青藏高原臭氧的准两年振荡

通过对臭氧卫星观测资料及大气环流资料的分析,研究了青藏高原上空臭氧的季节和年际变化.通过分析青藏高原地区臭氧准两年振荡(QBO),并与同纬度无山区及赤道地区臭氧QBO进行比较,指出:青藏高原臭氧QBO的平均周期为29个月,平均振幅为8DU.青藏高原臭氧QBO变化位相与热带平流层纬向风场QBO相反,即热带平流层纬向西风时,青藏高原上空臭氧总量偏小,东风时臭氧总量偏大.还讨论了与青藏高原臭氧QBO相关的大气环流物质输送理论.     

青藏高原臭氧的ENSO

通过对臭氧卫星观测资料及大气环流资料的分析,研究了青藏高原上空臭氧年际变化中的ENSO信号,并与同纬度无山区及赤道地区进行比较.研究指出:在ElNino年(南方涛动指数为负),青藏高原臭氧总量偏大,在LaNina年(南方涛动指数为正),青藏高原臭氧总量偏小.同时讨论了与ENSO事件有关的大气环流物质输送.     

青藏高原臭氧的ENSO

通过对臭氧卫星观测资料及大气环流资料的分析，研究了青藏高原上空臭氧年际变化中的 ＥＮＳＯ信号，并与同纬度无山区及赤道地区进行比较。研究指出：在 Ｅ１ Ｎｉｎｏ年（ＳＯＩ指数为负）青藏高原臭氧总量增加，在 Ｌａ Ｎｉｎａ年（ＳＯＩ指数为正）青藏高原臭氧总量减小。本文同时讨论了与ＥＮＳＯ事件有关的大气环流物质输送。     

Stratospheric temperature trends: impact of ozone variability and the QBO

In most climate simulations used by the Intergovernmental Panel on Climate Change 2007 fourth assessment report, stratospheric processes are only poorly represented. For example, climatological or simple specifications of time-varying ozone concentrations are imposed and the quasi-biennial oscillation (QBO) of equatorial stratospheric zonal wind is absent. Here we investigate the impact of an improved stratospheric representation using two sets of perturbed simulations with the Hadley Centre coupled ocean atmosphere model HadGEM1 with natural and anthropogenic forcings for the 1979–2003 period. In the first set of simulations, the usual zonal mean ozone climatology with superimposed trends is replaced with a time series of observed zonal mean ozone distributions that includes interannual variability associated with the solar cycle, QBO and volcanic eruptions. In addition to this, the second set of perturbed simulations includes a scheme in which the stratospheric zonal wind in the tropics is relaxed to appropriate zonal mean values obtained from the ERA-40 re-analysis, thus forcing a QBO. Both of these changes are applied strictly to the stratosphere only. The improved ozone field results in an improved simulation of the stepwise temperature transitions observed in the lower stratosphere in the aftermath of the two major recent volcanic eruptions. The contribution of the solar cycle signal in the ozone field to this improved representation of the stepwise cooling is discussed. The improved ozone field and also the QBO result in an improved simulation of observed trends, both globally and at tropical latitudes. The Eulerian upwelling in the lower stratosphere in the equatorial region is enhanced by the improved ozone field and is affected by the QBO relaxation, yet neither induces a significant change in the upwelling trend.     

The Tibetan Ozone Low and Its Long-Term Variation During 1979–2010

A Tibetan ozone low was found in the 1990s after the Antarctic ozone hole.Whether this ozone low has been recovering from the beginning of the 2000s following the global ozone recovery is an intriguing topic.With the most recent merged TOMS/SBUV(Total Ozone Mapping Spectrometer/Solar Backscatter Ultra Violet) ozone data,the Tibetan ozone low and its long-term variation during 1979-2010 are analyzed using a statistical regression model that includes the seasonal cycle,solar cycle,quasi-biennial oscillation(QBO),ENSO signal,and trends.The results show that the Tibetan ozone low maintains and may become more severe on average during 1979-2010,compared with its mean state in the periods before 2000,possibly caused by the stronger downward trend of total ozone concentration over the Tibet.Compared with the ozone variation over the non-Tibetan region along the same latitudes,the Tibetan ozone has a larger downward trend during 1979-2010,with a maximum value of-0.40±0.10 DU yr 1 in January,which suggests the strengthening of the Tibetan ozone low in contrast to the recovery of global ozone.Regression analyses show that the QBO signal plays an important role in determining the total ozone variation over the Tibet.In addition,the long-term ozone variation over the Tibetan region is largely affected by the thermal-dynamical proxies such as the lower stratospheric temperature,with its contribution reaching around 10% of the total ozone change,which is greatly different from that over the non-Tibetan region.     

HCl Quasi-Biennial Oscillation in the Stratosphere and a Comparison with Ozone QBO

1. Introduction The quasi-biennial oscillation (QBO) of the mean zonal wind in the equatorial stratosphere was discov- ered by Reed et al. (1961) and Veryard and Ebdon (1961). Later, Funk and Garnham (1962) and Ra- manathan (1963) were the first to descri…     

热带平流层臭氧准两年周期振荡的特征及数值模拟

利用HALOE的观测资料、对热带地区平流层臭氧垂直分布的年际变化及其准两年周期振荡（QBO）进行研究，并同赤道上空平均的纬向风场的准两年周期振荡进行了模拟研究。资料分析结果表明，平流层臭氧浓度高值区的位置在南北方向上和垂直方向上的有明显的准两年周期，臭氧浓度高值中心的南北移动和上下移动又引起局地臭氧总量的周期性变化和准两年周期振荡南北半球不对称。而臭氧浓度中心位置的准两年周期变化与赤道上空平均纬向风的准两年周期振荡密切相关。资料分析还表明，赤道上空平流层中臭氧浓度QBO的位相随高度变化多次。模拟试验表明，纬向风QBO引起垂直经圈环流的变化，在平流层有三对余差环流圈。它们对O3在不同纬度和高度的输送是引起O3准两年周期振荡的重要动力原因。其中，余差环流在平流层中层（25－35km)的环流圈起着重要的作用。     

Relationship between the interannual variations of total ozone in the Northern Hemisphere and the QBO of basic flow in the tropical stratosphere

The harmonic analyses of monthly mean total ozone in the atmosphere over the Northern Hemisphere for 26 years (1960-1985) are made by using the Fourier expansion. The analysed results show that there is obviously a quasi-biennial oscillation (QBO) in the interannual variations of the amplitudes of total ozone. Generally, the amplitudes of wavenumber 1 and 2 during the westerly of the equatorial QBO are larger than those during the easter-ly. In the early winter, the amplitude of wavenumber 1 during the easterly phase is larger, and in the late winter, it is larger during the westerly phase. These are in good agreement with the observational distributions.     

中层大气行星波在臭氧的季节和年际变化中输运作用的数值研究──Ⅰ．常定流的情况

本文构造了一个３４层球坐标原始方程波－流相互耦合谱模式，利用此模式从拉格朗日平均环流的观点研究了在常定流下行星波对臭氧的输运作用。研究结果表明，行星波对臭氧的输运有明显的季节变化，在北半球冬季，由于行星波上传到平流层而大大增强了中高纬地区向极地向下的Ｏ３输运；并且还表明，热带纬向风的ＱＢＯ不仅通过影响东、西风切变而引起热带Ｏ３分布的年际变化，而且通过影响行星波的传播引起了行星波对Ｏ３输运的年际变化，这表现为当热带纬向风处于东风位相时，中高纬地区行星波对Ｏ３的输运比西风位相时强。     

Interannual variations in total ozone fields at high latitudes of the Northern Hemisphere, November to March 1998–2005

Synoptic analysis of monthly and daily mean total ozone fields is carried out using ground-based (Roshydromet) and TOMS measurements. Large interannual changes in the evolution of the stratospheric polar vortex and the North Pacific anticyclone influence the formation and dynamics of the winter-spring ozone fields in the stratosphere of high northern latitudes. The analysis shows considerable variations in the direction of zonal ozone transport from the sector of ozone inflow from low latitudes and accumulation in the Far East depending on the winter polar stratosphere temperature and the quasi-biennial oscillation (QBO) phase. In years with the easterly QBO phase and the warm polar stratosphere, ozone at the end of winter is transported to northeastern Canada and Atlantic. In years with the easterly phase and cold polar stratosphere, ozone transport is directed to northern Eurasia. These characteristics will be verified on extensive observational data.     

Ozone variations in the Northern polar region

Summary All total ozone observations ever made in the Northern polar region, including some from the 1930's, have been corrected and the basic climatology presented. The long-term ozone changes were considered in relation to the stratospheric temperatures. For each deviation from the monthly normal of the 100 hPa temperature by 1°C, there was found to be a corresponding 5–6 m atm-cm change in the monthly ozone deviation. A distinction between the ozone regimes over the Scandinavian, Canadian and East Siberian sectors of the polar region was noted. The strong appearance of the QBO (Quasi Biennial Oscillation) in the interannual ozone fluctuations was obvious. It is demonstrated that for the past three decades the total ozone experienced a few periods with positive and a few periods with negative deviations. In view of this, trends in ozone must obviously be based on greater than 10 years of data. During 1964–86, the weighted trend over the polar stations was (–0.9±0.4)% per decade. There have been, however, three periods (1958–64, 1968–76 and 1979–86), coinciding with the declining phase of the 11 year sunspot cycle, during which the ozone at all polar stations has been declining by about 0.5% per year (or less if the QBO component is filtered out). Some of the differences with Antarctic ozone are mentioned and the dominant role of the stratospheric circulation for the ozone variations is discussed. In general the Arctic ozone observations show no evidence of a major ozone decline similar to that over Antarctica.With 9 Figures     

NUMERICAL INVESTIGATION OF QBO IN OZONE

In this paper, a two-dimensional primitive equation model, coupling dynamical, radiative andphotochemical processes, is used to simulate the quasi-biennial oscillation (QBO) in ozone. TheQBO in total ozone has been successfully simulated when the forcing of equatorial stratosphericQBO in zonal wind is imposed. The simulated characters of QBO in ozone are in close agreementwith those observed. We further analyzed the mechanism of formation and maintenance of QBO inozone. In the different phases of QBO in equatorial stratospheric wind field, the global circulationhas so great difference that it makes the effects of advection transfer and eddy transfer present aquasi-biennial periodical variation. Chemical effect and dynamical effect are basically out-of-phase.They together form and maintain the QBO in ozone. Total variation rate is a tiny difference of thetwo large amounts. At the lower level of middle-high latitudes, however, it has a phase differenceof about 1-2 months between dynamical and negative chemical effects, where the dynamical effectis comparatively greater. QBO in ozone has no clear counter effects on atmospheric circulation. The experiment resultsshow that the effects of QBO in ozone on temperature field and wind field are very small.     

Vertical Ozone Profile over Tibet Using Sage I and II Data

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东亚季风降水的年际变化

通过对东亚夏季风区域30年降水量的分析研究，我们发现东亚夏季风降水年际变化中的主要成份是准二年周期变化，ENSO与东亚夏季风降水的年际变化以及准二年周期有着明显的联系。     

区域酸性沉降的数值研究：Ⅱ.个例模拟和试验

利用建立的区域酸性污染物沉降模式，配合中尺度模式ＭＭ４预报的气象场，以１９９１年６月１２￣１４日淮河流域的一次降雨过程作为实例，对我国东半部及其相邻地区的酸沉降进行了数值模拟和试验研究。结果表明，模式基本上能够模拟出区域酸性沉降的特征，具有良好的综合模拟性能和广阔的应用前景。     

北半球冬季行星波的传播及其输运作用

利用变换欧拉平均方程讨论了行星波动力学。观测和模拟结果都表明,在北半球冬季准定常行星波的经向传播存在两支波导。一支为高纬度波导,另一支则为低纬度波导。这些结果与理论分析相当一致。通过对EP通量进一步的研究表明,平流层爆发性增温是沿高纬度波导传播的异常行星波与平均气流相互作用的结果。而热带风场的准两年周期振荡（QBO）是低纬度平流层下层大气纬向平均流的一个重要年际变化,它可以影响行星波沿低纬度波导的传播;此外,由一个行星波一平均流耦合模式模拟的结果表明,这个热带风场的变化还可以通过波流相互作用调制行星波沿高纬度波导的传播。 行星波对臭氧的输运作用在文中也进行了分析。行星波强迫出的剩余平均环流表明,耗散的行星波有强的输运作用;向北的涡动热量输送可以强迫出一个正的输运环流,其在低纬度上升并在高纬度下沉。同时研究还表明,热带风场的QBO对行星波传播的调制对输运环流也有重要影响,模式结果表明,在QBO的东风位相期间行星波引起的输运作用明显增强,其结果可用于解释平流层高纬度臭氧的年际变化。     

The propagation characteristics of interannual low-frequency oscillations in the tropical air-sea system

The time series of sea surface temperature (SST), sea level pressure (SLP), zonal wind (U) and total cloudiness (CA), for the period of 1950-1979, over a 8o×8o grid-point latitudinal belt between 32oS and 32oN are made from COADS (Comprehensive Ocean-Atmosphere Data Set). The time harmonic analysis and power spectra analysis show that there exist quasi-biennial oscillation (QBO), three and half years oscillation (SO), five and half years oscillation (FYO) and eleven years oscillation (EYO) in these time series. The main propagation characteristics of these interannual low-frequency oscillations are as follows:(1) The variance analysis of SST shows that there is an active region of QBO and SO (with maximum variance), coming from the southwestern part of the subtropical Pacific, stretching eastward up to the west coast of South America, and then northward to the eastern equatorial Pacific. The QBO and SO disturbances of SST follow the same route and cause the anomaly of SST (El Nino and period of cold water) in the eastern equatorial Pacific.(2) Either the QBO or SO of SST can cause El Nino events, although it is easier when they are situated in the same phase of warm water at the eastern equatorial Pacific. The FYO of SST seems to be a standing oscillation. It plays an important role on the formation of strong El Nino events or strong cold water events.(3) The QBO and SO of U propagate eastward along the equator. The origin of QBO and SO may at least be traced as far as the western Indian Ocean. While they propagate along the equator, it strengthens two times at 90oE and the western Pacific, respectively. Like SST, the FYO of U is somehow a standing oscillation.(4) The Oscillations of U have a good coupling relationship with those of SST, while they propagate. When the QBO and SO of SST move to the east side of the eastern equatorial Pacific, it is the time for the QBO and SO of U to enter into the east part of the western Pacific.It is clear that, when we do research work on the formation of El Nino events, our consideration would not be confined to the tropics, it should cover the subtropical region in the southern Pacific. The features of the circulation and other oceanic states in this area are very important to the El Nino events.     

平流层准零风层统计特征及准两年周期振荡对其影响分析

根据形成机制的不同将平流层准零风层（Quasi-Zero Wind Layer,QZWL）划分为由平流层准两年周期振荡（Quasi-Biennial Oscillation,QBO）各高度处于不同位相形成的第一类QZWL和由于平流层低层经向温度梯度逆转而形成的第二类QZWL;利用ERA-40再分析资料分析了两类QZWL在不同季节中空间结构的变化规律,讨论了平流层QBO对两类QZWL年际变化产生的影响。研究结果表明：第一类QZWL集中出现在冬季赤道附近地区,第二类QZWL在夏季热带外地区和冬季20°N～40°N太平洋地区上空;QZWL夏季高度比冬季低约3 km,夏季QZWL出现高度比冬季稳定,约在50～70 hPa之间;由于受到QBO的直接影响,第一类QZWL出现的高度和纬度范围存在明显的年际变化,第二类QZWL受到QBO的影响主要体现在QBO西风位相年和东风位相年相比,冬季20°N～40°N范围内存在第二类QZWL的概率较高。     

Total ozone variations in the tropical belt: An application for quality of ground based measurements

Summary The study of the regime of ozone variations in the huge tropical belt (25° S to 25° N), which are, in general, very small and zonally nearly symmetric, permits to establish a statistical model for estimating the ozone deviations using Total Ozone Mapping Spectrometer (TOMS) data. The equatorial stratospheric winds at 25 and 50hPa and the solar flux at 10.7 cm are used as major predictors and the linear trend was also estimated. The 10m/sec stratospheric wind change is related to1.2% ozone change at the equator, to practically no change in the 8–15° belts and up to 1.4% change with opposite phase over the tropics in spring but nearly zero change in fall. The solar cycle related amplitude is about 1.4% per 100 units of 10.7 cm solar flux. The ozone trends are negative: not significant over the equator and about –2% per decade (significant at 95% level) over the tropics. The latter could have been enforced by the 2 to 4% lower ozone values during 1991–1993, part of which might be related to the effects of the Mt. Pinatubo eruption, but might also be due to the strong QBO. The estimated deviations are verified versus reliable observations and the very good agreement permits applying the model for quantitative quality control of the reported ozone data from previous years. The standard deviation of the difference between observed ozone deviations and those estimated from the model is only 0.9–1.6% for yearly mean, that means instruments used for total ozone observations in the tropical belt should have systematic error of less than 1%. Cases when the discrepancies between the model and reported observations at a given station exceed 2–3% for time interval of 2 or more years should be verified.With 17 Figures     

Statistical analysis and comparison of external factor effects on the total ozone field over the Russian territory in 1973–2007

The analysis of external factors, which are most significant for the formation of the monthly mean total ozone (TO) field and ozone transport over the Russian Federation, based on observation data obtained from about 30 ground-based stations of the ozonometric network averaged over a year, December through March and June through August, over five climatic regions, is considered. Performed spectrum and discriminant analysis allowed obtaining quantitative estimates of the impact of the Arctic Oscillation, deviation of the winter temperature of the lower polar stratosphere, quasi-biennial oscillations (QBO), 11-year solar cycle, El Niño-Southern Oscillation (ENSO) on the TO and to assess the regional differences in the effects of these factors. In December–March, in the years with a negative Arctic Oscillation phase, warm stratosphere, and the easterly QBO phase (QBO-E), the ozone content increases significantly relative to the opposite phases of oscillations on average by 35, 28, and 26 Dobson units (DU), respectively. The spectra, similar to the discriminant function, demonstrate strong influence of the 11-year solar cycle and QBO on the TO even in the summer months, while the QBO is more pronounced in the eastern part of the Russian Federation. The ENSO effect was not singled out against the general “noisy” background of the cold six-month period, when many atmospheric processes become active: however, during the summer months, in warm periods of the ENSO, the TO, at the 97% significance level, increases over most of the Russian area. The rest of the obtained results are significant at the 95–99.9% level.