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1.
利用地面水平能见度估算并分析中国地区气溶胶光学厚度长期变化特征 总被引：7，自引：1，他引：6
首先对1980年前后能见度资料非均一性进行了处理, 得到中国地区1960～2005年能见度时间序列, 并由此估算得到气溶胶光学厚度时间序列。对比已有观测及研究结果, 本文获得的气溶胶光学厚度时间序列能够较好地反映出中国地区气溶胶光学厚度长期变化特征。中国地区气溶胶光学厚度呈现逐年增加的趋势, 但1985年后增加趋势减缓, 这种变化在大城市区域表现得更为明显。中国地区气溶胶光学厚度空间分布上呈现东南部高、 西北部低的特征, 东南部地区气溶胶光学厚度普遍大于0.4, 最大值出现在四川盆地, 气溶胶光学厚度超过0.8。 相似文献
2.
利用美国SAGE II (Stratospheric Aerosol and Gas Experiment II)卫星最新版（6.0版）1.020 μm通道逐日气溶胶消光系数资料，得出了对流层中上层及平流层（10 km以上高度）气溶胶光学厚度的平均分布和变化特征。结果表明:气溶胶光学厚度在低纬度大，在印度洋的岛屿上空有三个高值中心，气溶胶光学厚度高值中心与对流层中上层的上升气流的高值中心相对应。与17年(1984～2000年)年平均相比，近6年（1995～2000年）孟加拉湾至青藏高原东南部上空气溶胶光学厚度明显增加；中国东部地区上空气溶胶光学厚度增加，中西部地区则减小。气溶胶光学厚度存在三个经向的增加带和两个经向的减小带。中纬度与赤道之间的布鲁尔-多普森环流（Brewer-Dobson Circulation）带来的低层大气与对流层中上层及平流层之间的气溶胶输送是导致气溶胶这种经向一致变化的主要因素。气溶胶的这种输送产生的近地面大气污染物向中上层大气输送有可能产生重要的气候变化。 相似文献
3.
M. S. Vasiliev S. V. Nikolashkin R. N. Boroyev 《Russian Meteorology and Hydrology》2017,42(11):700-704
The transparency of the atmosphere over the central part of Yakutia is classified using ground-based observations of aerosol optical depth (AOD) for the period of 2004-2014. The annual variations in monthly mean values of AOD are compared with satellite monitoring data. It is revealed that every year the days with the values of AOD corresponding to the class III of atmospheric transparency (turbid atmosphere) made up 25-30% of the total number of AOD measurement days. 相似文献
4.
S. A. Sitnov I. I. Mokhov G. I. Gorchakov A. V. Dzhola 《Russian Meteorology and Hydrology》2017,42(8):518-528
The mechanism of smoke haze formation over the European part of Russia (EPR) in the summer of 2016 is analyzed using satellite measurements, ground-based observations, reanalysis data, and trajectory modeling. The analysis reveals that smoke in the atmosphere over EPR with the aerosol optical depth increase up to 3 was caused by the long-range transport of combustion products from Siberian wildfires. The increase in the concentration of smoke aerosol in the atmosphere over EPR was accompanied by the increase in the concentration of carbon monoxide in the air. The long-range atmospheric transport of the products of pyrogenic emission from east to west for a distance up to 5000 km with the speed of 5–6 m/s predominantly occurred in the lower troposphere. The peculiarities of tropospheric circutation over Northern Eurasia in July 2016 are identified which were responsible for the transport of combustion products in the troposphere for thousands of kilometers in the direction opposite to the westerlies that prevail in the mid-latitudes. 相似文献
5.
Ice samples from the 905 m deep Dome C core (East Antarctica) were studied in terms of insoluble microparticle contents. Various
techniques were used: right angle light scattering, nephelometer (multiangle light scattering), Coulter counter and microscope
analyses, in order to make a thorough study of the physical and optical properties of microparticles and their variations
over the last 30000 years. Because of the possible effect of atmospheric turbidity on the earth-atmosphere radiation balance,
optical parameters of climatic importance were estimated for insoluble microparticles.
The detailed profile of total microparticle mass concentrations shows a drastic (factor of 17 ± 13) difference between high
Last Glacial Maximum (LGM) and low Holocene concentrations. The optical scattering properties of 18000 BP continental dust
do not indicate a significant difference with respect to Holocene dust in terms of particle size distribution and complex
refractive index. The number to log radius size distribution of microparticles for the entire 30 000 yr period can be fitted
by a log-normal distribution with two parameters (modal radius 0.25 ± 0.08 μm; geometric standard deviation 2.2. ± 0.2). However,
for the smallest particles a better adjustment between experimental and theoretical scattering diagrams is obtained by adding
to the observed size distribution another log-normal distribution (modal radius = 0.025 μm, σ
g
= 2). The complex refractive index is 1.53 to 1.56 for the real part and 0.005 ± 0.005 for the imaginary part at the wavelength
used (λ= 546 nm).
During the LGM stage, over the whole of Antarctica, the change in the total optical depth due to the drastic change in the
insoluble aerosol loading is small because insoluble impurities are not the dominant aerosol component. It may have produced
a slight warming of the snow surface (≈ 2 K). In the dust source regions, the optical depth would have been a maximum of 2
to 4 times the present value. The possible warming of the atmosphere in these regions is estimated at 3 K per day and should
therefore be taken into account in paleoclimate reconstruction models. 相似文献
6.
This study simulates optical depth of marine warm clouds for year 2001 based on interactively predicted aerosol concentrations with a global chemical transport model (CTM) driven by the ERA-40 re-analysis meteorological data. The simulated aerosol and cloud droplet number concentrations (CDNC) largely reproduce the variations between polluted and pristine marine environment as revealed by surface and aircraft measurements. By constraining cloud liquid water path (CLWP) with satellite microwave measurements, the simulated global and southern hemispheric aerosol optical depth (AOD) and cloud optical depth (COD) are well within 10% of the observed values. As a result of larger anthropogenic aerosol loadings over the northern oceans, the simulated CDNC and COD are, respectively, by 51 and 18% higher than those over the southern oceans, while the column-averaged droplet effective radius is 13% smaller. These simulated interhemispheric differences, while qualitatively consistent with satellite observations, are larger than the observations. Inclusion of drizzle effect improved the disparities but not entirely. The constrained CTM generally captures the seasonality in AOD and CLWP observations, and demonstrates that annual cycle of COD is dominated by CLWP. During winter monsoon the simulated and observed COD correlate more strongly with changes in AOD over the N. Indian Ocean. 相似文献
7.
1999年6月28日~7月19日在敦煌场, 7月25日~7月31日在青海湖水面场进行了一次大规模综合野外测量试验, 其中采用3台先进的法国CIMEL太阳辐射计对两个场地大气光学特性进行了系统全面测量, 获得大量晴空天气条件下的大气光学数据。利用Langley法处理气溶胶通道数据得到气溶胶光学厚度及其光谱变化。测量结果显示550 nm波长平均气溶胶光学厚度分别为0.12、0.18, 由气溶胶光学厚度的波长变化得到气溶胶Junge参数分别为2.6、3.0, 并与几种典型气溶胶类型比较。结果表明两地在晴空天气里, 气溶胶含量较小, 符合遥感卫星传感器辐射定标的大气条件。 相似文献
8.
利用全球自动观测网（AERONET）纳木错观测点（90．962°E,30．773°N）2009年1～12月的地基观测数据,对青藏高原中部气溶胶光学厚度的分布进行了分析研究,并利用观测结果对MODIS气溶胶光学厚度（AOD）产品进行检验。结果表明,2009年1～12月期间,气溶胶光学厚度月平均值呈现双峰双谷状分布,3月的值最大。9月以后的波长指数a较小,这一时期气溶胶粒子的粒径较大。混浊系数卢的平均值为0．063,说明该地区的空气较为清洁。利用该地基观测资料对MODISAOD产品进行检验,结果表明两者的相关系数平方为0．14,没有通过95％的置信度检验,适用性不显著,需要进一步订正该地区的MODIS气溶胶光学厚度产品。 相似文献
9.
利用地面激光雷达、太阳光度计观测反演气溶胶光学特性参数,结合PM2.5观测数据,分析了2018年1月25—28日北京一次完整污染过程中气溶胶光学特性变化。基于观测数据,利用短波辐射传输模式计算了不同程度污染日,晴空背景下气溶胶对辐射加热率的改变程度。结果表明:清洁日（25日）,PM2.5日平均质量浓度为19.00 μg·m-3,440 nm气溶胶光学厚度为0.13,单次散射反照率为0.87,整层气溶胶消光系数低于0.10 km-1,短波辐射均为增温效应;污染期间（26—27日）,PM2.5日平均质量浓度为83.21 μg·m-3,气溶胶光学厚度为2.48,气溶胶散射能力增强,单次散射反照率达到0.94,气溶胶主要消光层厚度提升至3.00 km高度,消光系数平均值为0.43 km-1,气溶胶在垂直方向的变化导致气溶胶中上层（1.50~3.00 km高度）加热作用强烈,短波辐射加热率平均值达到13.89 K·d-1,而低层（1.50 km高度以内）加热作用较弱,加热率平均值仅为0.99 K·d-1。气溶胶散射能力增强导致加热作用减弱,污染日加热率对于气溶胶散射能力变化更敏感。 相似文献
10.
Yu Zheng Huizheng Che Leiku Yang Jing Chen Yaqiang Wang Xiangao Xia Hujia Zhao Hong Wang Deying Wang Ke Gui Linchang An Tianze Sun Jie Yu Xiang Kuang Xin Li Enwei Sun Dapeng Zhao Dongsen Yang Zengyuan Guo Tianliang Zhao Xiaoye Zhang 《Acta Meteorologica Sinica》2017,31(6):1045-1061
The optical and radiative properties of aerosols during a severe haze episode from 15 to 22 December 2016 over Beijing, Shijiazhuang, and Jiaozuo in the North China Plain were analyzed based on the ground-based and satellite data, meteorological observations, and atmospheric environmental monitoring data. The aerosol optical depth at 500 nm was < 0.30 and increased to > 1.4 as the haze pollution developed. The Ångström exponent was > 0.80 for most of the study period. The daily single-scattering albedo was > 0.85 over all of the North China Plain on the most polluted days and was > 0.97 on some particular days. The volumes of fine and coarse mode particles during the haze event were approximately 0.05–0.21 and 0.01–0.43 μm3, respectively—that is, larger than those in the time without haze. The daily absorption aerosol optical depth was about 0.01–0.11 in Beijing, 0.01–0.13 in Shijiazhuang, and 0.01–0.04 in Jiaozuo, and the average absorption Ångström exponent varied between 0.6 and 2.0. The aerosol radiative forcing at the bottom of the atmosphere varied from –23 to –227,–34 to –199, and –29 to –191 W m–2 for the whole haze period, while the aerosol radiative forcing at the top of the atmosphere varied from –4 to –98, –10 to –51, and –21 to –143 W m–2 in Beijing, Shijiazhuang, and Jiaozuo, respectively. Satellite observations showed that smoke, polluted dust, and polluted continental components of aerosols may aggravate air pollution during haze episodes. The analysis of the potential source contribution function and concentration-weighted trajectory showed that the contribution from local emissions and pollutants transport from upstream areas were 190–450 and 100–410 μg m–3, respectively. 相似文献
11.
《Atmospheric Research》2008,87(3-4):194-206
This work aims at determining the aerosol particle radii in the atmosphere of Athens. Such a work is carried out in Athens for the first time. For this purpose, solar spectral direct-beam irradiance measurements were used in the spectral range 310–575 nm. To estimate the particle radius from aerosol optical depth retrieval, a minimization technique was employed based on the golden-section search of the difference between experimental and theoretical values of the aerosol optical depth. The necessary Mie computations were performed based on the algorithm LVEC.In this study, the mean particle radius of a given distribution was calculated every 30 min during cloudless days in the period November 1996 to September 1997. The largest particles were observed in the summer and the smallest during winter. The result was verified by the increased values of the aerosol optical depth and the turbidity factors calculated in the summer. The differences in the diurnal variation from season to season are attributed to the prevailing wind regime, pollutant emission and sink rates in the atmosphere of Athens. 相似文献
12.
Abstract Temporal variations of the transmission coefficient and aerosol optical depth of the atmosphere are considered using multi‐year observations at the Soviet polar stations in the Arctic. The contribution of atmospheric aerosol to the total extinction of solar radiation is estimated. A decreasing trend of atmospheric transparency due to the increase of aerosol contributing to the extinction of solar radiation during the last 25–30 years is noted. Estimates of the atmospheric aerosol influence on the incoming solar radiation indicate that a further systematic decrease of the transmission coefficient may lead to climatic changes of direct and total radiation in most polluted areas of the Arctic. 相似文献
13.
采用MODIS资料和美国发展的MODIS大气温、湿度廓线统计反演算法,估算大气温度、湿度廓线作为初始场,应用101层快速透过率模式(PFAAST)估算了大气透过率,并采用Newton非线性迭代算法反演中国西北荒漠戈壁地区大气温度廓线。结果表明:该方法对边界层高度及以上部分的大气温度反演得比较好,误差基本都在2 K范围内,边界层范围内的温度反演误差较大,反演误差与气溶胶光学厚度增量和地表温度估算误差呈显著正相关关系,与大气水汽混合比的关系较差。文中从敏感性试验和理论分析角度阐述了地表温度和气溶胶光学厚度估算误差对大气温度反演误差的影响,发现不同光谱波段的地表温度权重均随地表温度的增加有不同程度增加,地表温度反演误差增加将增加地表温度权重,提高地表温度估算误差有助于提高地表温度权重的精度;荒漠戈壁地区大气边界层中气溶胶浓度较高,光学厚度较大,使边界层大气透过率降低,进而降低卫星红外遥感波段的地表温度权重和空气温度权重。由于该模式没有很好地考虑边界层中沙尘气溶胶的影响,使卫星反演的大气透过率偏高,以至于高估地表温度权重和大气温度权重,使得反演的表面温度和空气温度偏低。该研究结合太阳光度计获得的光学厚度资料,采用统计方法对气溶胶效应引起的大气透过率误差和表面温度估算误差进行校正,并对物理算法进行本地化改进,实现了边界层温度廓线的反演。 相似文献
14.
A.D. Adamopoulos H.D. Kambezidis D.G. Kaskaoutis G. Giavis 《Atmospheric Research》2007,86(3-4):194-206
This work aims at determining the aerosol particle radii in the atmosphere of Athens. Such a work is carried out in Athens for the first time. For this purpose, solar spectral direct-beam irradiance measurements were used in the spectral range 310–575 nm. To estimate the particle radius from aerosol optical depth retrieval, a minimization technique was employed based on the golden-section search of the difference between experimental and theoretical values of the aerosol optical depth. The necessary Mie computations were performed based on the algorithm LVEC.In this study, the mean particle radius of a given distribution was calculated every 30 min during cloudless days in the period November 1996 to September 1997. The largest particles were observed in the summer and the smallest during winter. The result was verified by the increased values of the aerosol optical depth and the turbidity factors calculated in the summer. The differences in the diurnal variation from season to season are attributed to the prevailing wind regime, pollutant emission and sink rates in the atmosphere of Athens. 相似文献
15.
The aerosol optical properties and direct radiative forcing over the Mu Us desert of northern China,
acquired through a CE318 sunphotometer of the ground-based Aerosol Robotic Network (AERONET), are analyzed. The
seasonal variations in the aerosol optical properties are examined. The effect of meteorological elements
(pressure, temperature, water vapor pressure, relative humidity and wind speed) on the aerosol optical properties
is also studied. Then, the sources and optical properties under two different cases, a dust event and a pollution
event, are compared. The results show that the high aerosol optical depth (AOD) found in Yulin was mostly
attributed to the occurrence of dust events in spring from the Mu Us desert and deserts of West China and
Mongolia, as well as the impacts of anthropogenic pollutant particles from the middle part of China in the
other seasons. The seasonal variation and the probability distribution of the radiative forcing and the
radiative forcing efficiency at the surface and the top of the atmosphere are analyzed and regressed using
the linear and Gaussian regression methods. 相似文献
16.
Lidar Measurements of Aerosols in the Tropical Atmosphere 总被引：3，自引：0，他引：3
Measurements of atmospheric aerosols and trace gases using the Laser radar (lidar) techniques, have been in pro-gress since 1985 at the Indian Institute of Tropical Meteorology, Pune (18o32’N, 73o51’E, 559 m AMSL), India. These observations carried out during nighttime in the lower atmosphere (up to 5.5 km AGL), employing an Argon ion / Helium-Neon lidar provided information on the nature, size, concentration and other characteristics of the constituents present in the tropical atmosphere. The time-height variations in aerosol concentration and associated layer structure exhibit marked differences between the post-sunset and pre-sunrise periods besides their seasonal va-riation with maximum concentration during pre-monsoon / winter and minimum concentration during monsoon months. These observations also revealed the influence of the terrain of the experimental site and some selected me-teorological parameters on the aerosol vertical distributions. The special observations of aerosol vertical profiles ob-tained in the nighttime atmospheric boundary layer during October 1986 through September 1989 showed that the most probable occurrence of mixing depth lies between 450 and 550 m, and the multiple stably stratified aerosol lay-ers present above the mixing depth with maximum frequency of occurrence at around 750 m. This information on nighttime mixing depth / stable layer derived from lidar aerosol observations showed good agreement with the height of the ground-based shear layer / elevated layer observed by the simultaneously operated sodar at the lidar site. 相似文献
17.
利用静止卫星MTSAT反演大气气溶胶光学厚度 总被引：10，自引：1，他引：9
卫星遥感是获取气溶胶光学特性的重要手段,利用静止卫星可见光通道资料反演气溶胶光学厚度(AOD)的算法使用日本静止气象卫星MTSAT可见光通道资料反演了2008年5月中国地区陆地上的气溶胶光学厚度,将得到的结果分别与AERONET站点的地面观测值进行比较,得到了较好的线性相关关系,再将其与相应的MODIS气溶胶光学厚度产品进行比较,也得到了较为一致的分布,表明MTSAT反演的气溶胶光学厚度产品可以反映大气气溶胶光学厚度的日变化信息。最后对这种反演算法的误差来源进行了分析。 相似文献
18.
Estimation of the Aerosol Radiative Effect over the Tibetan Plateau Based on the Latest CALIPSO Product 总被引：2，自引：0，他引：2
Based on the CALIPSO (Cloud–Aerosol Lidar and Infrared Pathfinder Satellite Observation) Version 4.10 products released on 8 November 2016, the Level 2 (L2) aerosol product over the Tibetan Plateau (TP) is evaluated and the aerosol radiative effect is also estimated in this study. As there are still some missing aerosol data points in the daytime CALIPSO Version 4.10 L2 product, this study re-calculated the aerosol extinction coefficient to explore the aerosol radiative effect over the TP based on the CALIPSO Level 1 (L1) and CloudSat 2B-CLDCLASS-LIDAR products. The energy budget estimation obtained by using the AODs (aerosol optical depths) from calculated aerosol extinction coefficient as an input to a radiative transfer model shows better agreement with the Earth’s Radiant Energy System (CERES) and CloudSat 2B-FLXHR-LIDAR observations than that with the input of AODs from aerosol extinction coefficient from CALIPSO Version 4.10 L2 product. The radiative effect and heating rate of aerosols over the TP are further simulated by using the calculated aerosol extinction coefficient. The dust aerosols may heat the atmosphere by retaining the energy in the layer. The instantaneous heating rate can be as high as 5.5 K day–1 depending on the density of the dust layers. Overall, the dust aerosols significantly affect the radiative energy budget and thermodynamic structure of the air over the TP, mainly by altering the shortwave radiation budget. The significant influence of dust aerosols over the TP on the radiation budget may have important implications for investigating the atmospheric circulation and future regional and global climate. 相似文献
19.
20.
陆地上空标量辐射对地表反射率和大气气溶胶散射都具有很强的敏感性,而偏振反射只对大气气溶胶敏感,对地表不敏感。根据这个原理并结合POLDER(POLarization and Directionality of Earth Reflectance)资料的特点,作者提出综合利用标量辐射和偏振反射信息来实现陆地上空大气气溶胶和地表反照率的同时反演。首先,利用多角度偏振辐射观测提取大气气溶胶光学参数,再利用标量辐射测量对偏振反演结果作进一步筛选和订正,同时获得地表反射率。数值模拟试验结果证明,仅利用偏振信息只能获取大气气溶胶信息,而且其结果误差较大,特别是对于散射作用较强的短波长通道如670 nm误差更大,但经过标量辐射订正后的结果得到明显改善,气溶胶光学厚度和地表反射率与真实值之间相关系数都达到0.99以上。为提高查找表的计算效率,提出并建立了反演方案所需要的半参数化数值表,利用内插方法寻求气溶胶光学厚度和地表反射率的数值解的反演方法。 相似文献