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The spring 2011 final stratospheric warming above Eureka: anomalous dynamics and chemistry

机译:2011年春季最终的平流层升温在尤里卡:异常动态和化学

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In spring 2011, the Arctic polar vortex was stronger than in any other year on record. As the polar vortex started to break up in April, ozone and NO2 columns were measured with UV-visible spectrometers above the Polar Environment Atmospheric Research Laboratory (PEARL) in Eureka, Canada (80.05° N, 86.42° W) using the differential optical absorption spectroscopy (DOAS) technique. These ground-based column measurements were complemented by Ozone Monitoring Instrument (OMI) and Optical Spectrograph and Infra-Red Imager System (OSIRIS) satellite measurements, Global Modeling Initiative (GMI) simulations, and meteorological quantities. On 8 April 2011, NO2 columns above PEARL from the DOAS, OMI, and GMI datasets were approximately twice as large as in previous years. On this day, temperatures and ozone volume mixing ratios above Eureka were high, suggesting enhanced chemical production of NO2 from NO. Additionally, GMI NOx (NO + NO2) and N2O fields suggest that downward transport along the vortex edge and horizontal transport from lower latitudes also contributed to the enhanced NO2. The anticyclone that transported lower-latitude NOx above PEARL became frozen-in and persisted in dynamical and GMI N2O fields until the end of the measurement period on 31 May 2011. Ozone isolated within this frozen-in anticyclone (FrIAC) in the middle stratosphere was lost due to reactions with the enhanced NOx. Below the FrIAC (from the tropopause to 700 K), NOx driven ozone loss above Eureka was larger than in previous years, according to GMI monthly average ozone loss rates. Using the passive tracer technique, with passive ozone profiles from the Lagrangian Chemistry and Transport Model, ATLAS, ozone losses since 1 December 2010 were calculated at 600 K. In the air mass that was above Eureka on 20 May 2011, ozone losses reached 4.2 parts per million by volume (ppmv) (58%) and 4.4 ppmv (61%), when calculated using GMI and OSIRIS ozone profiles, respectively. This gas-phase ozone loss led to a more rapid decrease in ozone column amounts above Eureka in April/May 2011 compared with previous years. Ground-based, OMI, and GMI ozone total columns all decreased by more than 100 DU from 15 April to 20 May. Two lows in the ozone columns were also investigated and were attributed to a vortex remnant passing above Eureka at ~500 K on 12/13 May and an ozone mini-hole on 22/23 May.
机译:2011年春季,北极极地涡旋比记录的任何一年都强劲。由于4月份的极地漩涡开始分解,臭氧和NO2柱在加拿大Eureka(80.05°N,86.42°W)的极地环境大气研究实验室(珍珠)上方的UV可见光光谱仪测量了使用差动光学吸收的紫外线环境大气研究实验室(珍珠)光谱学(DOA)技术。这些基于基于基于臭氧监测仪(OMI)和光谱仪和红外成像仪系统(OSIRIS)卫星测量,全球建模倡议(GMI)模拟和气象量的基于地面柱测量。 2011年4月8日,从DOA,OMI和GMI数据集的珍珠上面的NO2列大约是前几年的两倍。在这一天,Eureka上面的温度和臭氧体积混合比率高,表明从NO的NO2的化学生产增强。此外,GMI NOx(NO + NO2)和N2O字段表明沿着涡流边缘的向下传输和从下纬度的水平传输也有助于增强的NO2。将低纬度NOx的抗气旋冻结在动态和GMI N2O领域中被冻结,并持续到2011年5月31日的测量期结束。在中间平流层中冻结在这种冷冻的抗气旋(FRIAC)内分离的臭氧是由于与增强NOx的反应而丢失。根据GMI每月平均臭氧损失率,NOX驱动臭氧损失的NOx驱动臭氧损失大于前几年。使用被动示踪技术,利用拉格朗日化学和运输模型的被动臭氧型材,2010年12月1日起的臭氧损失是在600克拉的计算。在2011年5月20日以上Eureka的空气质量下,臭氧损失达到4.2份当使用GMI和Osiris臭氧概况分别计算时,每百万乘体积(PPMV)(58%)和4.4 ppmV(61%)。这种气相臭氧损失导致欧洲州4月/ 2011年5月以上Eureka的臭氧柱量更快地减少。基于地面的,OMI和GMI臭氧总柱全部从4月15日至20日开始超过100 du。还研究了臭氧柱中的两次低点,归因于12/13中的〜500k的涡旋残余物,500k和22/23日的臭氧迷你孔。
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