降水现象对大气消光系数和能见度的影响   总被引：8，自引：2，他引：6       下载免费PDF全文

刘西川  高太长  刘磊  张伟  杨树臣  李涛 《应用气象学报》2010,21(4):433-441

大气中各种粒子对大气消光系数和能见度有不同程度影响,除气溶胶粒子外,降水粒子对能见度影响也不可忽视。为了解降水粒子对能见度的影响,确定能见度变化与降水现象之间的关系,该文在分析降水粒子的大小、速度、形状、谱分布、光学特性等特征的基础上,忽略气溶胶粒子的影响,建立基于实测谱分布的降水与能见度的理论模型,讨论不同类型降雨、降雪对大气消光系数和能见度的影响。同时选取Parsivel降水粒子谱仪在南京地区的降雨和降雪观测记录,利用实测数据来对比验证本文所建立的降水-能见度理论模型。结果表明:能见度随着降水强度的增大呈指数降低;受降水粒子特性和天气条件等多种因素影响,能见度与降水强度之间的关系并不是唯一对应的;降雨和降雪对能见度的影响各不相同,相比而言,降雨对能见度的影响比较容易确定,而降雪对能见度的影响比较复杂,主要因为雪花或冰晶的类型复杂多变,对大气消光系数有不同程度的影响。结合理论分析和实测数据对比验证,降水现象对能见度的影响得到了证实。  相似文献   

Multi-Source Emission Determination Using an Inverse-Dispersion Technique     

Thomas K. Flesch  Lowry A. Harper  Raymond L. Desjardins  Zhiling Gao  Brian P. Crenna 《Boundary-Layer Meteorology》2009,132(1):11-30

Inverse-dispersion calculations can be used to infer atmospheric emission rates through a combination of downwind gas concentrations and dispersion model predictions. With multiple concentration sensors downwind of a compound source (whose component positions are known) it is possible to calculate the component emissions. With this in mind, a field experiment was conducted to examine the feasibility of such multi-source inferences, using four synthetic area sources and eight concentration sensors arranged in different configurations. Multi-source problems tend to be mathematically ill-conditioned, as expressed by the condition number κ. In our most successful configuration (average κ = 4.2) the total emissions from all sources were deduced to within 10% on average, while component emissions were deduced to within 50%. In our least successful configuration (average κ = 91) the total emissions were calculated to within only 50%, and component calculations were highly inaccurate. Our study indicates that the most accurate multi-source inferences will occur if each sensor is influenced by only a single source. A “progressive” layout is the next best: one sensor is positioned to “see” only one source, the next sensor is placed to see the first source and another, a third sensor is placed to see the previous two plus a third, and so on. When it is not possible to isolate any sources κ is large and the accuracy of a multi-source inference is doubtful.  相似文献   

激光雷达反演参数k值的研究   总被引：3，自引：2，他引：1  

张文煜  王音淇  宋嘉尧  张镭  孙璐 《高原气象》2008,27(5)

采用532 nm激光雷达2006年在兰州市不同天气状况下的观测数据,结合能见度因子、CE318太阳光度计观测数据,对利用Klett法求解时,k在不同天气状况下的取值进行了初步研究,结果表明:只有当0.7≤k≤1.0时,气溶胶消光系数的大小与能见度估算出的值相接近。但在k=0.7时,计算出的气溶胶消光系数正、负参半;k=1.0时,消光系数廓线在晴天无云的天气状况下同实际情况不符。通过进一步分析研究激光雷达和光度计的同期观测资料发现:k=0.8时,较合理的数据所占比例为100%,k=0.9为84%,k=1.0仅为12%。对兰州市区而言,利用激光雷达分析气溶胶光学特性时,取k=0.8或k=0.9较为合理。  相似文献   

一个半线性耦合抛物型方程组爆破解的速率估计     

范萍  李刚  黄瑜 《南京气象学院学报》2008,31(3):441-446

考虑一个方程和非线性边界条件耦合的半线性抛物型方程组,运用Scaling方法、Green函数、Schauder估计等方法,研究该方程组解的爆破速率,并给出非线性反应项和吸收项对爆破速率的影响。  相似文献   

Time-dependent simulations of steady C-type shocks     

S. Van Loo  I. Ashmore  P. Caselli  S. A. E. G. Falle  T. W. Hartquist 《Monthly notices of the Royal Astronomical Society》2009,395(1):319-327

Using a time-dependent multifluid, magnetohydrodynamic code, we calculated the structure of steady perpendicular and oblique C-type shocks in dusty plasmas. We included relevant processes to describe mass transfer between the different fluids, radiative cooling by emission lines and grain charging, and studied the effect of single- and multiple-sized grains on the shock structure. Our models are the first of oblique fast-mode molecular shocks in which such a rigorous treatment of the dust grain dynamics has been combined with a self-consistent calculation of the thermal and ionization structures including appropriate microphysics. At low densities, the grains do not play any significant rôle in the shock dynamics. At high densities, the ionization fraction is sufficiently low that dust grains are important charge and current carriers and, thus, determine the shock structure. We find that the magnetic field in the shock front has a significant rotation out of the initial upstream plane. This is most pronounced for single-sized grains and small angles of the shock normal with the magnetic field. Our results are similar to previous studies of steady C-type shocks showing that our method is efficient, rigorous and robust. Unlike the method employed in the previous most detailed treatment of dust in steady oblique fast-mode shocks, ours allow a reliable calculation even when chemical or other conditions deviate from local statistical equilibrium. We are also able to model transient phenomena.  相似文献   

The global gas and dust budget of the Large Magellanic Cloud: AGB stars and supernovae, and the impact on the ISM evolution     

M. Matsuura  M. J. Barlow  A. A. Zijlstra  P. A. Whitelock  M.-R. L. Cioni  M. A. T. Groenewegen  K. Volk  F. Kemper  T. Kodama  E. Lagadec  M. Meixner  G. C. Sloan  S. Srinivasan 《Monthly notices of the Royal Astronomical Society》2009,396(2):918-934

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Stellar sources of dust in the high-redshift Universe     

Rosa Valiante  Raffaella Schneider  Simone Bianchi  Anja C. Andersen 《Monthly notices of the Royal Astronomical Society》2009,397(3):1661-1671

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The escape of ionizing photons from supernova-dominated primordial galaxies     

Hidenobu Yajima  Masayuki Umemura  Masao Mori  Taishi Nakamoto 《Monthly notices of the Royal Astronomical Society》2009,398(2):715-721

In order to assess the contribution of Lyman break galaxies (LBGs) and Lyman α emitters (LAEs) at redshifts  3 < z < 7  to the ionization of intergalactic medium (IGM), we investigate the escape fractions of ionizing photons from supernova-dominated primordial galaxies by solving the three-dimensional (3D) radiative transfer. The model galaxy is employed from an ultra-high-resolution chemodynamic simulation of a primordial galaxy by Mori & Umemura, which well reproduces the observed properties of LAEs and LBGs. The total mass of model galaxy is  10¹¹ M_⊙  . We solve not only photoionization but also collisional ionization by shocks. In addition, according to the chemical enrichment, we incorporate the effect of dust extinction, taking the size distributions of dust into account. As a result, we find that dust extinction reduces the escape fractions by a factor of 1.5–8.5 in the LAE phase and by a factor of 2.5–11 in the LBG phase, while the collisional ionization by shocks increases the escape fractions by a factor of  ≈2  . The resultant escape fractions are 0.07–0.47 in the LAE phase and 0.06–0.17 in the LBG phase. These results are well concordant with the recent estimations derived from the flux density ratio at 1500 to 900 Å of LAEs and LBGs. Combining the resultant escape fractions with the luminosity functions of LAEs and LBGs, we find that high- z LAEs and LBGs can ionize the IGM at   z = 3–5  . However, ionizing radiation from LAEs as well as LBGs falls short of ionizing the IGM at   z > 6  . That implies that additional ionization sources may be required at   z > 6  .  相似文献   

广西来宾蓬莱滩二叠纪瓜德鲁普统—乐平统界线剖面元素和同位素地球化学研究及地质意义   总被引：4，自引：0，他引：4  

杨振宇  沈渭洲  郑连弟 《地质学报》2009,83(1):1-15

广西来宾蓬莱滩二叠系瓜德鲁普统-乐平统界线剖面已被国际地质科学联合会确定为国际界线层型标准剖面,在该界面附近发生了一次重要的全球性生物绝灭事件。蓬莱滩剖面样品采自乐平统合山组底部(由硅质岩和透镜状灰岩组成)和瓜德鲁普统茅口组上部来宾灰岩(由硅质灰岩、灰岩和少量硅质岩组成)。它们具有高的SiO2含量(除3个样品低于10%以外,其余样品均大于17%,平均为43.44%)、m值(>50)与Sr/Ba值(>1.0)和低的MgO/CaO(绝大部分低于02)与 V/(V+Ni)值(<046); Ce和Eu亏损明显。这些地球化学特征反映它们是在相对氧化的浅海环境中形成的,硅的来源非常丰富。样品的εNd(t)值(-7.5~-3.3)和(87Sr/86Sr)i值(0.70705~0.70739)都位于全球大洋Nd、Sr同位素演化曲线晚二叠纪时期区域内。有机碳的δ13Corg值变化明显(-26.7‰~-23.2‰),尤其是在瓜德鲁普统与乐平统以及茅口组与合山组界线附近发生显著的负漂移(达34‰),而且与无机碳的δ13C值呈现大致平行的变化趋势,证实在该界线附近发生过生物绝灭事件。虽然对瓜德鲁普统—乐平统交替时期发生的生物绝灭事件已提出过包括海平面下降在内的多种假设,但本文认为,由地幔柱上升引起的、以峨嵋山玄武岩喷发为代表的超级火山活动以及由此引起的环境效应是该时期生物绝灭的主要原因。  相似文献   

Dust extinction and X-ray emission from the starburst galaxy NGC 1482     

N.D. Vagshette  M.B. Pandge  S.K. PandeyM.K. Patil 《New Astronomy》2012,17(5):524-532

We present the results based on multiwavelength imaging observations of the prominent dust lane starburst galaxy NGC 1482 aimed to investigate the extinction properties of dust existing in the extreme environment. (B-V) colour-index map derived for the starburst galaxy NGC 1482 confirms two prominent dust lanes running along its optical major axis and are found to extend up to ∼11 kpc. In addition to the main lanes, several filamentary structures of dust originating from the central starburst are also evident. Though, the dust is surrounded by exotic environment, the average extinction curve derived for this target galaxy is compatible with the Galactic curve, with R_V = 3.05, and imply that the dust grains responsible for the optical extinction in the target galaxy are not really different than the canonical grains in the Milky Way. Our estimate of total dust content of NGC 1482 assuming screening effect of dust is ∼2.7 × 10⁵ M_⊙, and provide lower limit due to the fact that our method is not sensitive to the intermix component of dust. Comparison of the observed dust in the galaxy with that supplied by the SNe to the ISM, imply that this supply is not sufficient to account for the observed dust and hence point towards the origin of dust in this galaxy through a merger like event.Our multiband imaging analysis reveals a qualitative physical correspondence between the morphologies of the dust and Hα emission lines as well as diffuse X-ray emission in this galaxy. Spatially resolved spectral analysis of the hot gas along outflows exhibit a gradient in the temperature. Similar gradient was also noticed in the measured values of metallicity, indicating that the gas in the halo is not yet enriched. High resolution, 2-8 keV Chandra image reveals a pair of point sources in the nuclear region with their luminosities equal to 2.27 × 10³⁹ erg s⁻¹ and 9.34 × 10³⁹ erg s⁻¹, and are in excess of the Eddington-limit of 1.5 M_⊙ accreting source. Spectral analysis of these sources exhibit an absorbed-power law with the hydrogen column density higher than that derived from the optical measurements.  相似文献