福建省复杂地形下旬平均气温分布式模拟     

李威鹏  邱新法  曾燕  施国萍  徐金勤  王丹丹 《热带地理》2019,39(2):229-236

为建立高时空分辨率的福建省复杂地形下气温栅格数据集，利用福建省及其周边33个常规气象站观测资料，基于数字高程模型（DEM）数据，综合考虑海拔、太阳总辐射、地表长波有效辐射对旬平均气温的影响，模拟了福建省复杂地形下旬均温的空间分布。结果表明：1）常规站验证结果显示：各旬气温绝对误差平均值（MAE）最小为0.46℃，最大为2.3℃，全年平均为0.87℃；加密站验证结果显示，MAE最大为2.3℃，最小0.5℃，全年平均为0.96℃。2）模拟结果能反映旬均温的宏观分布规律与局地细节特征。宏观范围内，旬均温受纬度影响较大，由北至南气温逐渐升高，沿海地区旬均温整体高于内陆，山区旬均温明显较低；局地范围内，各坡向上气温差异显著，海拔越高、坡度越大，差异越明显；地形因子对旬平均温的影响具有季节差异，具体表现为冬季时地形因子对旬均温的影响最大，秋季次之，春夏季节中地形因子对旬均温的影响最弱。  相似文献   

江苏省夏季浓雾的时空分布特征及气象影响因子分析     

宗晨  钱玮  包云轩  袁成松  周林义  崔驰潇  王宏斌 《气象》2019,45(7):968-977

利用江苏省70个国家基本站逐10 min连续观测资料,对江苏省夏季浓雾的时空分布特征及影响因子进行分析研究。结果表明:(1)夏季浓雾易在气温小于29℃、风速低于3 m·s~(-1),且盛行偏东风的条件下形成;低温高湿的梅雨期是夏季浓雾在6月高发(42.4%)的可能原因。(2)夏季浓雾生消时间与秋、冬季显著不同,主要发生于00—06时,消散集中于05—08时,持续时间主要在6 h以内。(3)夏季浓雾以辐射雾为主,辐射雾、平流雾和锋面雾分别占58. 1%、35. 5%和6.4%。(4)夏季浓雾发生频次呈现从东北部沿海地区向西南部内陆地区递减的趋势,淮北地区夜间降温幅度高于苏南地区是出现这一现象的主要原因。(5)成雾前6～24 h出现的弱降水为近地层提供水汽,此后天气转晴,静稳的大气层结下有利于夏季浓雾的出现。  相似文献   

苏州市一次重霾污染天气过程的数值模拟   总被引：1，自引：1，他引：0  

吴珂  包云轩  蔡敏  金建平  牛利  严明良 《气象科学》2019,39(1):104-116

本文对苏州地区2015年12月13—15日发生的一次典型的重霾污染天气过程进行了数值模拟,分析了颗粒物及其组分的时空变化特征及其气象影响因子,以期为该区域空气污染治理和预防提供科学依据。结果表明:(1)利用WRF-Chem模式对此次重霾污染天气过程的污染气体成分进行数值模拟后发现,小时平均的PM_(2.5)、PM_(10)、CO、SO_2、NO_2模拟值与实测值的相关系数较高,达到0.68以上,通过了P0.01的显著性检验,且日变化过程对应也较好。(2)通过分析此次污染过程的天气背景,发现污染形成期高空环流比较平直,中层为均匀的弱高压控制,地面受弱高压脊控制,这种形势容易导致颗粒物的堆积。后期地面等压线密集时,风速大,有利于污染物的输送与扩散。(3)通过分析此次污染过程期间气象要素的变化发现,有逆温、风速小、相对湿度大等不利的气象条件是导致此次污染过程发生的重要原因之一。(4)HYSPLIT轨迹分析显示,此次重霾过程主要受北方大范围灰霾颗粒物南下影响,北方污染气团逐步南推,14至15日本地大气扩散条件差、污染物累积,最终导致本地污染加重,从而发生重霾事件。(5)火点图的分布进一步验证了此次重霾污染过程是由外来污染气团输入所导致。  相似文献   

近50多年来淮河流域气候水分盈亏时空变化   总被引：1，自引：0，他引：1  

颜雅琼  申双和 《气象科学》2019,39(4):457-466

水分盈亏是区域干湿气候划分的重要依据。基于淮河流域63个气象台站1957—2014年逐日观测数据,运用累积距平、Mann-Kendall突变分析、Morlet小波分析及ArcGIS反权重空间插值法,结合Penman-Monteith蒸散计算模型获得淮河流域水分盈亏量的周期特征、突变特征及其时空分布特征,并分析其主要影响因子。结果表明:(1)水分盈亏月变化基本符合5月最低,7月最高。(2)从季节分布来看,水分亏缺面积秋季春季冬季夏季,亏缺程度春季最强。从平均年水分盈亏量分布来看,水分盈亏量由南向北递减。且不论季节还是年状况,山地及河流对区域水分盈亏量的南北递减存在滞后作用。(3)从各因子气候倾向率的时空分布来看,江苏东南部、山东西部、河南大部、湖北中部水分盈亏量变化的主导因子为潜在蒸散量,其他区域的主导因子为降雨量。(4)淮河流域水分盈亏量存在周期特征,第一主周期为10 a。  相似文献   

大涡技术对模拟台风眼墙替换过程的影响          下载免费PDF全文

陈小宇  吴立广  李煜斌 《大气科学学报》2019,42(2):161-173

眼墙替换是影响台风强度和内核结构的一种重要过程。本研究在高分辨率的数值理想试验中加入大涡模拟技术,对比分析大涡模拟对眼墙替换过程的影响。结果表明:大涡模拟的加入使得模拟台风的强度和边界层入流增强。整个眼墙替换过程共用时约20～22 h,但大涡模拟试验中外眼墙形成更迅速,同时强度和上升运动偏弱。外眼墙完全取代内眼墙之后的台风强度超过替换过程之前的强度。此外,使用大涡技术可以更好地模拟出眼墙替换过程中内外眼墙之间的moat区下沉运动,结构特征与前人观测中所发现的结构特征一致。因此,在台风数值研究中引入大涡模拟技术,有助于更好地模拟眼墙替换过程中的台风结构特征和变化。  相似文献   

Synoptic analysis of sea level pressure patterns and Vertically Integrated Moisture Flux Convergence VIMFC during the occurrence of durable and pervasive rainfall in Iran     

《Dynamics of Atmospheres and Oceans》2019

To carry out this research, interpolated data of daily rainfall from Iran’s Asfazari data base during 1/1/1979–31/12/2013 is used. The day along with pervasive rainfall considered a day that at least 50% of Iran’s territory has received more than 1 mm for at least two consecutive days. Based on mentioned thresholds, 224 days selected for statistical analysis. The sea level pressure data, zonal and meridional wind components and specific humidity with spatial resolution of 0.25*0.25 Gaussian degree in spatial domain of 10 °N to 60 °N and 15 °E to 75 °E obtained from the European Center for Medium range Weather Forecasting (ECMWF) ERA-Interim for selected days. Then on the data matrix of sea level pressure, the cluster analysis by Ward linkage method done and 4 sea level pressure patterns with different configuration of synoptic systems were identified. The findings showed that in the sea level, the interaction between southern thermal low pressure systems (Arabia low pressure) with Europe and Siberia cold immigrant high pressure both by individual and integration and anticyclone circulation of Arab sea from the low level of 1000–500 hPa of troposphere have the most role on occurrence of durable and pervasive rainfall of Iran. The most Vertically Integrated Moisture Flux Convergence in the first layer of troposphere (1000–850 hPa) observed in low height regions, in the second layer of troposphere (775–700 hPa) on Zagros Mountains and in third layer of troposphere (600–500 hPa) is seen in mountains leeward of Iran. Also the results showed that the maximum rainfall cores has the most coordination with Vertically Integrated Moisture Flux Convergence (VIMFC) in the second layer of troposphere (775–700 hPa) on the Zagros heights in the southwest of Iran.  相似文献   

Interdecadal variability of the mega-ENSO–NAO synchronization in winter     

Zhiwei Wu  Peng Zhang 《Climate Dynamics》2015,45(3-4):1117-1128

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基于GridMet模型的浙江省温湿指数空间分布及地形影响分析     

施国萍  何永健  张眉  邱新法  曾燕 《地球信息科学学报》2019,21(12):1923-1933

温湿指数是气候舒适度评价模型之一,通过温度与湿度的组合反映人体与周围环境的热量交换,本文利用2003-2018年浙江省及其周边71个气象站点月平均气温、地面水汽压数据,以及MODIS水汽产品,基于GridMet模型模拟了浙江省各月温湿指数空间分布（100 m×100 m）,分析了浙江省温湿指数随地形因子（海拔、坡度、坡向）变化的特征;讨论了各地形因子对温湿指数空间分布的影响程度。结果表明：① 海拔、坡度、坡向3个地形因子中,1月温湿指数随坡向的变化最大,7月最小;② 同坡向上,坡度变化对1月温湿指数影响较大,而海拔变化则是对7月影响最大;③ 南坡1月温湿指数随海拔和坡度增加均略为增加,南坡其他月份及北坡各月均为随海拔和坡度增加温湿指数减小;④ 北坡相对于南坡而言,海拔和坡度对温湿指数的影响更为明显。浙江大部分山区由于地形影响,夏季较为“舒适”,适宜建立避暑消夏的旅游项目。  相似文献   

Solar cycle distribution of strong solar proton events and the related solar-terrestrial phenomena   总被引：1，自引：0，他引：1  

Guiming Le  Xingxing Yang  Liuguang Ding  Yonghua Liu  Yangping Lu  Minhao Chen 《Astrophysics and Space Science》2014,352(2):403-408

We investigated the solar cycle distribution of strong solar proton events (SPEs, peak flux ≥1000 pfu) and the solar-terrestrial phenomena associated with the strong SPEs during solar cycles 21–23. The results show that 37 strong SPEs were registered over this period of time, where 20 strong SPEs were originated from the super active regions (SARs) and 28 strong SPEs were accompanied by the X-class flares. Most strong SPEs were not associated with the ground level enhancement (GLE) event. Most strong SPEs occurred in the descending phases of the solar cycles. The weaker the solar cycle, the higher the proportion of strong SPES occurred in the descending phase of the cycle. The number of the strong SPEs that occurred within a solar cycle is poorly associated with the solar cycle size. The intensity of the SPEs is highly dependent of the location of their source regions, with the super SPEs (≥20000 pfu) distributed around solar disk center. A super SPE was always accompanied by a fast shock driven by the associated coronal mass ejection and a great geomagnetic storm. The source location of strongest GLE event is distributed in the well-connected region. The SPEs associated with super GLE events (peak increase rate ≥100%) which have their peak flux much lower than 10000 pfu were not accompanied by an intense geomagnetic storm.  相似文献   

Early stage of critical clusters growth in phenomenological and molecular dynamics simulation models     

《Atmospheric Research》2007,83(3-4):465-480

The growth of critical clusters is discussed in the paper according to the classical and molecular dynamics (MD) approaches. A new formula for molecule numbers in critical clusters has been derived within the framework of the classical approach. A set of equations controlling the early stage of growth in a neighborhood of a critical size is presented. As far as molecular dynamics simulation is concerned, a computational technique based on the DL_POLY code is described in brief. Computation results are presented concerning cluster formation of H₂O vapor, distribution of clusters versus time, cluster growth and radial density distribution of isolated clusters. A comparison with the classical results is made for a case of dense vapor, where the mechanism of strong condensation is predominant. The Hertz–Knudsen formula seems to be verified by the molecular dynamics results.  相似文献