北半球中高纬度对流层顶转换层中O3/H2O 混合关系的结构形态

利用北半球40°N～50°N纬度带上HALOE实验测量的O₃和H₂O廓线资料,根据示踪成分O₃和H₂O空间分布的化学寿命以及输运特征时间常数等性质,在等熵坐标中构建了对流层顶附近及最低平流层300～390 K等熵面间,O₃/H₂O混合关系的结构形态和季节特征.结果表明: (1) 在对流层顶转换层的320～380 K等熵面间O₃混合比廓线的斜率具有空间转折"突变",而H₂O混合比廓线的斜率则出现空间渐变转折.在对流层顶附近O₃和H₂O的源分别是平流层与对流层,使O₃混合比和H₂O混合比在320～380 K等熵面的两侧显现出截然不同的垂直分布梯度.(2) 在对流层顶附近O₃/H₂O达到最小二乘意义上的最佳拟合时,两者参考关系的对流层支与平流层支呈现出非规则"L"结构形态的季节与季节内变化,其中对流层支的斜率为负,而平流层支的斜率可随季节出现正负变化.同时,由"L"形态的转角处可确定随季节变化的化学对流层顶(chemopause)特征.(3) 由O₃/H₂O混合关系反映出对流层不同区域空气携带的物质成分分别与平流层空气混合而形成混合层,而且可使混合层的混合线不恒定.混合层的表现在2003年、2005年1月和2003年4月的混合程度相当,混合的等熵厚度大约是30 K,即在320～350 K等熵面间.2005年11月的混合高度有所增高,进入平流层的H₂O混合比要比2003年和2005年1月的小,混合的等熵厚度大约为30 K,在330～360 K等熵面间.不同季节混合的等熵厚度变化较小,但高度可随季节而变化.O₃/H₂O混合关系的平流层支随季节的变化很明显,1月最低平流层空气脱水是引起平流层支季节变化的重要原因.     

N2O增加对大气环境影响的模拟及其与甲烷和平流层水汽影响的比较

本文利用美国国家大气环境中心(NCAR)的二维化学、辐射和动力相互作用的模式(SOCRATES),模拟了大气中N₂O增加对O₃和温度的影响,并从化学、辐射和动力过程讨论了影响原因,此外还与大气甲烷和平流层水汽增加对大气环境的影响进行了对比.分析表明:大气中N₂O浓度增加以后,将通过化学过程引起30 km以上O₃损耗,30~40 km损耗较多;30 km以上降温明显,下平流层中低纬度地区以及对流层O₃增加并有微弱升温;30~40 km附近,北半球中高纬地区O₃减少以及降温幅度都大于南半球.对流层升温主要是N₂O和O₃增加所致,而平流层温度变化主要受O₃控制.北半球中高纬地区动力过程对温度变化的反馈较其它地区明显,这种反馈对平流层中高层北半球中高纬地区温度和O₃的变化都有明显影响.大气中甲烷增加引起的O₃损耗在45 km以上,45 km以下O₃增加.平流层水汽增加会引起40 km以上O₃减少,20~40 km大部分地区O₃增加.N₂O增加造成的O₃损耗正好位于臭氧层附近,其排放对未来O₃层恢复至关重要.N₂O增加引起下平流层15~25 km中低纬度地区有弱的升温,这与其它温室气体增加对该地区温度的影响不同,CO₂,CH₄和H₂O等增加后下平流层通常是降温.     

关于O3层垂直剖面遥感的逆转曲线的数学拟合模式

逆转遥感是当前获得大气O₃层垂直剖面资料的重要方法之一，而逆转曲线的质量对遥感结果的精度至关重要．本文在最小二乘法的基础上，结合逆转曲线的特征，加以适当处理，建立了逆转曲线的拟合数学模式．其性能良好，对研究O₃层垂直剖面的长期演变趋势具有重要意义．     

气象条件对京津冀地区O3和PM2.5双高污染的影响及对减排的启示作用

近年来,京津冀地区频繁发生O₃和PM_2.5同时超标的双高污染(CP)过程,给大气污染协同控制带来了严峻挑战.京津冀地区50%以上的CP事件发生在4～5月,并且在2018年达到了最高的11天. CP事件期间的O₃和PM_2.5浓度略低于但接近仅发生O₃和PM_2.5污染时的浓度,这表明双高污染会造成更为严重的危害.由斯堪的纳维亚遥相关型的两个中心与华北上空的异常反气旋环流中心组成的Rossby波波列导致京津冀地区出现高温、潮湿和静稳的气象条件,这同时增加了O₃和PM_2.5的浓度,有利于CP事件的发生.在2018年之后CP日数急剧减少,而气象条件并没有明显的趋势变化.因此,气象条件的变化并没有真正促成2019年和2020年CP日数的下降.这其中隐含着是PM_2.5相关排放的减少导致了CP日数的减少(2019年和2020年共减少约11天).本文所揭示的不同污染事件之间大气条件的差异有助于在日-周的时间尺...     

探测与2014年新疆于田MS7.3地震相关的大气CO和O3异常变化

基于AQUA AIRS传感器提取了2014年2月12日新疆于田M_S7.3地震前后CO和O₃数据, 讨论了数据变化与地震活动的关系。 差值法和异常指数法结果表明, 于田地震后CO和O₃在3月份达到最大异常, 且气体柱浓度异常沿NE向发震构造呈线性分布; 不同高度的CO和O₃的VMR值变化与差值法和异常指数法得到的结果相吻合; 地震前后短时间内CO和O₃气体柱浓度出现下降, 且地震当月最低。 初步推断可能是阿尔金断裂尾部在SW向运动过程中使得震区断裂带在弹性挤压状态下出现闭锁, 气体不流通导致; CO和O₃异常更多的可能是由于田地震引起地下气体大量释放, 其次可能是与地下气体逸散在大气圈中发生的一系列化学反应有关。 研究表明, 卫星高光谱遥感数据获得的CO和O₃的地球化学信息与地震有密切联系, 在地震监测及预测领域具有重要的应用价值。     

火星O2(a1Δg)气辉高光谱分辨辐射传输特性研究

1.27μm波段的氧分子近红外气辉是火星大气最重要的气辉辐射之一,该气辉高光谱分辨辐射传输模型的建立对于研制火星探测载荷,反演火星大气的风场温度场与臭氧浓度,以及研究火星空间物理,有重要的科学价值与工程意义.在研究火星大气O₂(a¹Δ_g)气辉光化学反应模型的基础上,提出了O₂(a¹Δ_g)气辉体辐射率的计算方法,并建立了火星大气气辉辐射传输理论;通过与用于研究火星大气特征的光谱学探测仪(Spectroscopy Spectrograph for the Investigation of Characteristics of the Atmosphere of Mars, SPICAM)的实测数据进行对比,验证了所建立的火星O₂(a¹Δ_g)气辉高光谱分辨辐射传输模型的准确性;针对火星与地球大气的O₂(a¹Δ_g)气辉,在体辐射率、自...     

全球Schwideski海潮模型K1、O1分波在中国大陆产生的地倾斜负荷潮

本文根据计算地倾斜负荷潮的积分Green函数方法,计算了全球Schwiderski海潮模型K₁、O₁分波在中国大陆产生的地倾斜负荷潮,绘制了K₁、O₁分波负荷潮椭圆及其长轴迹线,沿长轴方向分量的等潮时线,长、短半轴等值线诸地倾斜负荷潮参量在中国大陆境内的分布图,给出了它们的空间分布图象,为国内的地倾斜固体潮研究提供了重要的参考资料.     

地倾斜固体潮O1和K1日波分潮的海潮效应

本文采用沈育疆等编绘的海潮图,用Farrell给出的地倾斜负荷格林函数褶积积分法,计算了海潮O₁和K₁分潮对我国北京等12个测站地倾斜固体潮的海潮效应。对泰安等测站地倾斜固体潮的观测值进行了海潮改正。     

北半球不同纬度臭氧层系统混沌吸引子的特征研究

将TOMS测量的北半球不同纬度各纬向平均逐日O。总量作为无规序列,利用时滞方法重构序列的相空间吸引子,计算其系统状态演化过程中形成的整体结构特征.结果表明,各纬度O₃层系统吸引子都具有非整数分维结构；此外,在完整的Lpapunov指数谱中,所有指数分量之和均为负值,且最大指数分量总是正值.反映出O₃层系统相空间总体上是收缩的,同时提供了存在奇怪吸引子的证据,表征O₃层系统的演化是一种耗散混饨运动.这对于进一步应用非线性动力系统理论和方法,深入研究O₃层系统的动力学特征具有重要意义.     

武汉和阿德莱德大气太阴N2潮及M2潮的对比分析

利用阿德莱德（35°S,138°E）和武汉（30.6°N,114.5°E）的流星雷达观测数据首次给出了80~100 km高度上周期为12.66太阳时的大气太阴半日潮汐（N₂潮）的季节、高度、年度变化及其与周期为12.42太阳时的大气太阴半日潮汐（M₂潮）的对比分析.分析结果表明：武汉和阿德莱德的N₂潮和M₂潮均有明显的季节、高度和年度变化.N₂潮与M₂潮的幅度比值大于其引力势之比0.191,在某些年份的不同季节和高度上,N₂潮的幅度甚至大于M₂潮的幅度.大多幅度之比接近或超过N₂潮和M₂潮引力势之比的2倍.中低热层的大气太阴N₂潮汐值得关注.     

Influence of wave activity on the composition of the polar stratosphere

The planetary wave impact on the polar vortex stability, polar stratosphere temperature, and content of ozone and other gases was simulated with the global chemical–climatic model of the lower and middle atmosphere. It was found that the planetary waves propagating from the troposphere into the stratosphere differently affect the gas content of the Arctic and Antarctic stratosphere. In the Arctic region, the degree of wave activity critically affects the polar vortex formation, the appearance of polar stratospheric clouds, the halogen activation on their surface, and ozone anomaly formation. Ozone anomalies in the Arctic region as a rule are not formed at high wave activity and can be registered at low activity. In the Antarctic Regions, wave activity affects the stability of polar vortex and the depth of ozone holes, which are formed at almost any wave activity, and the minimal ozone values depend on the strong or weak wave activity that is registered in specific years.     

The temporal and spatial characteristics of the surface air temperature variations over the Antarctic and its surrounding area

The characteristics of the spatial distribution, temporal variations trend and oscillation for the surface air temperature variations during 1957—1993 in the Antarctic and its surrounding area were analyzed. The results show that the short-time climate change in the Antarctic is complex both temporally and spatially. The Antarctic is by no means the strongest responding region to the global greenhouse effect. There is a distinguished difference in the trends of the temperature changes for the Antarctic and global mean, which could not be explained simply by the global greenhouse effect. Project supported by the National Antarctic Key Project of China (85-905).     

AIRS卫星温度和臭氧廓线在南极的验证分析

利用2008年中山站、Amundesen-Scott(SouthPole)站和Neumayer站为期一年的温度和臭氧探空数据,对AIRS第六版温度和臭氧垂直廓线产品在南极的精度进行了验证.结果表明,AIRS温度与探空温度总体上具有显著的一致性,其中对流层偏差最小(RMSe2℃),近地面温度由于受到下垫面影响偏差略大(RMSe～2℃),平流层偏差较大(2℃RMSe3℃),AIRS温度平均低于探空观测且受季节变化影响显著,秋冬季偏差整体上高于春夏季.AIRS臭氧反演精度在平流层(RMSe～25%)要优于对流层(RMSe～30%),RMSe最大值出现在UT-LS区域(可达40%)且在"臭氧洞"期间明显增大.AIRS产品精度在南极沿岸和内陆存在差异,由于南极地区探空资料较少且主要位于沿海,故在南极内陆地区进行探空观测对于提高卫星资料精度,改善该区域天气预报能力具有重大意义.     

Systems modelling of stratospheric ozone transport and photochemistry

A scheme of a system of physical and chemical processes controlling the production, transport and destruction of ozone and its gaseous catalysts, as well as other related gases in the low and high stratosphere is presented. An account is made of temperature variations of the stratospheric layer resulting from changes in ozone content; also included is the effect of temperature variations on photochemical reaction rates and ozone and other gases transport between atmospheric layers. Parameters describing major relations of the system are inferred from the analysis of ozone and trace gas data and from the results of model calculations of interdependence between variations in temperature and ozone content of the layer.An analysis of minor fluctuations of the linearized system shows that photochemical processes are responsible for its aperiodic stability and that gas transport between atmospheric layers destabilizes the system.     

我国上空平流层中微量气体的垂直分布和变化趋势

利用1992～2005年卤素掩星试验（HALOE）的观测资料分析了中国上空平流层的几种微量气体（NO, NO2, HF, HCl, CH4, H2O 和O3）混合比的垂直分布和变化趋势,以期为研究平流层的辐射和化学过程提供一些有用的数据. 文中除给出我国上空平流层各高度上平均的各种微量气体的含量外,还给出青藏高原上空这些微量气体的含量. 分析结果表明,平流层各种微量气体混合比的垂直分布有其不同的特征,在对流层上层到平流层底部各种微量气体的混合比分布和季节变化与平流层相比有明显的差异;分析结果还表明,这些微量气体的季节变化、准两年周期振荡和长期变化趋势都很明显,并且在平流层的不同高度上它们的变化趋势是不相同的. 在平流层中层,NO, NO2, HCl 和H2O 混合比在1998年以前都是增加而后则是明显下降的,但O3相反,在1998年以前明显减少,1998年后其减少的趋势不明显. 这表明,近年来平流层中层这些微量气体的减少使得它们对臭氧的破坏有所缓解. 但在平流层下层,臭氧的耗损仍然很明显.     

Impact-induced perturbations of atmospheric sulfur

Asteroids and comets that are vaporized during hypervelocity impact events can inject large masses of S into the stratosphere where it can potentially affect the radiation budget of the Earth, alter the chemistry of the ozone layer, and eventually be converted to sulfuric acid rain. Relatively small carbonaceous asteroids, 0.3 km in diameter, contain 5 times more S than the entire modern stratosphere and these objects hit the Earth at an average rate of 1 per 10,000 years. Larger impact events, capable of injecting 10¹⁵ g of S into the stratosphere, occur at an average rate of 1 per 1 million years. Calculations indicate there is sufficient O and H in the vapor plumes of most impact events to convert the S to sulfuric acid aerosols. If this conversion occurs, then the larger impact events could depress mean surface temperatures by more than 2°C for 3 years or longer.     

The effects of water vapour and oxides of nitrogen on ozone and temperature structure of the stratosphere

Summary A steady-state mean meridional model of the stratosphere is used to investigate the effects of water vapour and nitrogen oxides on ozone and temperature distributions in the stratosphere. The Chapman classical photochemical scheme for ozone is extended to include the dominant reactions involving hydrogen compounds and nitrogen oxides. The ozone and temperature changes are studied under radiative-photochemical equilibrium conditions and in a model incorporating both transport and radiative-photochemical processes. It is found that both hydrogen and nitrogen reactions contribute to substantial decreases in ozone and temperature under photochemical equilibrium conditions, but the computed distribution do not resemble those observed. The effect of transport processes is to reduce the deviations in the ozone mixing ratio and temperature with the computed distributions having many features in common with the observations. It is found that the ozone and temperature respond more readily to the arbitrary increase of nitrogen oxides than to that of water vapour.     

Extension of Antarctic ozone hole to lower latitudes in the South-American region

A comparison of monthly mean values of total ozone at South Pole, Buenos Aires (Argentina), Cachoeira Paulista and Natal (Brazil), and Huancayo (Peru) revealed that whereas South Pole showed an ozone depletion of 45% in October 1987 (as compared to October, 1977), Buenos Aires showed a small decrease (10%) while the other locations showed very small decreases (1–2%). When daily values are considered, the Antarctic ozone hole of October 1987 seems to have caused 10% depletion at Buenos Aires and 5% at Natal and Huancayo in December 1987. However, a large part of this is normal seasonal variation, except at Huancayo, where a residual effect of 5% depletion in December 1987 remains. The QBO effects (5–8% changes in the ozone level in 2–3 years) could cause 10–15% fluctuations in solar UVB on the ground on clear-sky days and could be a possible health hazard unless factors like cloudiness reduce the UVB intensities.     

Temperature and ozone variations in the stratosphere

Examined are temperature and ozone variations in the Northern Hemisphere stratosphere during the period 1958–77, as estimated from radiosondes rocketsondes, ozonesondes, and Umkehr measurements. The temperature variation in the low tropical stratosphere is a combination of the variation associated with the quasi-biennial oscillation, and a variation nearly out of phase with the pronounced 3-yearly temperature oscillation (Southern Oscillation) present in the tropical troposphere since 1963. Based on radiosonde and rocketsonde data, the quasibiennial temperature oscillation can be traced as high as the stratopause, the phase varying with both height and latitude. However, the rocketsonde-derived temperature decrease of several degrees Celsius in the 25–55 km layer of the Western Hemisphere between 1969 (sunspot maximum) and 1976 (sunspot minimum) is not apparent in high-level radiosonde data, so that caution is advised with respect to a possible solar-terrestrial relation.There has been a strong quasi-biennial oscillation in ozone in the 8–16 km layer of the north polar region, with ozone minimum near the time of quasi-biennial west wind maximum at a height of 20 km in the tropics. A quasi-biennial oscillation in ozone (of similar phase) is also apparent from both ozonesonde data and Umkehr measurements in 8–16 and 16–24 km layers of north temperate latitudes, but not higher up. Both measurement techniques also suggest a slight overall ozone decrease in the same layers between 1969 and 1976, but no overall ozone change in the 24–32 km layer. Umkehr measurements indicate a significant 6–8% increase in ozone amount in all stratospheric layers between 1964 and 1970, and in 1977 the ozone amount in the 32–46 km layer was still 4% above average despite the predicted depletion due to fluorocarbon emissions. The decrease in ozone in the 32–46 km, layer of mid latitudes following the volcanic eruptions of Agung and Fuego is believed to be mostly fictitious and due to the bias introduced into the Umkehr technique by stratospheric aerosols of volcanic origin. Above-average water vapor amounts in the low stratosphere at Washington, DC, appear closely related to warm tropospheric temperatures in the tropics, presumably reflecting variations in strength of the Hadley circulation.     

The signal of the 11-year solar cycle in the global stratosphere

The search for a signal of the 11-year sunspot cycle in the heights and temperatures of the lower stratosphere was previously successfully conducted for the northern hemisphere with a data set from the Freie Universität Berlin, covering four solar cycles. This work has been extended to the whole globe by means of the NCEP/NCAR reanalyses for the period 1968–1996. The re-analyses show that the signal exists in the southern hemisphere too, and that it is of nearly the same size and shape as on the northern hemisphere. The NCEP/NCAR reanalyses yield higher correlations with the solar cycle than do the Berlin analyses for the same period, because the interannual variability is lower in the NCEP/NCAR data.The correlations between the solar cycle and the zonally averaged temperatures at the standard levels between 200 and 10 hPa are largest between the tropopause and the 25 km level, that is, in the ozone layer. This may be partly a direct effect in this layer, because of more absorber (ozone) and more ultraviolet radiation from the sun in the peaks of the 11-year solar cycle. However, it is more likely to be mainly an indirect dynamical consequence of UV absorption by ozone in the middle and upper stratosphere.The largest temperature correlations move with the sun from one summer hemisphere to the other, and the largest height correlations move poleward from winter to summer.