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Influence of ENSO and MJO on the zonal structure of tropical tropopause inversion layer using high-resolution temperature profiles retrieved from COSMIC GPS Radio Occultation

机译:利用从COSMIC GPS无线电掩星获得的高分辨率温度廓线,ENSO和MJO对热带对流层顶反转层带状结构的影响

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Using COSMIC GPS Radio Occultation (RO) observations from January 2007 to December 2016, we retrieved temperature profiles with the height resolution of about 0.1?km in the upper troposphere and lower stratosphere (UTLS). We investigated the distribution of static stability ( Nsup2/sup ) and the zonal structure of the tropopause inversion layer (TIL) in the tropics, where a large change in the temperature gradient occurs associated with sharp variations in Nsup2/sup . We show the variations in the mean Nsup2/sup profiles in coordinates relative to the cold-point tropopause (CPT). A very thin ( Nsup2/sup in the range of 11.0– 12.0 × 10 - 4 s sup?2/sup . The mean and standard deviation of TIL sharpness, defined as the difference between the maximum Nsup2/sup ( maxNsup2/sup ) and minimum Nsup2/sup ( minNsup2/sup ) within ±1 km of the CPT, is ( 10.5 ± 3.7 ) × 10 - 4 s sup?2/sup . The maxNsup2/sup is typically located within 0.5?km above CPT. We focused on the variation in TIL sharpness in two longitude regions, 90–150 sup°/sup E (Maritime Continent; MC) and 170–230 sup°/sup E (Pacific Ocean; PO), with different land–sea distribution. Seasonal variations in TIL sharpness and thickness were related to the deep convective activity represented by low outgoing longwave radiation (OLR) during the Australian and Asian monsoons. The deviation from the mean sharpness (sharpness anomaly) was out of phase with the OLR anomaly in both the MC and PO. The correlation between the sharpness anomaly over the MC and PO and the sea surface temperature (SST) Ni?o?3.4 index was ?0.66 and +0.88 , respectively. During La Ni?a (SST Ni?o?3.4 + 0.5 K) in the PO, warmer SSTs in the MC and PO produce more active deep convection that tends to force the air upward to the tropopause layer and increase the temperature gradient there. The intraseasonal variation in sharpness anomaly during slow and fast episodes of the Madden–Julian Oscillation (MJO) demonstrates that eastward propagation of the positive sharpness anomaly is associated with organized deep convection. Deep convection during MJO will tend to decrease Nsup2/sup below CPT and increase Nsup2/sup above CPT, thus enlarging the TIL sharpness. Convective activity in the tropics is a major control on variations in tropopause sharpness at intraseasonal to interannual timescales.
机译:利用2007年1月至2016年12月的COSMIC GPS无线电掩星(RO)观测,我们获得了对流层和低平流层(UTLS)高度分辨率约为0.1?km的温度剖面。我们研究了热带地区静态稳定性(N 2 )的分布和对流层顶反转层(TIL)的带状结构,其中温度梯度发生较大变化,而N < sup> 2 。我们展示了相对于冷点对流层顶(CPT)坐标的平均N 2 剖面的变化。非常薄的(N 2 在11.0-12.0×10-4 s ?2 范围内。TIL清晰度的平均值和标准偏差定义为最大C 2 (maxN 2 )和最小N 2 (minN 2 )在CPT的±1 km之内,是(10.5±3.7)×10-4 s ?2 。maxN 2 通常位于CPT上方0.5?km之内,我们着眼于TIL清晰度的变化在两个经度区域,海陆90°E <150°° E和东太平洋170°<230°E ° E(太平洋; PO),海陆分布不同。 TIL锐度和厚度的季节性变化与澳大利亚和亚洲季风期间以低外向长波辐射(OLR)表示的深对流活动有关,二者均偏离了平均锐度(锐度异常)与OLR异常。 MC和PO。MC和PO上的锐度异常与海面温度之间的相关性(SST)Ni 3 O 3 3.4指数分别为0.66和+0.88。在PO上的La Ni?a(SST Ni?o?3.4 + 0.5 K)期间,MC和PO中较暖的SSTs会产生更活跃的深对流,这会迫使空气向上流到对流层顶层并增加那里的温度梯度。在Madden–Julian涛动(MJO)的慢速和快速发作期间,季节内清晰度异常的季节内变化表明,正清晰度异常向东传播与有组织的深度对流有关。 MJO期间的深对流将趋向于降低CPT以下的N 2 并增加高于CPT的N 2 ,从而增大TIL清晰度。热带地区的对流活动是对季节内到年际尺度对流层顶锐度变化的主要控制。

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