首页> 外文期刊>Journal of Geophysical Research. Biogeosciences >Midstratospheric ozone variability over Bern related to planetary wave activity during the winters 1994-1995 to 1998-1999
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Midstratospheric ozone variability over Bern related to planetary wave activity during the winters 1994-1995 to 1998-1999

机译:1994-1995年至1998-1999年冬季,伯尔尼上层平流层臭氧变化与行星波活动有关

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Since November 1994, continuous observations of the stratospheric and mesospheric ozone volume mixing ratio (VMR) profiles over Bern (46.95 degreesN, 7.45 degreesE), Switzerland, are performed using the Ground based Millimeter-Wave Ozone Spectrometer (GROMOS), an instrument of the Network for the Detection of Stratospheric Change. We report on large episodic perturbations of the midstratospheric (25-40 km) ozone VMR values observed during the winters 1994-1995 through 1998-1999. Backward trajectory calculations show that the observed episodes are coincident with periods of enhanced meridional transport. Representations of the isentropic potential vorticity field indicate that this transport goes along with significant deformations and southward excursions of the polar vortex in association with strong planetary wave activity. Along the eastern edge of the distorted vortex, northward advection of subtropical air leads to anomalously high ozone VMR values in the midlatitudes middle stratosphere, whereas the passage of polar vortex air over Bern leads to midstratospheric ozone minima. Besides a comprehensive analysis of all extreme episodes detected between November 1994 and June 1999, details are presented for one specific episode. For another episode the influence of photochemical processes is investigated, and it is found that photochemistry acts to damp (rather than to enhance) the effects of planetary-wave-driven meridional transport. It is concluded that the extreme ozone episodes observed over Bern during winter, are primarily a dynamical feature, their amplitude being determined by the meridional ozone VMR gradient rather than by photochemical processes. [References: 41]
机译:自1994年11月以来,瑞士陆上毫米波臭氧光谱仪(GROMOS)连续观测了瑞士伯尔尼(46.95°N,7.45°E)的平流层和中层臭氧体积混合比(VMR)剖面。平流层变化检测网络。我们报告了在1994-1995年冬季至1998-1999年冬季观测到的平流层中层(25-40 km)臭氧VMR值的大的周期性扰动。向后的轨迹计算表明,观测到的事件与子午线运输增强的时期相吻合。等熵势涡场的表示表明,这种传输伴随着强烈的行星波活动伴随着极涡的明显变形和向南偏移。沿着扭曲涡流的东边缘,亚热带空气的北向平流导致中纬度平流层中空的臭氧VMR值异常高,而极地涡旋空气在伯尔尼上方的通过导致平流层中臭氧的最小值。除了对1994年11月至1999年6月期间检测到的所有极端事件进行全面分析之外,还提供了一个特定事件的详细信息。对于另一事件,研究了光化学过程的影响,发现光化学的作用是抑制(而不是增强)行星波驱动的子午线传输的影响。结论是,冬季在伯尔尼观测到的极端臭氧事件主要是动力学特征,其幅度取决于子午臭氧VMR梯度而不是光化学过程。 [参考:41]

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