasonal mean, were detected only for KT <= 134 K. The average KT for PMCs at 80 degrees-82.2 degrees N was lower than that at 60 degrees-75 degrees N by 5-8 K. The average KT coincident with PMCs was 1.4 to 7.9 K lower than that for non-PMC cases. There was up to 7% of non-PMC detections for the very low KT, <= 130 K. The total random and systematic uncertainty of this analysis was 9 K.
机译:我们研究了极地中层云(PMC)亮度和同时由两个卫星仪器(光谱仪和红外成像仪系统)和使用宽带发射辐射法测量的大气探测的同时中层运动温度(KT)之间的关系。分析了2002年7月和2003年的两个十五天期间。巧合的是,在此高度范围<= 142 K中,平均KT小于等于3小时且小于等于200 km的PMC在82-84 km处达到峰值。仅检测到明亮的PMC,其亮度至少是季节性平均值的两倍当KT <= 134 K时。在80度至82.2度N下,PMC的平均KT比在60度至75度N下的平均KT低5-8K。与PMC一致的平均KT比其低1.4-7.9 K对于非PMC案件。对于非常低的KT,<= 130 K,最多有7%的非PMC检测到。该分析的总的随机和系统不确定性是9K。

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