中国利用星载激光雷达开展沙尘和污染研究的综述   总被引：1，自引：0，他引：1       下载免费PDF全文

王天河  孙梦仙  黄建平 《大气科学学报》2020,43(1):144-158

激光雷达作为一种新兴的主动遥感探测工具,被广泛应用于大气遥感、环境监测等领域。星载激光雷达由于其较广的探测范围、较高的时空分辨率、可获得连续的廓线数据等优势,已经成为全球及区域气溶胶和云特性观测研究的强有力工具。本文总结了自2006年CALIPSO卫星发射以来,中国科学家在利用其开展沙尘气溶胶及污染研究方面的工作,重点阐述了沙尘气溶胶的时空分布、远距离传输、分类识别、光学特性、沙尘释放、辐射与气候效应,以及灰霾和烟尘特性等方面的最新研究成果。对以上研究成果的梳理,有助于深入理解中国在利用星载激光雷达开展沙尘与污染研究的水平,也为未来开拓中国自主研发星载激光雷达的遥感应用领域奠定了基础。  相似文献   

阿拉善高原干涸湖床沉积物与华北地区沙尘暴   总被引：16，自引：3，他引：13  

岳乐平  杨利荣  李智佩  王珉  张维吉  聂浩刚  张睿  武力超 《第四纪研究》2004,24(3):311-317

文章通过内蒙古阿拉善高原古居延泽干涸湖床沉积物、周缘活动沙丘、沙质草原地表土壤及古代弃荒土地的粒度组成分析,论述干涸湖床沉积物对沙尘天气的影响。古居延泽湖床沉积粒度分析结果表明,干涸湖床的地表湖相沉积物粒径小于10μm的颗粒占64%以上,可以在一般风暴条件下在大气中搬运几千公里,这意味着西北地区干涸湖床产生的粉尘在风暴作用下可以横扫整个东亚北部地区。中国西北地区冬、春季多西北风造成沙尘暴或扬沙天气,西部沙漠、沙地或沙质草场遭遇强风时沙尘被席卷进气流,但其中粗砂粒扬起的高度、搬运的距离有限,当风力稍稍减弱,粗颗粒砂粒沉降,而粉尘继续悬浮运移。当强风途径下一个沙区时新的沙尘加入,沙尘暴呈“接力方式”继续向东南部移动。  相似文献   

A global satellite view of the seasonal distribution of mineral dust and its correlation with atmospheric circulation     

《Dynamics of Atmospheres and Oceans》2014

Aerosols make a considerable contribution to the climate system through their radiative and cloud condensation nuclei effects, which underlines the need for understanding the origin of aerosols and their transport pathways. Seasonal distribution of mineral dust around the globe and its correlation with atmospheric circulation is investigated using satellite data, and meteorological data from ECMWF. The most important sources of dust are located in North Africa, the Middle East and Southwest Asia with an observed summer maximum, and East Asia with a spring peak. Maximum dust activity over North Africa and the Middle East in summer is attributed to dry convection associated with the summertime low-pressure system, while unstable weather and dry conditions are responsible for the spring peak in dust emission in East Asia. Intercontinental transport of mineral dust by atmospheric circulation has been observed, including trans-Atlantic transport of North African dust, trans-Pacific transport of Asian dust, and transport of dust from the Middle East across the Indian Ocean. The extent of African dust over the Atlantic Ocean and its latitudinal variation with season is related to the large-scale atmospheric circulation, including seasonal changes in the position of the intertropical convergence zone (ITCZ) and variation of wind patterns. North African aerosols extend over longer distances across the North Atlantic in summer because of greater dust emission, an intensified easterly low level jet (LLJ) and strengthening of the Azores-Bermuda anticyclonic circulation. Transport of East Asian aerosol is facilitated by the existence of a LLJ that extends from East Asia to the west coast of North America.  相似文献   

2014年4月大气环流和天气分析   总被引：2，自引：1，他引：1  

樊利强  张涛  孙瑾 《气象》2014,40(7):898-904

2014年4月大气环流特征为,北半球极涡呈单极型分布,中心位于喀拉海北端附近;亚洲大陆东部高压脊强度偏强,导致4月我国气温较常年同期(11.0℃)偏高1.1℃,为1961年同期以来第五高值。东亚大槽强度和位置、南支系统和西北太平洋副热带高压接近常年平均状况。4月全国平均降水量为43.7 mm,比常年同期略偏少。月内,江南南部和华南等地出现短时强降水、雷雨大风等强对流天气;北方地区出现多次沙尘天气过程;此外,部分站次出现极端高温、极端降温事件。  相似文献   

青岛一次沙尘污染事件的气象条件特征     

马艳  郭丽娜  黄容 《干旱气象》2014,(5):773-780

2008年5月28日至6月1日青岛市区出现了持续5 d的大气污染,其中29-30日为重度污染,其余3日为轻度污染。本文基于青岛常规地面和高空观测资料以及环境监测站SO2、NO2、PM10监测资料,利用资料分析和中尺度数值模拟的方法,分析造成青岛此次持续多日的大气污染的污染源、大气环流和气象要素特征。分析结果表明：此次污染过程主要是外来沙尘引起的PM10污染;持续较强的逆温层结以及近地面层弱南北风频繁交替出现造成沙尘在近地层往复、积聚,最终导致连续多日的空气污染。  相似文献   

一次雷暴大风引发的强沙尘暴天气的中尺度系统分析     

王伏村  付双喜  张德玉  张浩文  代德彬  刘玉洁 《干旱气象》2014,32(6):954-961

使用探空、地面和张掖多普勒天气雷达观测资料对2013年7月30日发生在河西走廊的一次强沙尘暴天气进行了分析。结果表明：这次雷暴大风沙尘天气是对流层低层冷平流作用下,不稳定能量释放形成的β、γ中尺度对流系统造成的,雷暴下击暴流的辐散流和密度流是引发地面强风和沙尘暴的直接因素。高层干、中层相对湿和低层干的层结,易产生雷暴大风天气。1 h正变压和负变温演变能很好地反映雷暴下击暴流形成的雷暴高压和冷池的强弱变化,同时也反映了下击暴流的辐散气流和冷池密度流造成的地面大风及沙尘天气的变化。  相似文献   

Accumulation and risk assessment of heavy metals in dust in main living areas of Guiyang City,Southwest China     

Xiaoyan Li  Shuting Zhang  Mei Yang 《中国地球化学学报》2014,33(3):272-276

Guiyang is a famous tourist city located in southwestern China. In this study, dust from eleven residential areas, seven city squares, and nine schools was collected to measure the heavy metal levels and evaluate its risk. At each sampling site, 4-5 sub-samples were taken as a bulk sample. All samples were air-dried, ground, passed through a 0.105 mm nylon sieve, digested with HNO3-HC104 to determine the concentrations of Cd, Cu, Ni, Pb and Zn by ICP-MS, and digested with 1：1 aqua regia to determine As by AFS. The results show that the concentrations of As, Cd, Cu, Ni, Pb and Zn in dust of Guiyang City follow normal distribution with means of 16.1, 1.54, 138, 47.7, 129 and 479 mg/kg, respectively. Levels of As, Cd, Cu, Ni, Pb and Zn exceed the background level of soil in Guizhou Province by 33%, 96%, 100%, 78%, 96%, and 100%, respectively. Cd, Cu, Pb and Zn are heavily accumu- lated in dust of living areas with accumulation factors of 4.10, 5.12, 4.12 and 5.51, respectively. City square pos- sesses the highest geometric means of As, Cd, Cu, Pb, and Zn. The risks of heavy metal exposure to teenagers are not obvious and in an order ofAs〉Pb〉Cu〉Ni〉Zn （Cd）.  相似文献   

Salt Desert and Saline-Ackaline Mixed Dust Storms:An Ignored Issure for Global Climate Change     

SONG Huailong 《《地质学报》英文版》2014,88(Z1):196-197

正Salt desert,saline-alkaline dust storm and saline-alkaline mixed dust storm are significant but ignored problems for a long time.After many years of observations and researches,the author believes that salt desert,saline-alkaline dust  相似文献   

干涸尾闾湖盆区泥漠地表磨蚀释尘特征     

曲书锋  张国明  刘连友  李力  肖雨婷  向明珠  孙煦然  韩旭娇 《中国沙漠》2022,42(4):81-88

沙粒的表面磨蚀效应是地表产尘、释尘的重要机制,针对干湖盆泥漠地表开展磨蚀释尘实验研究,对理解干湖盆地表风蚀过程及盐碱尘暴形成机理具有重要意义。对采自西居延海干涸湖盆泥漠地表土样进行室内磨蚀模拟实验,研究了不同粒级（细、中、粗）沙粒不同落沙角度（30°,45°,60°）的磨蚀效应。结果表明：（1）泥漠地表磨蚀实验中能够产生明显释尘效应的沙粒粒级阈值为中沙（0.25 mm<M_d<0.50 mm）;（2）磨蚀粒径粒级相同时,磨蚀角度会对泥漠地表磨蚀释尘速率产生影响,磨蚀量的角度排序为60°>30°>45°,但同一粒级3种角度下的磨蚀释尘率差异不显著。（3）磨蚀角度为45°时,计算了泥漠地表的质量磨蚀率与能量磨蚀率,其中中沙为0.04 g·kg^-1、0.43 g·J^-1,粗沙为0.08 g·kg^-1、0.74 g·J^-1,极粗沙为0.26 g·kg^-1、2.54 g·J^-1;在磨蚀沙粒粒级倍增而磨蚀角度不变情况下,泥漠地表磨蚀释尘率与能量磨蚀率未发生正比例线性增长变化。  相似文献   

Hα emission objects in Circinus     

S. Noroozi  M. Haas  Z. Chen  R. Chini 《Astronomische Nachrichten》2013,334(3):282-287

We present a new survey for Hα emission objects in the Circinus cloud complex and introduce an efficient photometric method for detecting Hα emission via observations in a narrow‐band filter. The observed flux is compared to a blackbody fit of the continuum. Our search strategy reveals 20 stars with strong Hα emission (EW > 10 Å), eight of them being new detections. All Hα stars display infrared excess corroborating their youth. On the other hand, the region contains a number of infrared excess objects that do not show Hα emission. Our results support the picture that accretion – as witnessed by Hα emission – is a highly variable phenomenon. Therefore, Hα surveys can only trace the temporarily active objects. In contrast, infrared excess is a more robust tracer that reveals most of the population of young stellar objects in a star forming region. Our analysis of the general stellar content of the region yields a reliable distance of 450 pc for the Circinus cloud. Moreover, we find a ratio of total‐to‐selective extinction of R^V = 2.8 suggesting that smaller‐than‐normal dust grains may be present. (© 2013 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)  相似文献