'Notches' in the average profiles of bright pulsars     

Maura A. McLaughlin  Joanna M. Rankin 《Monthly notices of the Royal Astronomical Society》2004,351(3):808-812

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A model for 'double notches' in radio pulsar profiles     

G. A. E. Wright 《Monthly notices of the Royal Astronomical Society》2004,351(3):813-822

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涠西南凹陷涠洲10-3油田及围区流三段沉积相研究   总被引：3，自引：0，他引：3  

李茂  董桂玉  漆智 《沉积学报》2015,33(2):314-325

为了促进涠西南凹陷涠洲10-3油田及围区流三段油藏的滚动勘探开发,开展了油区沉积相精细研究。利用岩芯、录井、测井和地震等资料,在识别不同级别层序界面和湖泛面的基础上,将涠洲10-3油田及围区流三段划分为2个长期基准面旋回和8个中期基准面旋回,建立了高分辨率层序地层对比格架。在岩芯描述基础上,进行单井沉积相、连井沉积相、平面沉积相分析,认为研究区流三段发育冲积扇、扇三角洲和湖泊3种沉积相,并系统划分了沉积微相类型。探讨了碎屑流沉积的相带归属,将发育在河道中的碎屑流沉积划分为河道型碎屑流沉积,将单独产出的碎屑流沉积根据沉积环境不同划分为水上非河道化碎屑流沉积和水下非河道化碎屑流沉积。最后对各中期基准面旋回的沉积相展布特征和演化规律进行了探讨,并建立了符合研究区的沉积相模式。  相似文献   

结合VIIRS和监测数据插值的北京雾霾监测方法     

李伟  郑新奇 《测绘学报》2015,(Z1):123-128

本文使用2014-03-20至2014-03-26的北京市VIIRS夜间灯光影像数据和地面监测站PM2.5质量浓度数据,通过遥感图像处理和GIS空间分析相结合,对雾霾强度变化及PM2.5质量浓度空间分布进行分析,提出一种监测雾霾的新方法。结果表明,VIIRS夜间灯光影像成像特征与雾霾浓度变化密切相关,结合同时期地面监测站PM2.5监测数据,能定性反映北京市雾霾强度变化及定量反映PM2.5质量浓度的空间分布。该方法不仅弥补了MODIS等数据在夏季的雾霾监测效果优于冬季的不足,同时也填补了传统光学遥感卫星难以在夜间监测雾霾的空白。  相似文献   

济南PM2.5质量浓度与气象条件相关性初步研究          下载免费PDF全文

黄善斌  李本轩  王文青 《山东气象》2020,40(1):90-97

通过对济南2013年12月—2018年2月PM2.5质量浓度数据分析得出,PM2.5质量浓度平均和最大值均为冬季最高,春秋季次之,夏季最低;PM2.5质量浓度值1月和12月最高,8月最低;其质量浓度呈明显的逐年递减趋势。在不同风向上PM2.5质量浓度存在显著差异性,在N风向和ESE(盛行)风向上均出现了质量浓度较大值,一方面与污染物的异地输送有关,另一方面与济南的特殊地形有关。研究表明,无论污染源在山脉的背风侧还是迎风侧,都很容易导致高浓度污染;尤其在冬季,山脉地形还会加重逆温影响,使污染程度加重。通过相关性研究发现,冬季、春季和秋季,PM2.5质量浓度与相对湿度和平均总云量均呈正相关,与日照时数及其距平呈负相关;冬季,PM2.5质量浓度与平均气温及其距平以及最高、最低气温均呈正相关,与平均、最高、最低气压均呈负相关;春季和秋季,PM2.5质量浓度与气温距平值呈正相关;夏季和秋季,PM2.5质量浓度与日降水量呈负相关,而且随着雨强的增大,对PM2.5的洗消作用越显著。上述变量间相关性均通过了P≤0.01显著性检验。  相似文献   

利用WRF-Chem模拟研究京津冀地区夏季大气污染物的分布和演变   总被引：9，自引：4，他引：5  

庞杨  韩志伟  朱彬  李嘉伟 《南京气象学院学报》2013,(6):674-682

应用WRF—Chem（Weather Research and Forecasting Model with Chemistry）模式模拟研究了2007年8月京津冀地区近地面O3、NO2、PM2.5浓度的时空变化特征,将模拟结果与观测数据进行详细对比,结果表明,模式可以较好地模拟O3、PM2.5,浓度的空间分布和时间变化特征,成功再现了8月33和PM2.5的几次积累增加过程,其中O,的模拟值与观测值的相关系数为0．69～0．86,PM2.5的相关系数为0．44～0．49,但模式对NO2的模拟相对较差,相关系数为0．27～0．43。北京、天津地区为O3月均低值区,月均体积浓度约30×10^-9,渤海及京津冀以西地区O3月平均体积浓度可达60×10^-9;PM2,呈现南高北低的分布特征,变化范围为120～240μg／m3。14时月平均03体积浓度在北京、天津地区低于周边地区,约为60×10^-9;而PM2.5质量浓度在环渤海地区和河北南部较高,为100～120μg/m^3。8月17日北京出现一次典型的高浓度O,污染事件,14时北京地区温度达到33℃,O3体积浓度为80×10^-9～110×10^-9。在局地排放、化学反应和外来输送的共同作用下,渤海西岸和北岸PM2.5的质量浓度超过120μg／m3,其中二次气溶胶质量浓度为50～100μg／m3,一次排放人为气溶胶质量浓度为10～20μg／m3,海盐质量浓度为1～7μg／m3,二次气溶胶是该地区PM2.5的主要贡献者。  相似文献   

2010-2011年鞍山市能见度特征          下载免费PDF全文

赵胡笳  马雁军  朱轶明  高清源 《气象与环境学报》2013,29(1):18-22

利用2010年6月至2011年5月鞍山大气成分观测站的能见度资料,统计分析能见度与PM₁₀、PM_2.5、PM_1.0质量浓度、风速、降水强度和气溶胶光学厚度等气象要素的相关性。结果表明：鞍山市能见度月均值从8月份开始呈上升趋势,11月份达到峰值后开始显著下降,2月份达到最低值,自3月开始又出现较大幅度增长,进入夏季后略有下降;PM_2.5/PM₁₀、PM_1.0/PM₁₀比值与能见度呈反相关,能见度增大,PM_2.5/PM₁₀、PM_1.0/PM₁₀比值减小,且PM_1.0/PM₁₀的减小趋势更大,说明影响能见度的颗粒物以细粒子为主。平均风速与能见度变化趋势基本一致,与PM_2.5/PM₁₀、PM_1.0/PM₁₀的变化趋势呈反相关。随着雨强的增大,降水日能见度平均值随之减小,降水前一日和后一日的能见度平均值均大于降水日,且降水前一日及后一日的能见度改变量及改变率的绝对值随着降水强度的增加而增加。波长指数的变化说明影响鞍山能见度变化的污染物粒子整体较稳定,能见度与AOD成明显的反相关。  相似文献   

Concentrations and Distribution of Trace Metals of PM_(10) and TSP Particles Collected in the Qingdao Area     

LI Xianguo  FENG Lijuan  QI Jianhua  CHEN Xingmao  ZHANG ManpingCollege of Chemistry & Chemical Engineering  Ocean University of China  Qingdao  P.R.China 《中国海洋大学学报(英文版)》2003,2(2)

Aerosol samples of PM10 (particulate matter with aerodynamic diameters less than 10μm) and TSP (total suspended particles) were simultaneously collected from April 2001 to March 2002 at the top of Mount Baguan on the downtown campus of Ocean University of China, Qingdao, China. The concentrations of Al, Fe, Mn, Cu, Pb and Zn were determined by means of inductively coupled plasma atomic emission spectrometry (ICP-AES). The monthly variability of the mass concentrations of aerosol particles and the concentrations of trace metals are presented and discussed. The distribution pattern of these metals in PM10 and TSP is also discussed. During the observation period, the mass concentration of PM10 at this site ranged from 13.80 to 306.42μgm-3 , while that of TSP ranged from 31.02 to 568.82μgm-3. Both PM10 and TSP reached their highest concentrations in springtime, while the lowest values occurred in summertime. The concentrations of crustal metals followed the same variation pattern, while those of anthropo  相似文献   

Atmospheric boundary-layer structure observed during a haze event due to forest-fire smoke   总被引：1，自引：0，他引：1  

Markus?PahlowEmail author  Jan?Kleissl  Marc?B.?Parlange 《Boundary-Layer Meteorology》2005,114(1):53-70

During a haze event in Baltimore, U.S.A. from July 6 to 8, 2002, smoke from forest fires in the Québec region (Canada), degraded air quality and impacted upon local climate, decreasing solar radiation and air temperature. The smoke particles in and above the atmospheric boundary layer (ABL) served as a tracer and provided a unique opportunity to investigate the ABL structure, especially entrainment. Elastic backscatter lidar measurements taken during the haze event distinctly reveal the downward sweeps (or wisps) of smoke-laden air from the free atmosphere into the ABL. Visualisations of mechanisms such as dry convection, the entrainment process, detrainment, coherent entrainment structures, and mixing inside the ABL, are presented. Thermals overshooting at the ABL top are shown to create disturbances in the form of gravity waves in the free atmosphere aloft, as evidenced by a corresponding ripple structure at the bottom of the smoke layer. Lidar data, aerosol ground-based measurements and supporting meteorological data are used to link free atmosphere, mixed-layer and ground-level aerosols. During the peak period of the haze event (July 7, 2002), the correlation between time series of elastic backscatter lidar data within the mixed layer and the scattering coefficient from a nephelometer at ground level was found to be high (R=0.96 for z =324 m, and R=0.89 for z=504 m). Ground-level aerosol concentration was at a maximum about 2 h after the smoke layer intersected with the growing ABL, confirming that the wisps do not initially reach the ground.  相似文献   

Effects of the number of stations and time resolution on derivation     

Odim Mendes  Jr.  Aracy Mendes da Costa  Fernando Celso Perin Bertoni 《Journal of Atmospheric and Solar》2006,68(18):2127-2137

For at least 30 years now it has been well known that the Dst index can be modelled using the solar wind as input. Since then, many attempts have been made to improve the predictability of Dst using different approaches. These attempts are useful, for instance, to understand which features of the solar wind–magnetosphere interactions are most important in producing magnetospheric activity and how the Dst index would improve the space weather forecast. The Dst index is by far the most reliable and simple indication that a magnetic storm is in progress. In this work, the effect of using more than four magnetic stations and shorter time intervals than the hourly averages used in Sugiura's procedures is evaluated. The discussion is based on the results presented by Burton in 1975 and Feldstein in 1984 considering 4 or 12 magnetic stations and time averages of 2.5 min for a magnetic disturbed period that occurred from February 7–28, 1967, including two geomagnetic storms. The analysis has shown that the global representation of a magnetic storm by the standard Dst (Sugiura) is well preserved either using 4, 6, 12 magnetic stations or using 1 h, 2.5 min 1 min averages. A brief review of the current understanding of Dst has been included to support the discussions. The analysis performed has shown that a more refined Dst index (time and number of stations>4) would be useful to investigate the intrinsic processes and the different current systems involved in the ring current development during magnetic storms; the standard Dst, as it is conceived, is quite adequate to monitor geomagnetic storms and identify their overall features; concerning the magnetic stations normally considered, the inclusion of higher magnetic latitude stations (>35) may underestimate the observed Dst.  相似文献