生物质燃烧颗粒物有机示踪化合物的测定和应用   总被引：2，自引：0，他引：2  

张烃刘咸德  董树屏祁辉 Hélène Cachier Magda Claeys 《岩矿测试》2006,25(2):107-113

使用气相色谱-质谱法对2002年7月-2003年7月的北京市大气粗、细颗粒物样品中的左旋葡聚糖等糖类化合物进行了测定。结果表明，左旋葡聚糖主要存在于细颗粒中，可以作为示踪化合物来研究生物质燃烧现象。生物质燃烧对北京市大气颗粒物有较重要的贡献。对应于12％-40％的PM2.5有机碳和10％-33％的PM10有机碳。北京市在2002年10月和11月受到明显的生物质燃烧的影响，可能由于农田秸杆焚烧和秋季落叶焚烧。2003年5月7日颗粒物样品受到直线距离约为1000km以外的内蒙古自治区呼伦贝尔市大兴安岭林区森林大火烟雾的影响。生物质燃烧事件具有突发性，可以长距离传输；生物质作为农村生物燃料的使用其燃烧排放具有经常性和持久性的特征。  相似文献   

云模式中气溶胶物理过程参数化方案研究概述   总被引：2，自引：1，他引：2  

刘校辰  刘奇俊 《气象》2006,32(6):3-12

介绍了大气气溶胶的浓度、气溶胶的谱形等物理性质对云的微物理过程造成的影响以及目前云模式中常用到的一些气溶胶物理过程的体积水、分档等参数化方案，并评述了这些参数化方案各自的特点。提出了在设计气溶胶物理过程参数化方案时需要注意和有待解决的几个问题，建议在设计气溶胶-云相互作用的模式时，要根据不同的研究目的选择合适的参数化方案。  相似文献   

国内外气溶胶观测网络发展进展及相关科学计划   总被引：16，自引：6，他引：16  

延昊  矫梅燕  毕宝贵  刘桂清 《气象科学》2006,26(1):110-117

气溶胶是气候变化研究中的一个极大的不确定性因素,国内外在此方面开展了大量的观测和科学研究。本文首先对当前全球两大气溶胶观测网络,世界气象组织(WMO)的全球大气观测计划(GAW)和气溶胶自动观测网(AERONET)的组织、规模、设备、数据和气溶胶网络的规范作了介绍,并对近年来国际上的重大气溶胶科学计划的目标、实验方法、步骤作了介绍,说明观测网络的重要性。在此基础上对中国气溶胶观测网络的地位做了分析,并指出其在正在开展的中国气溶胶科学研究中的重要性。  相似文献   

大城市气溶胶对光化辐射通量及臭氧的影响研究(Ⅰ)——国内外研究现状与观测事实述评   总被引：3，自引：7，他引：3  

邓雪娇  吴兑  铁学熙  李菲  谭浩波  毕雪岩 《广东气象》2006,(3):10-17

介绍了气溶胶对光化辐射通量及臭氧的影响研究的国内外动态,分析了广州城市气溶胶对紫外线及臭氧影响的观测实例,说明了大气气溶胶与臭氧变化规律及其相互作用机制研究已成为大气化学研究领域具有重要理论和实用价值的前沿课题。  相似文献   

沙尘气溶胶对西北地区植被遥感的影响分析     

张杰  郭铌  郝志毅 《高原气象》2006,25(1):116-122

选取扬沙—浮尘天气发生中、后的对地观测卫星EOS-MODIS数据,利用6S辐射传输模式对该卫星资料进行大气订正,分析了沙尘气溶胶对沙尘多发区的西北地区植被指数(VI)遥感的影响。结果表明,与晴空天气得到的反射率相比,沙尘使红光通道反射率ρ1、近红外通道反射率ρ2和蓝光通道反射率ρ3均增加,归一化植被指数NDVI有不同程度的降低,降低最大值为0.246。抗大气植被指数ARVI也有所降低,降低最大值为0.231。应用晴空天气条件下的资料,建立了西北干旱区ARVI与NDVI之间的线性关系,并证明了在沙尘天气条件下,利用ARVI计算NDVI的方法,所得的结果较好。  相似文献   

Characteristics of Aerosol Ionic Compositions in Summer 2003 at Lin''''an of Yangtze Delta Region   总被引：1，自引：0，他引：1       下载免费PDF全文

YAN Peng  ZHANG Yangmei  YANG Dongzhen  TANG Jie  ZHOU Xiuji 《Acta Meteorologica Sinica》2006,20(3):374-382

With the size-resolved aerosol mass and ion composition data obtained at Lin'an regional atmospheric pollution monitoring station in July 2003, the size distributions of aerosol mass and ionic components, and the correlations between major ion pairs were analyzed. The primary results indicate that in the period of in-situ measurement, the aerosols are mainly composed of fine particles. The mass of aerosols with size less than 2.1μm accounts for 66% of the total mass of all size ranges, in which about 50% of the mass is contributed by the particles with size less than 0.65μm. Similar to the size distributions of aerosol mass, the water-soluble ions are mainly concentrated in the size range of <0.65μm, accounting for about 77% of the sum of analyzed ions, and the ions within the range of <2.1μm reach 88%. The sulfate, ammonium, and potassium are the dominant ionic components in fine particles (particle size less than 2.1μm). Ion correlation analysis suggests that the sulfates in fine particles are mostly in the compounds of (NH4)2SO4, Na2SO4, and K2SO4, but for submicron particles the sulfates are mainly in the form of (NH4)2SO4.  相似文献   

大气臭氧总量的经验计算方法   总被引：1，自引：0，他引：1  

白建辉 《南京气象学院学报》2006,29(6):799-805

依据臭氧生消与紫外辐射(UV)能量利用相互作用的观点,考虑与臭氧有关的主要因子UV、大气中物质在化学和光化学反应中对UV能量的吸收、气溶胶粒子的散射等,在分析1990—1992年臭氧总量、太阳辐射、气象资料的基础上,建立了计算臭氧总量的经验模式,其优点是所用资料均可由常规气象站获得。结果表明,计算值与观测值符合得比较好。利用该经验模式计算了北京地区1979年1月—1996年6月的臭氧总量,计算值与观测值同样比较一致,二者相对偏差的最大值、最小值、平均值分别为15.2%、0.05%和4.9%,相对偏差在±10%之内的比例为91.4%,因而该经验模式是合理、可行的。1991年之后北京地区臭氧的下降与Pinatubo火山气溶胶的影响有关。  相似文献   

Atmospheric Electrification in the Solar System     

Karen L. Aplin 《Surveys in Geophysics》2006,27(1):63-108

Atmospheric electrification is not a purely terrestrial phenomenon: all Solar System planetary atmospheres become slightly electrified by cosmic ray ionisation. There is evidence for lightning on Jupiter, Saturn, Uranus and Neptune, and it is possible on Mars, Venus and Titan. Controversy surrounds the role of atmospheric electricity in physical climate processes on Earth; here, a comparative approach is employed to review the role of electrification in the atmospheres of other planets and their moons. This paper reviews the theory, and, where available, measurements, of planetary atmospheric electricity which is taken to include ion production and ion–aerosol interactions. The conditions necessary for a planetary atmospheric electric circuit similar to Earth’s, and the likelihood of meeting these conditions in other planetary atmospheres, are briefly discussed. Atmospheric electrification could be important throughout the solar system, particularly at the outer planets which receive little solar radiation, increasing the relative significance of electrical forces. Nucleation onto atmospheric ions has been predicted to affect the evolution and lifetime of haze layers on Titan, Neptune and Triton. Atmospheric electrical processes on Titan, before the arrival of the Huygens probe, are summarised. For planets closer to Earth, heating from solar radiation dominates atmospheric circulations. However, Mars may have a global circuit analogous to the terrestrial model, but based on electrical discharges from dust storms. There is an increasing need for direct measurements of planetary atmospheric electrification, in particular on Mars, to assess the risk for future unmanned and manned missions. Theoretical understanding could be increased by cross-disciplinary work to modify and update models and parameterisations initially developed for a specific atmosphere, to make them more broadly applicable to other planetary atmospheres.  相似文献   

Trace Metal Solid State Speciation in Aerosols of the Northern Levantine Basin,East Mediterranean   总被引：3，自引：0，他引：3  

Mustafa Koçak  Nilgun Kubilay  Barak Herut  Malcolm Nimmo 《Journal of Atmospheric Chemistry》2007,56(3):239-257

An established three stage sequential leach scheme was applied to a series of selected high volume aerosol samples (n = 35) collected from the Turkish Eastern Mediterranean coastline (Erdemli). Samples were selected according to their air mass back trajectory history to reflect the contrasting mixtures of aerosol material present in the Eastern Mediterranean marine aerosol. Two populations were adopted, those samples which were classed as “anthropogenic” and those which were “Saharan” dominated aerosol populations. Applying the three stage leach it was possible to define the proportion for each of the considered metals (Al, Fe, Cu, Pb, Cd, Zn and Mn) present in the (a) “exchangeable” (b) “carbonate / oxide” and (c) “refractory” phases, representing novel solid state aerosol speciation data for this marine system. Clear trends were established, conforming with data from previous studies with mainly crustal derived metals (Al and Fe) being present in the refractory phases (Al > 88%; Fe > 84%) and those influenced by anthropogenic sources being dominating in the exchangeable phase, although for these metals the variability was comparatively high (12–64%; 19–85%; 40–100% for Zn, Pb and Cd, respectively). For the majority, greater exchangeable fractions were present the lower the crustal source contribution to the aerosol population, whereas the “refractory” fraction exhibited contrasting behaviour. This was illustrated by the novel application of the mixing diagram, presenting each of the three speciation stages against the corresponding percent anthropogenic contribution to each collected sample. Zn, Pb and Cd all illustrated progressive decrease in the percent exchangeable with increasing crustal contribution to the aerosol population. The percent exchangeable was discussed in terms of its use to represent the upper limit of the bioavailable fraction of metal associated with the aerosol, post deposition. The mixing diagram approach enabled the prediction of the residual fractions for Cd, Pb and Zn (41 ± 4%; 62 ± 4% and 82 ± 5%, respectively,) in Saharan end-member material.  相似文献   

Study on Two Categories of Sudden Stratospheric Warming   总被引：1，自引：0，他引：1       下载免费PDF全文

ZHANG Hengde  GAO Shouting  LU Weisong 《Acta Meteorologica Sinica》2007,21(4):450-464

  相似文献