Long-term analysis of the Antarctic total ozone zonal asymmetry by MERRA-2 and CMIP6 data

O. Ivaniha
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Abstract

. Objectives. To analyze ozone monthly mean data from the MERRA-2 reanalysis and CMIP6 model. To determine Antarctic ozone asymmetry climatology for austral spring months (September, October, November) over the 1980–2014 period. Methods. Processing and visualization of the MERRA-2, CMIP6 data on total ozone and ozone partial pressure, following analysis, interpretation, and comparison. Getting 2D (total ozone column) and 3D (ozone partial pressure) monthly mean ozone values for the zonal band (0 ° –90 ° S) at pressure levels (1000–0.1 hPa) for each month of the chosen period. Calculating climatology of the total ozone and ozone partial pressure. Comparison of model and reanalysis of results. Results. The amplitude of ozone zonal asymmetry was calculated to provide the monthly, latitudinal, longitudinal and altitudinal analysis. It is shown that the largest ozone zonal asymmetry is observed in spring, especially in October, with dominant wave-1 structure with zonal minimum over 0 ° –90 ° W, and maximum over 120 ° –180 ° E longitudinal sectors. The area with high ozone content is located at the 40 ° –80 ° S zonal band and gradually shifts to the south from September to November. The model underestimates amplitude of ozone zonal asymmetry, especially in October. Conclusions. Latitudinal mean maximums in zonal mean ozone distribution are observed over 62 ° S, in October over 66 ° S, and in November over 68 ° S for MERRA-2 and over 64 ° S, 65 ° S and 66 ° S respectively for CMIP6. The poleward shift of ozone latitude maximum continues until March with decreasing of ozone level, but in April, the shift reverses its direction to equatorward and ozone level starts to increase, however in the model this process is slower. In September the shift again becomes poleward. In the longitudinal distribution wave-1 pattern dominates with a shift of longitude ozone minimum. From September to October the shift is eastward, and from October to November westward by MERRA-2 data and only eastward by CMIP6 data. The highest difference in altitude ozone distribution is observed during October in the stratosphere between ozone zonal minimum and maximum points and reaches approximately 68% (44%) of the zonal average value at 65 ° S (65.4 ° S) by MERRA-2 (CMIP6) data. MERRA-2 profiles unlike CMIP6 one show higher location of altitudinal maximum over the zonal minimum and lower over the zonal maximum with the zonal mean in the middle. All three CMIP6 profiles have the same height of altitude maximum.
MERRA-2和CMIP6资料对南极总臭氧纬向不对称性的长期分析
. 目标。分析MERRA-2再分析和CMIP6模式的臭氧月平均数据。确定1980-2014年期间南方春季月份(9月、10月和11月)的南极臭氧不对称气候学。方法。MERRA-2、CMIP6总臭氧和臭氧分压数据的处理和可视化,分析、解释和比较。得到所选时间段内各月压力水平(1000-0.1 hPa)下纬向带(0°-90°S)月平均臭氧值2D(总臭氧柱)和3D(臭氧分压)。计算臭氧总量和臭氧分压的气候学。模型比较及结果再分析。结果。计算臭氧纬向不对称的振幅,提供月、纬、纵、高的分析。结果表明,臭氧纬向不对称性最大的季节是春季,特别是10月,以波-1结构为主,纬向最小值在0°~ 90°W,最大值在120°~ 180°E。臭氧含量高的区域位于40°-80°S纬向带,从9月到11月逐渐向南移动。该模式低估了臭氧纬向不对称的振幅,特别是在10月份。结论。纬向平均臭氧分布的纬向平均最大值在62°S以上,10月在66°S以上,11月在68°S以上,CMIP6分别在64°S、65°S和66°S以上。臭氧纬度最大值极移一直持续到3月,臭氧水平下降,但在4月,极移方向逆转到赤道方向,臭氧水平开始上升,但在模式中这一过程较慢。9月,北极再次转向北极。在纵向分布上,波1型占主导地位,臭氧最小值在经度上有偏移。从9月到10月,MERRA-2数据显示为东移,从10月到11月向西移动,CMIP6数据显示仅向东移动。根据MERRA-2 (CMIP6)资料,10月平流层臭氧纬向最大值和最小值的差异最大,约占65°S(65.4°S)纬向平均值的68%(44%)。与cmip1不同,MERRA-2剖面的纬向最大值高于纬向最小值,纬向最大值低于纬向最大值,纬向平均值位于中间。所有三个CMIP6剖面具有相同的高度最大值。
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