沙尘天气过程沙地下垫面沙尘通量的获取与分析研究

利用浑善达克沙地地区2004年春季沙尘暴和微气象学加强观测实验资料,计算了浑善达克沙地地区不同沙尘天气条件下湍流交换系数、湍流动量通量和感热通量、沙尘浓度通量;研究了沙尘暴过程中湍流作用、沙尘输送特征及起沙条件。结果显示:浑善达克沙地地区非沙尘天气白天近地层热力湍流作用强于动力湍流,湍流交换以感热交换为主;沙尘天气过程中,近地面层湍流动力作用明显增加,湍流动量和感热交换都对湍流输送有主要贡献,感热通量数值有不同程度的降低。较强沙尘暴天气过程中动力湍流强于热力湍流。随着沙尘天气经历起沙、平衡、沉降的演变过程,沙尘通量数值呈现由正值为主,过渡到向上和向下数值相当、向下数值比例增加。非沙尘天气、扬沙天气和沙尘暴天气过程的沙尘通量值范围分别是±5μg/(m2.s)、±30μg/(m2.s)和-200—300μg/(m2.s)之间。浑善达克沙地地区,非沙尘天气也存在一定量的沙尘输送,但数值较小。浑善达克沙地地区沙尘通量与摩擦速度的三次方成正比,为F=Cu3*。临界起沙风速和临界摩擦速度分别约为6m/s和0.4m/s。     

1500—1910年西北地区沙尘天气研究

通过对西北地区明清时期史料的系统查阅,收集到1500—1910年西北地区沙尘天气记录年份137个,最终确定沙尘天气最终数量为250次。分析发现,1500—1910年西北地区的沙尘天气呈波动之势,其中17、19世纪沙尘天气频发态势明显;季节以春季为多;空间分布以甘肃河西走廊、陇东、宁夏北部和南部、陕北、关中一带沙尘记载较多,其中以甘肃民勤为最;沙尘天气与气温的反相关明显,与气候干湿变化的关系在河西地区需要进一步研究,在陕西地区有较为明显的相关性。     

利用多通道MODIS遥感资料反演沙尘气溶胶尺度分布的个例试验

为了利用水面进行大气气溶胶粒子尺度分布的反演,需要水体光谱反射率资料;本文利用水库上空MODIS观测的表观反射率资料来订正出实际的水体光谱反射率。假设在干旱的春季水库水面反射率变化不大,用订正的水库水面光谱反射率平均值进行大气气溶胶尺度分布的反演。从两天个例研究来看,利用多通道MODIS资料可以反演出大气气溶胶粒子的尺度变化。结合天气分析2002年4月11日水库上空气溶胶光学厚度增加、粒子变粗,是由于上游区域的沙尘在高空强西北气流引导下到达本地区。     

沙尘气溶胶辐射强迫全球分布的模拟研究

为了定景了解沙尘气溶胶对气候的影响,文中利用一个改进的辐射传输模式,结合伞球气溶胶数据集(G-ADS),计算了晴空条件下,冬夏两季沙尘气溶胶的直接辐射强迫在对流层顶和地面的全球分布,并讨论了云对沙尘气溶胶辐射强迫的影响.计算结果表明,对北半球冬季和夏季而言,在对流层顶沙尘气溶胶的全球短波辐射强迫的平均值分别为-0.477和-0.501 W/m2;长波辐射强迫分别为0.11和0.085 W/m2;全球平均短波地面辐射强迫冬夏两季分别为-1.362和-1.559 W/m2;长波辐射强迫分别为0.274和0.23 W/m2.沙尘气溶胶在对流层顶和地面的负辐射强迫的绝对值郁随太阳天顶角的余弦和地表反照率的增加而增大;地表反照率对沙尘气溶胶辐射强迫的强度和分布都有重要影响.研究指出:云对沙尘气溶胶的直接辐射强迫的影响不仅取决于云量,而且取决于云的高度和云水路径,以及地面反照率和太阳高度角等综合因素.中云和低云对沙尘气溶胶在对流层顶的短波辐射强迫的影响比高云明显.云的存在都使对流层顶长波辐射强迫减少,其中低云的影响最为明显.因此,在估算沙尘气溶胶总的直接辐射强迫时,云的贡献不可忽视.     

导致一例强沙尘暴的若干天气因素的观测和模拟研究

利用常规观测资料和数值模拟方法对 2 0 0 1年 4月 6～ 8日由蒙古气旋强烈发展触发的内蒙古地区强沙尘暴天气过程进行了分析研究。结果表明 :在这次“锋面气旋型”沙尘暴过程中 ,气旋冷锋是该天气系统引发沙尘暴的主要因素 ,冷锋过境对沙尘暴的触发作用远强于气旋发展。影响沙尘暴的天气因素中 ,地面大风形成主要源于气旋发展和锋后强冷平流 ,高空动量的有效下传则是另一重要原因。高空急流加强及其形成的次级环流使高空动量下传到对流层中层 ,其下方形成深厚混合层使这一动量继续下传到地面 ,是高空动量有效下传的机制。“混合层”可以从本质上反映有利沙尘暴形成的大气层结特征 ,其强度和高度很大程度决定沙尘暴的强弱。这次过程深厚混合层的形成是深厚干对流和强沙尘暴产生的主要原因。而它的形成则是长时间地面加热的结果 ,这也是特强沙尘暴仅发生在内蒙古中部偏北地区而不是下垫面条件更为适宜的内蒙古西部的原因。混合层空气的平流作用对内蒙古中部偏北地区深厚混合层的形成具有相当的贡献 ,其作用程度与地形分布密切相关。地面热通量试验证明地面加热不仅对冷锋过境产生的上升运动强度具有直接影响 ,也影响混合层形成和高空动量下传 ,并因此影响沙尘暴强度。     

The mineralogy and possible sources of spring dust particles over Beijing

A severe Asian Dust Storm （ADS） event occurred on 16-17 April 2006 in northern China. The mineral compositions of dust samples were analyzed using X-ray diffraction （XRD）. The results indicated that dust particles of the ＂17 April 2006＂ dust storm were dominated by quartz （37.4%） and clay （32.9%）, followed by plagioclase （13.7%）, with small amounts of calcite, K-feldspar, dolomite, hornblende and gypsum （all less than 10%）. The clay fractions with diameter less than 2 μm were separated from the dust storm particles by centrifuging and were further analyzed by XRD. The results revealed that the clay species were mainly illite/smectite mixed layers （I/S） （49%） and illite （34%）, with small amount of kaolinite （8%） and chlorite （9%）.
In order to evaluate the feasibility of using the mineralogy to trace the sources of dust particles, the XRD results of the ＂17 April 2006＂ dustfall particles were compared with the dust particles over past years. The results confirmed that the finer dust particles represented by the ADS PM10 displayed a smaller quartz/clay ratio than the dustfall particles. The dust storm particles, either from the ADS PM10 or from the ＂17 April 2006＂ dustfall, showed a lower level of dolomite contents and lower dolomite/clay ratios compared with the non-dust storm dustfall particles. This implies that dolomite could be used to distinguish between the dust contributions from local and non-local sources. Similar trends were found for the gypsum and the gypsum/clay ratio. Moreover, the two dustfall samples had a lower level of illite/smectite mixed layers and a higher level of illite than airborne PM10, implying that the dustfall particles tend to be enriched with illite in its clay fraction.     

2002年春季北京沙尘天气成因及源地分析

利用气象卫星资料对2002年春季北京沙尘天气成因及源地进行分析,得出:我国北方地区连续数年的持续少雨以及2001年冬天以来的异常温暖是2002年北京沙尘天气频发的主要气候原因;2002年春季影响北京的沙尘天气分别来源于蒙古国境内和内蒙古阴山地区及浑善达克沙地毗邻地区,前者所造成的影响明显大于后者。     

Assessment of geochemical and sedimentological characteristics of atmospheric dust in Shiraz,southwest Iran

Geogenic dust is commonly believed to be one of the most important environmental problems in the Middle East.The present study investigated the geochemical characteristics of atmospheric dust particles in Shiraz City(south of Iran).Atmospheric dust samples were collected through a dry collector method by using glass trays at 10 location sites in May 2018.Elemental composition was analysed through inductively coupled plasma optical emission spectrometry.Meteorological data showed that the dustiest days were usually in spring and summer,particularly in April.X-ray diffraction analysis of atmospheric dust samples indicated that the mineralogical composition of atmospheric dust was calcite+dolomite(24%)palygorskite(18%)quartz(14%)muscovite(13%)albite(11%)kaolinite(7%)gypsum(7%)zircon=anatase(3%).The high occurrence of palygorskite(16%-23%) could serve as a tracer of the source areas of dust storms from the desert of Iraq and Saudi Arabia to the South of Iran.Scanning electron microscopy indicated that the sizes of the collected dust varied from 50 μm to0.8 μm,but 10 μm was the predominant size.The atmospheric dust collected had prismatic trigonal-rhombohedral crystals and semi-rounded irregular shapes.Moreover,diatoms were detected in several samples,suggesting that emissions from dry-bed lakes,such as Hoor Al-Azim Wetland(located in the southwest of Iran),also contributed to the dust load.Backward trajectory simulations were performed at the date of sampling by using the NOAA HYSPLIT model.Results showed that the sources of atmospheric dust in the study area were the eastern area of Iraq,eastern desert of Saudi Arabia,Kuwait and Khuzestan Province.The Ca/Al ratio of the collected samples(1.14) was different from the upper continental crust(UCC) value(UCC=0.37),whereas Mg/A1(0.29),K/Al(0.22) and Ti/Al(0.07) ratios were close to the UCC value(0.04).This condition favours desert calcisols as the main mineral dust sources.Analysis of the crustal enrichment factor(EF_(crustal)) revealed geogenic sources for V,Mo,Pb,Sr,Cu and Zn(2),whereas anthropogenic sources affected As,Cd,Cr and Ni.     

空间尘埃等离子体中的重力波特性

建立尘埃等离子体中重力波的基本方程,推导尘埃等离子体中重力波的色散关系,分析地球极区中间层顶处尘埃等离子体层中的重力波特性,研究了重力波在电子密度垂直分层的尘埃等离子体中的反射. 结果表明尘埃等离子体改变了通常大气中的重力内波的色散关系,限制了小水平波数重力内波的传播,改变了波的能量特性,减小了重力波在不均匀大气中垂直向上传播时振幅的增长;在尘埃等离子体中传播时重力波可被电子密度垂直分层的结构反射而导致波能量的集中, 它产生的湍动所导致的空间电子密度的不均匀性分布是极区上空PMSEs的可能机制.     

2017年5月长三角地区一次沙尘重污染天气成因分析

利用地面污染物监测数据、常规气象数据,ECMWF再分析数据以及L-波段无线电探空数据,并结合后向轨迹模型,对2017年5月长三角地区的一次沙尘重污染天气过程进行成因分析。结果表明:此次沙尘重污染过程是天气系统、地面及边界层气象条件共同作用的结果。东亚大槽东移、冷空气南下并配合地面高压的发展使河西走廊、宁夏大部、内蒙古西部出现沙尘天气,为后期长三角地区沙尘的输送提供了沙源; 850 h Pa上较大的风速为上游沙尘源区向下游长三角地区输送提供了通道;高压中心的下沉运动和白天增强的热对流活动使得高层沙尘影响地面具备了足够的动力条件;当沙尘抵达长三角上游地区后,不断减弱的冷空气和趋于静稳的近地面形势不利于污染物扩散,加剧了此次污染过程。