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首页> 外文期刊>Journal of the Atmospheric Sciences >Thermal structure of the mesopause region (80-105 km) at 40 degrees N latitude. Part I: Seasonal variations
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Thermal structure of the mesopause region (80-105 km) at 40 degrees N latitude. Part I: Seasonal variations

机译:中纬度地区(北纬40度)(80-105公里)的热结构。第一部分:季节性变化

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Sodium wind/temperature lidar measurements taken throughout the diurnal and annual cycles at Urbana, Illinois (40 degrees N, 88 degrees W), from February 1996 through January 1998 are used to characterize the seasonal variations of the mesospheric temperature structure between 80 and 105 km. By averaging data over several weeks and over the complete diurnal cycle, the significant effects of gravity waves, tides, and planetary waves are surpressed. The observed mean annual temperature structure is largely consistent with the assumption of radiative equilibrium between direct solar UV heating and radiative cooling by DR emission. Large seasonal variations of the mean thermal structure are observed. Below 91 gm, there is strong adiabatic coding in summer caused by the mean upward velocities associated with the diabatic circulation system. The maximum amplitude of the annual variation is 9.7 K at approximately 84 km. Above 98 km, Increased UV absorption by O-2 during summer drives an annual oscillation in this region with an amplitude of approximately 5 K. These two phenomena determine the seasonal variation of the mesopause altitude. The annual variation in solar UV heating in the lower thermosphere induces a modest 5-km peak to peak annual variation in the mesopause altitude. The mesopause is near 101 km in winter and similar to 96 km in late summer. However, the summer cooling below 91 km is strong enough to define the minimum temperature, causing the mesopause altitude to fall to similar to 87 km from about 7 May to about 15 July (similar to 70 days). The mesopause thickness, defined here as the altitude range where the temperature is within 5 K of the minimum, increases dramatically from approximately 7 hm in winter to over 16 km in summer. Significant biases can occur in some parameters calculated from nighttime-only observations. The inversion layers that persist between 85 and 96 km in nighttime temperature profiles are virtually eliminated when data are averaged over the complete diurnal period. The strong annual temperature variation present around 84 km is overestimated by 40%, rind the strong semiannual variation above 95 km is overestimated by as much as 150% when computed using only nighttime measurements. The low summer mesopause exists for a much longer period(similar to 126 days) in the nighttime observations. The mesopause temperature averaged over the annual cycle is 188 K compared to 190 K for the nighttime average. This bias is most pronounced during summertime when the difference is 7 K. [References: 38]
机译:从1996年2月至1998年1月,在伊利诺伊州厄巴纳(北纬40度,北纬88度)的整个昼夜和年度周期中测量钠风/温度激光雷达,以表征80至105 km之间中层温度结构的季节性变化。通过对数周和整个昼夜周期内的数据进行平均,可以抑制重力波,潮汐和行星波的重大影响。观测到的年平均温度结构在很大程度上与太阳直射紫外线加热与DR辐射辐射冷却之间的辐射平衡假设相符。观察到平均热结构的季节性大变化。低于91 gm,由于绝热循环系统的平均上升速度,夏季有很强的绝热编码。年变化的最大幅度在大约84 km处为9.7K。在98公里以上,夏季O-2对紫外线的吸收增加,使该区域的年振荡幅度约为5K。这两个现象决定了中年更年期的季节性变化。在较低的热圈中,太阳紫外线加热的年变化引起中绝经高度的5 km峰到峰的年变化。冬季中绝经时间接近101公里,夏末则接近96公里。然而,夏季低于91 km的降温足以确定最低温度,导致从5月7日到7月15日(约70天)的绝经高度下降到约87 km。中腹厚度(此处定义为温度在最小值5 K以内的海拔范围)从冬天的大约7 hm急剧增加到夏天的16 km以上。根据仅夜间观测值计算出的某些参数可能会出现明显偏差。当对整个昼夜周期内的数据进行平均时,夜间温度分布持续在85至96 km之间的反演层实际上被消除了。仅使用夜间测量值计算,在84 km附近存在的强烈的年度温度变化被高估了40%,而在95 km以上存在的强烈的半年度变化被高估了150%。夏季观测到的夏季中低位偏低的时间更长(约126天)。在一年周期中,平均绝经温度为188 K,而夜间平均为190K。在夏季,当差异为7 K时,这种偏差最为明显。[参考文献:38]

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