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21.
利用Herold等建立的地表反射率库及MODIS遥感影像研究城市区和非城市区典型地物在可见光红蓝波段地表反射率的比值特性。在此基础上,利用MODIS 1km分辨率遥感影像红蓝可见光波段实现了气溶胶光学厚度的反演,采用卫星过境时间前后半小时北京和香河AERONET站的气溶胶光学厚度观测平均值作为验证参考。结果显示,66.67%的反演结果处于±0.05±0.15τ的误差界限内,反演算法不受地表反射率的限制,而且只利用了可见光红蓝波段,避免缺少近红外波段数据的限制。 相似文献
22.
东亚地区春季二氧化硫的输送与转化过程研究I.模式及其验证 总被引:5,自引:0,他引:5
结合新近评估的东亚地区污染源资料,作者利用一个耦合的区域化学输送模式系统以探讨东亚地区春季期间气象过程、气相与液相化学过程、非均相化学过程、气溶胶过程和干湿沉降过程对二氧化硫输送及转化过程的影响,并研究二氧化硫和硫酸盐气溶胶的空间分布及变化特征.模拟的二氧化硫和硫酸盐气溶胶的浓度值与2001年春季飞机和地面获取的观测值进行了比较.比较结果显示,模拟值与观测值具有很好的一致性,模式系统很好地反映了二氧化硫和硫酸盐气溶胶的分布特征和变化规律,再现了许多观测到的重要特征,为进一步分析模拟结果奠定了基础. 相似文献
23.
The Grid-point Atmospheric Model of IAP LASG version 2 (GAMIL2) has
been developed through upgrading the deep convection parameterization, cumulus
cloud fraction and two-moment cloud microphysical scheme, as well as changing
some of the large uncertain parameters. In this paper, its performance is
evaluated, and the results suggest that there are some significant improvements
in GAMIL2 compared to the previous version GAMIL1, for example, the components
of the energy budget at the top of atmosphere (TOA) and surface; the geographic
distribution of shortwave cloud radiative forcing (SWCF); the ratio of
stratiform versus total rainfall; the response of atmospheric circulation to
the tropical ocean; and the eastward propagation and spatiotemporal structures
of the Madden Julian Oscillation (MJO). Furthermore, the indirect aerosols
effect (IAE) is -0.94 W m-2, within the range of 0 to -2 W m-2
given by the IPCC 4th Assessment Report (2007). The influence of uncertain
parameters on the MJO and radiation fluxes is also discussed. 相似文献
24.
The aerosol number spectrum and gas pollutants were measured and the new particle formation (NPF) events were discussed in Nanjing. The results showed that the size distributions of aerosol number concen- trations exhibited distinct seasonal variations, implying the relations of particle sizes and their sources and sinks. The number concentrations of particles in the nuclei mode (10-30 nm), Aitken mode (30-100 nm), accumulation mode (100 -1000 nm) and coarse mode (〉1μm) varied in the order of summer 〉 spring 〉 autumn, summer 〉 autumn 〉 spring, autumn 〉 summer 〉 spring, and spring 〉 autumn 〉summer, re- spectively. The diurnal variation of total aerosol number concentrations showed three peaks in all observed periods, which corresponded to two rush hours and the photochemistry period at noon. In general, the NPF in summer occurred under the conditions of east winds and dominant air masses originating from marine areas with high relative humidity (50%-70%) and strong solar radiations (400 -700 W m-2). In spring, the NPF were generally accompanied by low relative humidity (14%-30%) and strong solar radiations (400-600 W m-2). The new particle growth rates (GR) were higher in the summertime in the range of 10- 16 nm h-1. In spring, the GR were 6.8-8.3 nm h-1. Under polluted air conditions, NPF events were seldom captured in autumn in Nanjing. During NPF periods, positive correlations between 10- 30 nm particles and 03 were detected, particularly in spring, indicating that NPF can be attributed to photochemical reactions. 相似文献
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27.
GUAN Fulai ZHENG Youfei CAI Ziying YU Changwen ZHANG Nan 《Acta Meteorologica Sinica》2011,25(4):494-505
Solar radiation is an important energy source for plants on the earth and also a major component of the global energy balance.Variations in solar radiation incident at the earth's surface profoundly affect the human and terrestrial environment,including the climate change.To provide useful information for predicting the future climate change in China,distinctive regional features in spatial and temporal variations of the surface solar radiation (SSR) and corresponding attributions (such as cloud and aerosol) are analyzed based on SSR observations and other meteorological measurements in North and East China from 1961 to 2007.Multiple models,such as the plane-parallel radiative transfer model,empirical and statistical models,and corrclation and regrcssion analysis methods are used in the study.The results are given as follows.(1) During 1961-2007,the total SSR in North China went through a process from quickly “dimming” to slowly “dimming”,while in East China,a significant transition from “dimming” to “brightening” occurred.Although there are some differences between thc two regional variation trends,long-term variations in SSR in the two regions are basically consistent with the observation worldwide.(2) Between the 1960s and 1980s,in both North and East China,aerosols played a critical rolc in the radiation dimming.However,after 1989,different variation trends of SSR occurred in North and East China,indicating that aerosols were not the dominant factor.(3) Cloud cover contributed less to the variation of SSR in North China,but was thc major attribution in East China and played a promoting role in the reversal of SSR from dimming to brightening,especially in the “remarkable brightening” period,with its contribution as high as 70%. 相似文献
28.
塔克拉玛干沙漠腹地及周边地区PM10时空变化特征及影响因素分析 总被引:2,自引:2,他引:0
利用Thermo RP 1400a对塔克拉玛干沙漠腹地塔中及周边的哈密与和田进行了长达6 a多的沙尘气溶胶PM10连续观测,结合气象资料,分析了该区域沙尘气溶胶PM10的基本特征及影响因素。其结果是:①在哈密、塔中与和田,浮尘、扬沙日数呈上升趋势,沙尘暴日数变化不明显,沙尘天气出现的频率和强度是影响沙漠地区沙尘气溶胶PM10浓度的主要因素。②PM10质量浓度具有明显的区域分布特征,塔克拉玛干沙漠东缘的哈密最低,其次为沙漠南缘的和田,最高的为沙漠腹地的塔中。③每年3—9月是哈密PM10质量浓度的高值时段;塔中与和田PM10质量浓度高值时段分布在3—8月,平均浓度分别在500~1 000 μg·m-3之间变化。④哈密、塔中与和田PM10季节平均浓度变化特征,春季>夏季>秋季>冬季;PM10平均浓度最高的塔中,春季在1 000 μg·m-3左右变化,夏季在400~900 μg·m-3之间,秋冬两季浓度较低基本上在200~400 μg·m-3之间变化。⑤哈密、塔中与和田沙尘暴季节PM10浓度远高于非沙尘暴季节,沙尘暴季节浓度基本上为非沙尘暴季节浓度的两倍以上;塔中2004年和2008年沙尘暴季节平均浓度分别是非沙尘暴季节的6.2倍和3.6倍。⑥沙尘天气过程中PM10质量浓度变化具有以下规律,晴天<浮尘天气<浮尘、扬沙天气<沙尘暴天气。⑦风速大小直接影响大气中PM10浓度,风速越大浓度越高。气温、相对湿度和气压是影响沙尘暴强度的重要因素,也间接影响大气中PM10浓度的变化。 相似文献
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30.
An investigation of the optical response of the atmosphere before, during, and afterthe total solar eclipse of 26 February 1998 at the Caribbean Peninsula of Paraguaná (Falcón State) in Venezuela, was made by measuring photometrically the intensity of the sky brightness in three strategic directions: zenith, horizon anti-parallel or opposite the umbra path, and horizon perpendicular to this path. From these measurements, and by applying in an inverse way an empirical photometric model, very rough estimations of theextinction coefficient, and also of the average optical depth, were obtained in one of these particular directions. However based on meteorological measurements such as those of relative humidity and temperature, and applying a different model, a better estimation in the visual of the total global extinction coefficient of the sky (except the horizon), were made considering the contribution of each component: atmospheric aerosol, water vapour, ozone and Rayleigh scattering. It is shown that this global coefficient is mostly dependent upon aerosol extinction. In spite of the strong reduction of sky brightness photometrically observed during the totality, the results show that the sky was not dark. This is confirmed by the results obtained for the total global extinction coefficient. Additionally it is estimated that the total solar eclipse that took place also in Falcón State, Venezuela, at the beginning of the last century on 3 February 1916, was 30% darker that the 1998 eclipse, and that atmospheric aerosol played a relevant and similar role in the scattering of sunlight during the totality as it was for 1998's. Visual observations made during each event, which show that at length only one or two bright stars could be seen in the sky, support the results obtained for both eclipses. 相似文献