首页 | 本学科首页   官方微博 | 高级检索  
相似文献
 共查询到20条相似文献,搜索用时 171 毫秒
1.
金燕  黄意玢  王维和 《气象》1992,18(8):13-15
本文用LOWTRAN 6程序计算了5.7—7.1μm和6.5—7.6μm两个水汽通道的透过率、射出辐射及权重函数,并将两者加以比较,探讨降低水汽通道探测高度的可能性。  相似文献   

2.
地球大气透过率及辐射率计算   总被引:13,自引:3,他引:10       下载免费PDF全文
吴晓 《应用气象学报》1998,9(1):124-128
文章介绍了一种比较简单实用的地球大气的光谱透过率和到达大气层顶的红外辐射率的计算模型,光谱波长从4 μm到∞ μm,吸收气体H2O、CO2、O3的吸收计算采用Elsasser带模式及其经验参数,H2O的连续吸收公式是美国LOWTRAN-6计算程序的水汽连续吸收经验公式。透过率的计算结果与LOWTRAN计算结果相一致。以这种透过率简化模型为基础,建立了辐射传递正演计算模型,开发了相应软件,并用于卫星遥感射出长波辐射的资料处理中,取得了良好结果。  相似文献   

3.
静止气象卫星水汽通道位置的选择   总被引:1,自引:1,他引:1       下载免费PDF全文
对静止气象卫星上6.3μm 附近水汽通道位置的选取进行了初步研究。并在4.8μm 至8.5μm 区间分26个通道用 LOWTRAN6等一组程序计算了通道透过率、辐射亮度及权函数。所选的通道对较低高度的水汽有较好的感应能力。  相似文献   

4.
黄意玢  金燕 《气象》1991,17(2):55-57
LOWTRAN 6是计算地球大气透过率和本底辐射的程序。本文简单介绍了该程序的基本假定、功能和结构。  相似文献   

5.
大气对NOAA通道辐射透过率的影响研究   总被引:2,自引:2,他引:2       下载免费PDF全文
本文利用LOWTRAN7大气辐射计算模式,对NOAA三个通道分别选取不同的模式大气进行计算,得到了各种模式大气的大气透过率。详细计算了探测路径上卷云、不同气溶胶模式、大气温度、水汽含量变化等气象要素及大气成分的变化对大气透过率的影响,得出一些有意义的结论。  相似文献   

6.
LOWTRAN6在微机上的初步应用   总被引:2,自引:0,他引:2  
LOWTRAN 6是计算大气透过率及本底辐射的 Fortran 语言程序。本文简要介绍了该程序的基本假设、功能和结构,重点讨论了移植到386档微机(32位字长)上应用的初步情况。  相似文献   

7.
从红外太阳透过率反演大气可降水量的研究   总被引:6,自引:0,他引:6  
从红外波段太阳透过率测量中可以反演大气可降水量#AW#a。我们在近、中红外波段选取了三对波长,用LOWTRAN 7辐射传输模式,主要研究了散射和气溶胶对这三对波长反演#AW#a算式的影响。结果表明,通常采用近红外波长对(即0.9422~0.862 μm)反演#AW#a并非最佳选择,因为其反演算式受到大气状态(混浊度)的很大影响;而在稍远段两对波长(1.47~1.55 μm和3.704~3.067 μm)对应的算式较为稳定。  相似文献   

8.
孙囡  陈逸伦  傅云飞 《气象学报》2019,77(3):563-578
辐射平衡是气候决定性因素之一, 温湿廓线对辐射计算有重要影响。利用中国东部地区1960—2008年74个探空站资料, 将SBDART(Santa Barbara DISORT Atmospheric Radiative Transfer)辐射传输模式自带的大气温湿廓线和探空测得的实际大气温湿廓线进行对比, 并代入SBDART模式中, 分别计算晴空条件下不同温湿廓线对辐射通量的影响。结果表明:(1)中国东部地区的大气温湿廓线有明显的区域和季节特点;(2)模式地面向下辐射通量与实际相比有较明显差异, 尤其是在东北地区的冬季、中东部地区的夏季和华南地区的冬季, 差值达20—35 W/m2, 相对误差达2.01%—3.18%;(3)在东北地区的冬季、中东部地区的冬季以及华南地区的夏、冬季, 模式计算的大气顶向上辐射通量与实际相比差值达10—22 W/m2, 相对误差可达3.67%—8.94%;(4)模式与实际辐射加热率的差值在0.03—0.29 K/d。研究表明, 模式自带的大气温湿廓线区域和季节划分并不够细致, 不足以代表中国东部地区各个区域及季节的温湿特点。建立一套中国东部地区的大气标准廓线可以为辐射模拟提供更准确的输入量。   相似文献   

9.
太阳辐射计探测晴空水汽总量方法研究   总被引:3,自引:0,他引:3  
朱晓苏  周军 《大气科学》1998,22(1):39-45
本文给出使用多波长太阳辐射计在0.94 μm水汽弱吸收带测量太阳透射辐射得出大气垂程水汽含量的方法。使用LOWTRAN 7建立仪器0.94 μm的水汽吸收带平均透过率表达式。提出了用两个相邻波长通道的线性近似消除气溶胶和瑞利散射的影响。对太阳辐射计与气象探空仪探测大气垂程水汽量的实验结果做了比较。  相似文献   

10.
根据世界民航组织和世界气象组织有关专家对当前亚音速飞机排放量的估计和将来20年内增长的预测,用辐射传输模式估算了飞机排放物对地面紫外辐射水平的影响。计算使用DISORT程序,这是一个经过检验可以较好地包括多次散射作用的离散坐标法程序。分别检验了飞机排放煤烟、硫酸盐粒子和卷云的多次散射及引起的臭氧增加对地面280~400 nm紫外辐射的影响。结果表明:根据目前的估计和预测,飞机排放的煤烟和硫酸盐粒子对地面紫外辐射没有影响;引起的臭氧变化也不至于引起地面紫外辐射的变化。但如果天空存在一层卷云(光学厚度0.042),就足以使得地面直射紫外辐射减少5%,总紫外辐射增加1%~2%。有资料表明,飞机排放的水汽可能使得某些地区卷云量增加了10%。因此,可能会对地面紫外辐射产生影响。  相似文献   

11.
The absorption properties of the water vapor continuum and a number of weak bands for H2O, O2, CO2, CO, N2O, CH4, and O3 in the solar spectrum are incorporated into the Fu-Liou radiation parameterization program by using the correlated k-distribution method (CKD) for the sorting of absorption lines. The overlap absorption of the H2O lines and the H2O continuum (2500-14500 cm^-1) are treated by taking the two gases as a single-mixture gas in transmittance calculations. Furthermore, in order to optimize the computation efforts, CO2 and CH4 in the spectral region 2850-5250 cm^-1 are taken as a new singlemixture gas as well. For overlap involving other absorption lines in the Fu-Liou spectral bands, the authors adopt the multiplication rule for transmittance computations under which the absorption spectra for two gases are assumed to be uncorrelated. Compared to the line-by-line (LBL) computation, it is shown that the errors in fluxes introduced by these two approaches within the context of the CKD method are small and less than 0.48% for the H20 line and continuum in the 2500-14500 cm^-1 solar spectral region, -1% for H2O (line) H2O (continuum) CO2 CH4 in the spectral region 2850-5250 cm^-1, and -1.5% for H2O (line) H2O (continuum) O2 in the 7700-14500 cm^-1 spectral region. Analysis also demonstrates that the multiplication rule over a spectral interval as wide as 6800 cm^-1 can produce acceptable errors with a maximum percentage value of about 2% in reference to the LBL calculation. Addition of the preceding gases increases the absorption of solar radiation under all sky conditions. For clear sky, the increase in instantaneous solar absorption is about 9%-13% (-12 W m^-2) among which the H20 continuum produces the largest increase, while the contributions from O2 and CO2 rank second and third, respectively. In cloudy sky, the addition of absorption amounts to about 6-9 W m^-2. The new, improved program with the incorporation of the preceding gases produces a smaller solar absorption in clouds due to the reduced solar flux reaching the cloud top.  相似文献   

12.
The absorption properties of the water vapor continuum and a number of weak bands for H2O, O2, CO2, CO, N2O, CH4, and O3 in the solar spectrum are incorporated into the Fu-Liou radiation parameterization program by using the correlated k-distribution method (CKD) for the sorting of absorption lines. The overlap absorption of the H2O lines and the H2O continuum (2500-14500 cm-1) are treated by taking the two gases as a single-mixture gas in transmittance calculations. Furthermore, in order to optimize the computation efforts, CO2 and CH4 in the spectral region 2850-5250 cm-1 are taken as a new single-mixture gas as well. For overlap involving other absorption lines in the Fu-Liou spectral bands, the authors adopt the multiplication rule for transmittance computations under which the absorption spectra for two gases are assumed to be uncorrelated. Compared to the line-by-line (LBL) computation, it is shown that the errors in fluxes introduced by these two approaches within the context of the CKD method are small and less than 0.48% for the H2O line and continuum in the 2500-14500 cm-1 solar spectral region, -1% for H2O (line) H2O (continuum) CO2 CH4 in the spectral region 2850-5250 cm-1, and -1.5% for H2O (line) H2O (continuum) O2 in the 7700-14500 cm-1 spectral region. Analysis also demonstrates that the multiplication rule over a spectral interval as wide as 6800 cm-1 can produce acceptable errors with a maximum percentage value of about 2% in reference to the LBL calculation. Addition of the preceding gases increases the absorption of solar radiation under all sky conditions. For clear sky, the increase in instantaneous solar absorption is about 9%-13% (~12 W m~2) among which the H2O continuum produces the largest increase, while the contributions from O2 and CO2 rank second and third, respectively. In cloudy sky, the addition of absorption amounts to about 6-9 W m-2. The new, improved program with the incorporation of the preceding gases produces a smaller solar absorption in clouds due to the reduced solar flux reaching the cloud top.  相似文献   

13.
The first measurements of cloud condensation nuclei(CCN) at five supersaturations were carried out onboard the research vessel "Sagar Kanya"(cruise SK-296) from the south to the head-bay of the Bay of Bengal as part of the Continental Tropical Convergence Zone(CTCZ) Project during the Indian summer monsoon of 2012. In this paper, we assess the diurnal variation in CCN distributions at supersaturations from 0.2% to 1%(in steps of 0.2%) and the power-law fit at supersaturation of 1%.The diurnal pattern shows peaks in CCN concentration(NCCN) at supersaturations from 0.2% to 1% between 0600 and 0700 LST(local standard time, UTC+0530), with relatively low concentrations between 1200 and 1400 LST, followed by a peak at around 1800 LST. The power-law fit for the CCN distribution at different supersaturation levels relates the empirical exponent(k) of supersaturation(%) and the NCCNat a supersaturation of 1%. The NCCNat a supersaturation of 0.4% is observed to vary from 702 cm~(-3) to 1289 cm~(-3), with a mean of 961 ± 161 cm~(-3)(95% confidence interval), representing the CCN activity of marine air masses. Whereas, the mean NCCNof 1628 ± 193 cm~(-3) at a supersaturation of 1% is higher than anticipated for the marine background. When the number of CCN spectra is 1293, the value of k is 0.57 ± 0.03(99% confidence interval)and its probability distribution shows cumulative counts significant at k ≈ 0.55 ± 0.25. The results are found to be better at representing the features of the marine environment(103 cm~(-3) and k ≈ 0.5) and useful for validating CCN closure studies for Indian sea regions.  相似文献   

14.
Vertical profiles of aerosol were measured in February 1993, and January - March 1995 using balloon-borne particle counters released from Kiruna, Sweden. Condensation nuclei (CN) and aerosol with radii 0.15 - 10.0 µm were measured in 8-12 size classes. The three flights in 1993 were within the polar vortex. Temperatures were below polar stratospheric cloud (PSC) threshold temperatures on one flight and a thin PSC was observed. The volcanic aerosol in the 1993 vortex was similar to that in 1992. In 1993, surface areas were 10 - 20 µm2 cm-3 and volumes 1 - 3 µm3 cm-3. In 1995 three of five flights were within the polar vortex. The volcanic aerosol had decreased to 3 - 7 µm2 cm-3 and 0.1 - 0.4 µm3 cm-3. The top of the volcanic aerosol layer in both years was near 500 K potential temperature (~20 km). A thick nitric acid and water PSC was observed in January 1995. In the thickest region of this PSC nearly all CN were observed to be activated, and surface areas of 5 - 10 µm2 cm-3 were calculated. The volumes observed in this PSC were closer to what would be expected for particles composed of nitric acid trihydrate than for ternary solution droplets. In 1993 the opposite was observed, the volumes in the thin PSC were closer to what would be expected for ternary solution droplets.  相似文献   

15.
The longwave (0-2380 cm-1) cooling rate due to water vapor in the troposphere and the stratosphere has been calculated by a new infrared transmission model in this paper. An exact scheme is used for treating the integration over wavenumber and the inhomogeneous path in the atmosphere. It is shown that the atmospheric window region (730-1200 cm-1) (mainly water vapor continuum) plays an important role in the total cooling near the surface, about 72% of the total cooling lying in this region at the height of 1 km; the CG approximation used for an inhomogeneous path is fairly applicable for calculating the cooling rate due to water vapor, with a maximum error of 0.16 K/day throughout the troposhere and the stratosphere; on the other hand, the error due to the diffusivity factor of 1.66 appears to be slightly larger near the surface. In this study, the influences on the calculation of above infrared cooling rate, of the temperature-dependence of the absorption coefficients of water vapor, the upper level cutoff and the integration step for altitude, and the substitution of the quasi-grey approximation for the exact integration over wavenumber, are also examined.  相似文献   

16.
利用2009年5月8日多普勒雷达资料和飞机穿云观测资料,综合分析了西风槽影响下山西省一次积层混合云的形成过程和微物理结构。结果表明,此次飞机探测到的积层混合云是由对流单体多次并合形成的带状对流云团减弱后形成的,云中嵌有明显的对流泡,最大强度为45~50dBZ,最大垂直尺度在6km左右。CDP(cloud droplet probe,前向散射粒子谱探头)、CIP(cloud ima-ging probe,二维灰度云粒子探头)、PIP(precipitation imaging probe,二维灰度降水粒子探头)测量的平均数浓度变化范围分别是132.4~220.2cm-3、1.54×10-1~6.28×100cm-3、9.09×10-4~7.34×10-3cm-3。二维图像表明,冷层中的固态粒子主要是形状不规则的霰粒子,说明过冷水供应充足;在-7℃左右观测到柱状聚合体和凇附程度不同的冰雪晶粒子,表明柱状冰晶通过凝华形成后,碰并和凇附是其增长为霰粒子的重要机制。不同高度的CDP平均谱(2~50μm)存在一定的差异,因低层水汽凝结作用较强,2~18μm的云粒子数浓度基本随高度的增加而降低;因暖层中碰并效率低和冷层中小冰晶浓度随高度增加,24~35μm粒子数浓度随高度增加而增大。CIP平均谱(25~1550μm),除4100m为双峰谱外,其他高度均为单峰谱。PIP平均谱(100~6200μm),4450m高度处的粒子谱宽和数浓度最大,3200~4000μm之间出现大值区域,表明对流单体及周边区域为较大固态降水粒子的形成提供了良好的环境。  相似文献   

17.
A coupled meteorology and aerosol/chemistry model WRF-Chem(Weather Research and Forecast model coupled with Chemistry) was used to conduct a pair of simulations with present-day(PD) and preindustrial(PI) emissions over East Asia to examine the aerosol indirect effect on clouds.As a result of an increase in aerosols in January,the cloud droplet number increased by 650 cm-3 over the ocean and East China,400 cm-3 over Central and Southwest China,and less than 200 cm-3 over North China.The cloud liquid water path(LWP) increased by 40-60 g m-2 over the ocean and Southeast China and 30 g m-2 over Central China;the LWP increased less than 5 g m-2 or decreased by 5 g m-2 over North China.The effective radius(Re) decreased by more than 4 μm over Southwest,Central,and Southeast China and 2μm over North China.In July,variations in cloud properties were more uniform;the cloud droplet number increased by approximately 250-400 cm-3,the LWP increased by approximately 30-50 g m-2,and Re decreased by approximately 3 ?m over most regions of China.In response to cloud property changes from PI to PD,shortwave(SW) cloud radiative forcing strengthened by 30 W m-2 over the ocean and 10 W m-2 over Southeast China,and it weakened slightly by approximately 2-10 W m-2 over Central and Southwest China in January.In July,SW cloud radiative forcing strengthened by 15 W m-2 over Southeast and North China and weakened by 10 W m-2 over Central China.The different responses of SW cloud radiative forcing in different regions was related to cloud feedbacks and natural variability.  相似文献   

18.
辽宁北部典型流域水生态功能区水生态安全评价   总被引:1,自引:0,他引:1  
基于流域水生态功能分区的水生态安全评价是指导流域水生态“分类、分区”综合管理的前提,本文在流域中小尺度上依据水生态空间格局分异的自然特征和社会属性,以辽河流域的清河和凡河支流为对象,在流域水生态功能三级分区的基础上,运用“压力-状态-响应模型”(PSR),通过对流域社会经济压力指标、环境压力指标、城市发展指标、资源环境发展指标、投资指标、治理指标等因素分析,筛选出13个评价指标。利用生态安全综合指数法,将流域水生态安全划分为极不安全、不安全、基本安全、安全、非常安全五个级别。其中,清河流域Ⅳ-5-9、Ⅳ-5-10、Ⅳ-5-11、Ⅳ-5-12、Ⅳ-5-14区处于基本安全,Ⅳ-5-8、Ⅳ-5-13属于不安全;凡河流域4个水生态功能三级区中,Ⅳ-5-1、Ⅳ-5-2、Ⅳ-5-3区属于基本安全、Ⅳ-5-4区为较安全。基于水生态功能分区的水生态安全评价和级别划分可为辽河流域水生态保护与流域生态管理提供科学依据。  相似文献   

19.
利用2009年石家庄地区的4次机载PMS探测资料,对不同天气条件下大气气溶胶的数浓度、平均直径垂直分布和谱分布及一次晴天条件下的水平分布进行分析。结果表明:PCASP 探头探测的0.1-3.0 μm气溶胶粒子最大数浓度的量级为102-104 cm-3之间,平均值量级为102-103 cm-3之间,平均直径最大值介于0.225-0.717 μm,平均值介于0.148-0.167 μm。晴天条件下,气溶胶的数浓度随高度递减,直径随高度变化不大;逆温层底气溶胶明显积累,气溶胶浓度在大气边界层内明显高于其他层次;阴天轻雾情况下边界层内的气溶胶数浓度大于雨天和晴天,雨天气溶胶浓度最低;晴天气溶胶数浓度的水平分布不均匀;在云中气溶胶浓度明显下降,在云外气溶胶浓度较高。不同天气条件和晴天不同高度情况下,石家庄地区气溶胶谱型呈单峰分布,小于0.3 μm的细粒子对气溶胶的数浓度贡献最大,且随着高度的增加谱宽变窄。  相似文献   

20.
A new remote sensing method is described to determine the vertical distribution and total content of atmospheric ozone. The method combines surface infrared, satellite infrared and ultraviolet channels. The width of the infrared channels is 0.01 cm-1, less than Lorentz half-width at the earth’s surface, rather than the present width, because these channels can obtain information about variations in the ozone profile below the profile main-peak. The numerical experiments show that the method has a satisfactory precision in determining total ozone content, just about 1 percent error, and vertical distribution from the earth to 65 km space. In addition, some semi-analysis functions for calculating backscattered ultraviolet and a relaxation equation are described in this paper.  相似文献   

设为首页 | 免责声明 | 关于勤云 | 加入收藏

Copyright©北京勤云科技发展有限公司  京ICP备09084417号