2010年沙尘天气对巴彦浩特空气质量的影响

利用巴彦浩特2010年1月至2011年2月PM10、SO2、NO2的逐日监测数据和同一时期气象观测资料,分析巴彦浩特空气污染物特征及PM10浓度与沙尘天气之间的关系。分析结果表明:2010年春、夏、秋三季巴彦浩特的主要污染物是PM10,冬季主要污染物是SO2;沙尘天气是造成巴彦浩特PM10浓度变化的最重要因素;影响巴彦浩特空气质量的沙尘主要来源于其西北方向和西北偏北方向。建议有关部门在巴彦浩特西北地区搞好生态保护与建设,以减轻沙尘天气对巴彦浩特地区空气质量的影响。     

山西沙尘天气的相关气候因子分析及预测模型的建立

对山西沙尘天气与蒙古国的降水、我国北方积雪日数、青藏高原积雪日数和表征气候异常变化信号的大气-海洋环流因子SOI指数的关系进行了分析,揭示了全球准周期性变化对沙尘天气趋势的主导性作用.得出蒙古国西部前一年降水对山西省的沙尘天气具有较好的指示性;青藏高原前一年冬季积雪日数和山西省的年沙尘日数呈较好的负相关性;当前冬青藏高原积雪日数多时,山西省少沙尘,反之,多沙尘.就我国北方特别是山西省上游地区的积雪日数而言,指示性比较强的区域分布在内蒙古、甘肃、新疆.这些区域内某些站点前一年冬季的平均积雪日数多时,山西省少沙尘,反之,多沙尘.此外,山西沙尘还与SOI指数有显著的滞后2 a的正响应关系,与SOI有滞后两年正相关的站点主要分布在中东部和东北部.在要素相关分析的基础上,综合各类因子制作了山西省沙尘预测模型,以期为沙尘天气的短期预测工作提供一些参考依据.     

Direct Climatic Effect of Dust Aerosol in the NCAR Community Atmosphere Model Version 3 （CAM3）

Direct climate responses to dust shortwave and longwave radiative forcing (RF) are studied using the NCAR Community Atmosphere Model Version 3 (CAM3). The simulated RF at the top of the atmosphere (TOA) is-0.45 W m-2 in the solar spectrum and +0.09 W m-2 in the thermal spectrum on a global average. The magnitude of surface RF is larger than the TOA forcing, with global mean shortwave forcing of-1.76 W m-2 and longwave forcing of +0.31 W m-2 . As a result, dust aerosol causes the absorption of 1.1 W m-2 in t...     

Relationship between East Asian Monsoon and Dust Weather Frequency over Beijing

The relationship between dust weather frequency (DWF), which denotes the number of days of dust weather events, over Beijing and the East Asian Monsoon (EAM) was studied using DWF data for Beijing during the period 1951--2006. Results show that, during this period, the blowing-dust weather frequency (BDWF), as well as the indices of East Asian winter monsoon (EAWM) and East Asian summer monsoon (EASM), all decreased considerably, with a t-test confidence level of 99%. The correlation coefficients between the chosen EAWM index and BDWF over Beijing in winter and the following spring were 0.34 and 0.33, respectively, with significance levels of 0.01 and 0.02, respectively. For the chosen EASM index and BDWF, these correlation coefficients were 0.51 and 0.45, respectively, with both at a confidence level exceeding 99.9%. With the linear trends removed, the values (in the same order as above) were 0.14, 0.14, -0.12, and -0.09, all not significant at the 95% confidence level. Clearly, the EAM relates mainly to DWF over long timescales. To a certain extent, the EAM might have some impact on DWF by affecting the associated surface air temperature and precipitation during the corresponding time period in sand-dust source regions at the interannual scale. A stronger (weaker) EAWM might advance (suppress) the occurrence of DWF, and the opposite for the EASM.     

Compositions and source apportionments of atmospheric aerosol during Asian dust storm and local pollution in central Taiwan

A study has been carried out on water soluble ions, trace elements, as well as PM_2.5 and PM_2.5–10 elemental and organic carbon samples collected daily from Central Taiwan over a one year period in 2005. A source apportionment study was performed, employing a Gaussian trajectory transfer coefficient model (GTx) to the results from 141 sets of PM_2.5 and PM_2.5–10 samples. Two different types of PM₁₀ episodes, local pollution (LOP) and Asian dust storm (ADS) were observed in this study. The results revealed that relative high concentrations of secondary aerosols (NO₃⁻, SO₄²⁻ and NH₄⁺) and the elements Cu, Zn, Cd, Pb and As were observed in PM_2.5 during LOP periods. However, sea salt species (Na⁺ and Cl⁻) and crustal elements (e.g., Al, Fe, Mg, K, Ca and Ti) of PM_2.5–10 showed a sharp increase during ADS periods. Anthropogenic source metals, Cu, Zn, Cd, Pb and As, as well as coarse nitrate also increased with ADS episodes. Moreover, reconstruction of aerosol compositions revealed that soil of PM_2.5–10 elevated approximately 12–14% in ADS periods than LOP and Clear periods. A significantly high ratio of non-sea salt sulfate to elemental carbon (NSS-SO₄²⁻/EC) of PM_2.5–10 during ADS periods was associated with higher concentrations of non-sea-salt sulfates from the industrial regions of China. Source apportionment analysis showed that 39% of PM₁₀, 25% of PM_2.5, 50% of PM_2.5–10, 42% of sulfate and 30% of nitrate were attributable to the long range transport during ADS periods, respectively.     

Continuous Measurement of Number Concentrations and Elemental Composition of Aerosol Particles for a Dust Storm Event in Beijing

A continuous measurement of number size distributions and chemical composition of aerosol particles was conducted in Beijing in a dust storm event during 21-26 March 2001. The number concentration of coarse particles （ 〉2μm） increased more significantly than fine particles （ 〈2μm） during the dust storm due to dust weather, while the anthropogenic aerosols collected during the non-dust-storm period tended to be associated with fine particles. Elemental compositions were analyzed by using proton-induced X-ray emission （PIXE）. The results show that 20 elements in the dust storm were much higher than in the non-dust-storm period. The calculated soil dust concentration during the dust storm was, on average, 251.8μg m^-3, while it was only 52.1μg m^-3 on non-dust-storm days. The enrichment factors for Mg, A1, P, K, Ca, Ti, Mn, Fe, C1, Cu, Pb, and Zn show small variations between the dust storm and the non-dust-storm period, while those for Ca, Ni and Cr in the dust storm were much lower than those in the non-dust-storm period due to significant local emission sources. A high concentration and enrichment factor for S were observed during the dust storm, which implies that the dust particles were contaminated by aerosol particles from anthropogenic emissions during the long-range transport. A statistical analysis shows that the elemental composition of particles collected during the dust storm in Beijing were better correlated with those of desert soil colleted from desert regions in Inner Mongolia. Air mass back-trajectory analysis further confirmed that this dust storm event could be identified as streaks of dust plumes originating from Inner Mongolia.     

Chemical Characteristics of Carbonaceous Aerosols During Dust Storms over Xi＇an in China

Characterization of carbonaceous aerosols including CC (carbonate carbon), OC (organic carbon), and EC (elemental carbon) were investigated at Xi'an, China, near Asian dust source regions in spring 2002. OC varied between 8.2 and 63.7 μg m-3, while EC ranged between 2.4 and 17.2 μ m-3 during the observation period. OC variations followed a similar pattern to EC and the correlation coeflcient between OC and EC is 0.89 (n=31). The average percentage of total carbon (TC, sum of CC, OC, and EC) in PM2.5 during dust storm (DS) events was 13.6%, which is lower than that during non-dust storm (NDS) periods (22.7%). CC, OC, and EC accounted for 12.9%, 70.7%, and 16.4% of TC during DS events, respectively. The average ratio of OC/EC was 5.0 in DS events and 3.3 in NDS periods. The OC-EC correlation (R2=0.76, n=6) was good in DS events, while it was stronger (R2=0.90, n=25) in NDS periods. The percentage of water-soluble OC (WSOC) in TC accounted for 15.7%, and varied between 13.3% and 22.3% during DS events. The distribution of eight carbon fractions indicated that local emissions such as motor vehicle exhaust were the dominant contributors to carbonaceous particles. During DS events, soil dust dominated the chemical composition, contributing 69% to the PM2.5 mass, followed by organic matter (12.8%), sulfate (4%), EC (2.2%), and chloride (1.6%). Consequently, CC was mainly entrained by Asian dust. However, even in the atmosphere near Asian dust source regions, OC and EC in atmospheric dust were controlled by local emission rather than the transport of Asian dust.     

载人飞船主着陆场区强对流天气成因

从数值预报资料入手,结合风廓线雷达、多普勒雷达及自动气象观测资料对2008年9月14日飞船主着陆场区一次雹暴过程进行分析。结果表明:这次雹暴过程中气象要素变化剧烈;侵入蒙古低压的冷锋带动中尺度辐合线移近场区时触发强对流迅猛发展;雹暴前期垂直风切变显著增大;深厚的对流不稳定层结、强烈的正涡度平流和垂直上升运动等是雹暴的主要成因;雹暴前期TBB值迅速降低,雷达RHI回波图上,在无回波穹窿区上部为雹源区;冰雹落在θse舌轴的北侧和高空锋区的南侧。     

MODIS沙尘暴判识方法与业务系统

为了利用MODIS资料对沙尘暴的范围和强度进行定量判识,应用2002--2004年多次MODIS资料,通过对沙尘暴、云、雪和沙漠光谱特征的分析,构建了定量判识沙尘暴范围和强度的两个沙尘指数.利用2002-2007年数次沙尘暴过程对沙尘指数的判别效果进行检验,表明构建的两个M()DIS沙尘指数能够有效地监测沙尘暴的范围和强度,且方法简单,适用于业务应用.针对目前西北沙尘暴遥感监测业务服务以定性图像为主,服务产品较为单一的问题,对MODIS沙尘暴判识方法进行业务化,并结合GIS进行沙尘暴影响范围的分析,开发研制了自动运行的MODIS沙尘暴监测和影响评估业务系统.系统具生成沙尘暴MODIS影像图、沙尘暴范围和强度遥感监测图、沙尘暴影响土地类型图、全国各省(直辖市)沙尘面积统计表、全国不同土地类型沙尘暴影响面积统计表、甘肃省各县沙尘暴的影响面积统计表和甘肃省不同土地类型沙尘影响面积统计表等功能,为沙尘暴定量和精细服务提供了丰富的产品.     

A taxonomic survey of comet composition 1985-2004 using CCD spectroscopy

A summary is presented of our spectroscopic survey of comets extending for roughly 19 years from 1985 to 2004 comprising data for 92 comets of which 50 showed good emissions. All data were re-analyzed using consistent reduction techniques. Our observations of comets over several apparitions and comets observed over an extended period indicate no major changes in compositional classification. To our regret, no major unidentified cometary features were found in our surveyed spectral region of 5200-10400 Å. Absolute production rates for the dominant parent molecule H₂O and the daughter species C₂, NH₂ and CN are determined within the limits of the Haser model as are values for the dust continuum, Afρ. From these data, production rate ratios are calculated for C₂/H₂O, NH₂/H₂O, CN/H₂O and Afρ/H₂O. Excluding the odd Comets Yanaka (1988r), 43P/Wolf-Harrington and 19P/Borrelly, with unusual spectra, our set of comets exhibited relatively uniform composition. Detailed analyses of our data resulted in four taxonomic classes:

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Comets of typical composition (∼70%); exhibiting typical ratios with respect to water of C₂, NH₂, and CN.

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Tempel 1 type (∼22%); having a deficiency in C₂ but normal NH₂ abundance.

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G-Z type (∼6%); having both low C₂ and NH₂ ratios.

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The unusual object Yanaka (1988r) (∼2%?); no detectable C₂ or CN emission but normal NH₂.

It is uncertain whether there is a clear separation between the comets of typical composition and those with C₂ depletion, or whether the latter consists of a group showing a continuum of decreasing C₂/CN ratios. Our spectroscopic investigations result in a visual record of the various compositional classes, which are illustrated in a number of figures. Production rate comparisons with the comet photometry program of Schleicher and A'Hearn [A'Hearn, M.F., and 4 colleagues, 1995. Icarus 118, 223-270] for 13 comets in common yielded good agreement once the different scale lengths are taken into account. An investigation into the possible origin of our compositional groups with respect to dynamical families of comets shows that the Halley family exhibits essentially no C₂ depletion. These objects were presumably formed in the region of Saturn and Uranus and scattered into the Oort cloud. Comets formed in the space near Neptune, responsible for the scattered Kuiper Belt show a mixture of “typical” and C₂ depleted objects, while we associate comets formed in-situ in the classical Kuiper belt with our C₂ depleted group.