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The effects of atmospheric waves on the amounts of polar stratospheric clouds

机译:大气波对极地平流层云量的影响

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A quantitative analysis on the relationship between atmospheric waves and polar stratospheric clouds (PSCs) in the 2008 austral winter and the 2007/2008 boreal winter is made using CALIPSO, COSMIC and Aura MLS observation data and reanalysis data. A longitude-time section of the frequency of PSC occurrence in the Southern Hemisphere indicates that PSC frequency is not regionally uniform and that high PSC frequency regions propagate eastward at different speeds from the background zonal wind. These features suggest a significant influence of atmospheric waves on PSC behavior. Next, three temperature thresholds for PSC existence are calculated using HNO3 and H2O mixing ratios. Among the three, the TSTS (a threshold for super cooled ternary solution)-based estimates of PSC frequency accord best with the observations in terms of the amount, spatial and temporal variation, in particular, for the latitude ranges of 55° S–70° S and 55° N–85° N. Moreover, the effects of planetary waves, synoptic-scale waves and gravity waves on PSC areal extent are separately examined using the TSTS-based PSC estimates. The latitude range of 55° S–70° S is analyzed because the TSTS-based estimates are not consistent with observations at higher latitudes (75° S) above 18 km, and PSCs in lower latitudes are more important to the ozone depletion because of the earlier arrival of solar radiation in spring. It is shown that nearly 100% of PSCs between 55° S and 70° S at altitudes of 16–24 km are formed by temperature modulation, which is influenced by planetary waves during winter. Although the effects of synoptic-scale waves on PSCs are limited, around an altitude of 12 km more than 60% of the total PSC areal extent is formed by synoptic-scale waves. The effects of gravity waves on PSC areal extent are not large in the latitude range of 55° S–70° S. However, at higher latitudes, gravity waves act to increase PSC areal extent at an altitude of 15 km by about 30% in September. Similar analyses are performed for the Northern Hemisphere. It is shown that almost all PSCs observed in the Northern Hemisphere are attributable to low temperature anomalies associated with planetary waves.
机译:使用Calipso,Cosmic和Aura MLS观察数据和重新分析数据,对2008年南冬季和2007/2008年北冬建立了大气波和极地平流层云(PSCS)关系的定量分析。 Southern Hemisphere中PSC发生频率的经度时间部分表明PSC频率不是区域均匀,并且高PSC频率区域以不同的速度从背景Zonal风中向东传播。这些特征表明大气波对PSC行为的显着影响。接下来,使用HNO3和H2O混合比计算用于PSC存在的三个温度阈值。在这三个中,基于55°S-70的纬度范围的观察,TST(超冷却三元溶液的阈值)基于PSC频率的估计值,特别是对于55°S-70的纬度范围此外,使用基于TST的PSC估计分别检查行星波,天线波,天平波和重力波对PSC区域范围的影响。分析55°S-70°S的纬度范围,因为基于TSTS的估计与在18公里的较高纬度(75°S)的观察结果中不一致,并且由于臭氧耗尽而下纬度的PSC对臭氧耗尽更重要春季太阳辐射的早期到来。结果表明,通过温度调制形成近55°S和70°S之间的PSC,在16-24km的海拔高度之间形成,该温度调制受到冬季行星波的影响。虽然Synoptic-Scale波对PSC的影响是有限的,但是在12km的高度左右超过PSC的60%的PSC区域范围由概要波形形成。在55°S-70°S的纬度范围内,重力波对PSC面积的影响不大。然而,在更高的纬度下,重力波的行为在15公里的海拔地区增加了PSC面积范围,达到约30%九月。对北半球进行类似的分析。结果表明,北半球观察到的几乎所有PSCs都是归因于与行星波相关的低温异常。

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