...
首页> 外文期刊>Advances in Atmospheric Sciences >Middle stratospheric polar vortex ozone budget during the warming Arctic winter, 2002–2003
【24h】

Middle stratospheric polar vortex ozone budget during the warming Arctic winter, 2002–2003

机译:2002-2003年北极冬季升温期间平流层中部极地涡旋臭氧的收支

获取原文
获取原文并翻译 | 示例
           

摘要

The ozone budget inside the middle stratospheric polar vortex (24–36 km) during the 2002–2003 Arctic winter is studied by analyzing Michelson Interferometer for Passive Atmospheric Sounding (MIPAS) satellite data. A comprehensive global chemical transport model (Model for Ozone and Related Chemical Tracers, MOZART-3) is used to analyze the observed variation in polar vortex ozone during the stratospheric sudden warming (SSW) events. Both MIPAS measurement and MOZART-3 calculation show that a pronounced increase (26–28 DU) in the polar vortex ozone due to the SSW events. Due to the weakening of the polar vortex, the exchange of ozone mass across the edge of the polar vortex increases substantially and amounts to about 3.0×107 kg according to MOZART-3 calculation. The enhanced downward transport offsets about 80% of polar vortex ozone mass increase by horizontal transport. A “passive ozone” experiment shows that only ∼55% of the vertical ozone mass flux in February and March can be attributed to the variation in vertical transport. It is also shown that the enhanced downward ozone above ∼32 km should be attributed to the springtime photochemical ozone production. Due to the increase of air temperature, the NO x reaction rate increases by 40%–80% during the SSW events. As a result, NO x catalytic cycle causes another 44% decrease in polar vortex ozone compared to the net ozone changes due to dynamical transport. It is also shown that the largest change in polar vortex ozone is due to horizontal advection by planetary waves in January 2003.
机译:通过分析用于被动大气探测(MIPAS)卫星数据的迈克尔逊干涉仪,研究了2002-2003年北极冬季平流层中极涡旋(24-36 km)内部的臭氧收支。全面的全球化学传输模型(臭氧和相关化学示踪剂模型,MOZART-3)用于分析平流层突然变暖(SSW)事件期间观测到的极地涡旋臭氧变化。 MIPAS测量和MOZART-3计算均显示,由于SSW事件,极地涡旋臭氧显着增加(26–28 DU)。由于极性涡旋的减弱,根据MOZART-3计算,整个极性涡旋边缘的臭氧质量交换量大大增加,达到约3.0×107 。向下运输的增强抵消了水平运输中约80%的极地涡旋臭氧质量增加。 “被动臭氧”实验表明,二月和三月的垂直臭氧质量通量中只有约55%归因于垂直迁移的变化。还表明,〜32 km以上向下臭氧的增加应归因于春季光化学臭氧的产生。由于空气温度的升高,在SSW事件期间,NO x 反应速率提高了40%–80%。结果,与动态运输引起的净臭氧变化相比,NO x 催化循环使极性涡旋臭氧又减少了44%。还表明,极地涡旋臭氧的最大变化是由于2003年1月行星波引起的水平对流。

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号