共查询到20条相似文献，搜索用时 109 毫秒
1.
An algorithm for remote sensing of water color from space 总被引：3，自引：0，他引：3
The ocean color algorithm proposed in this paper takes into account the effects of Rayleigh and aerosol scattering. The inherent reflectance and the diffuse transmittance of the Rayleigh atmosphere are expressed as functions of optical thickness and satellite measurement geometry with the aid of simple and accurate formulas. In the case of a turbid atmosphere, from which the aerosol optical thickness is unknown, the aerosol contribution is estimated with the aid of a measurement in a channel where the ocean is a blackbody (in the red or near infrared). If the relationship between the ocean color and the chlorophyll-like pigment concentration is assumed to be known at sea level, it is shown that the chlorophyll-like pigment concentration at an open ocean site can be determined from space to within a factor of 1.5 to 3 (uncertainty equal to 0.2 to 0.5 log interval), depending on the atmospheric turbidity. 相似文献
2.
发展了一个计算非均一大气条件下太阳辐射通量的一个简单而又精确的模式，其中包括关于大气球反射率与透过率的一个参数化表达式，并引入加权一次散射反照率和加权不对称因子，用于拟合非均一大气条件下计算辐射通量的四个经验订正因子。对清洁和浑浊的两类大气，都具有120060组的辐射通量模拟试验，以检验本模式的精度。这些模拟试验覆盖0－50的云光学厚度、0－0．8地表反射率、Junge和对数正态的气溶胶谱分布、－0．05气溶胶折射率虚部。在均一大气条件下，由本模式计算的120060组向上通量的标准差对清洁和浑浊两类大气分别为1．08％和1．04％；而向下通量的标准差分别为4.12%和3．31％。在非均一大气条件下，由本模式计算的向上通量的标准差对清洁和浑浊两类大气分别为3．01％和3．48％；而向下通量的标准差分别为4．54％和4．89％，其精度远优于均一假设下的计算结果。 相似文献
3.
Qiu Jinhuan 《大气科学进展》2002,19(3):433-447
A simple yet more accurate semiempirical model is developed to calculate solar radiative flux in the optically inhomogeneous atmosphere. In the model a parameterized expression of spherical reflectance and transmitance of the atmosphere is confirmed, and the weighted single scatter albedo and weighted asymmetric factor are introduced to fit four empirical correction factors responsible for radiative fluxes in the inhomogeneous atmosphere. For both clean and turbid models, there are 120060 sets of radiative flux simulations for accuracy checks of the model, which cover 0-50 cloud optical depths, 0-0.8 surface reflectance, Junge and Log-normal aerosol size distributions, and 0-0.05 imaginary parts of aerosol refractive indexes. In case of the homogeneous atmosphere, standard errors of the 120060 upward fluxes from the present model are 1.08% and 1.04% for clean and turbid aerosol models, respectively; and those of the downward fluxes are 4.12% and 3.31%. In case of the inhomogeneous atmosphere, standard errors of the upw ard fluxes from the present model are 3.01% and 3.48% for clean and turbid aerosol models.respectively; and those of the downward fluxes are 4.54% and 4.89%, showing a much better accuracy than the results calculated by using an assumption of the homogeneous atmosphere. 相似文献
4.
1999年6月28日~7月19日在敦煌场, 7月25日~7月31日在青海湖水面场进行了一次大规模综合野外测量试验, 其中采用3台先进的法国CIMEL太阳辐射计对两个场地大气光学特性进行了系统全面测量, 获得大量晴空天气条件下的大气光学数据。利用Langley法处理气溶胶通道数据得到气溶胶光学厚度及其光谱变化。测量结果显示550 nm波长平均气溶胶光学厚度分别为0.12、0.18, 由气溶胶光学厚度的波长变化得到气溶胶Junge参数分别为2.6、3.0, 并与几种典型气溶胶类型比较。结果表明两地在晴空天气里, 气溶胶含量较小, 符合遥感卫星传感器辐射定标的大气条件。 相似文献
5.
当气溶胶谱满足Junge分布时,Angstrom指数 (α) 可以准确地描述粒子大小,但真实大气气溶胶很少完全满足这一条件,仅用α判断粒子大小会有较大出入。基于北京、香河、兴隆、太湖4个Aeronet观测站21世纪以来各站历时都超过1年的气溶胶光学厚度资料,获得5511组lnτ与lnλ的二次拟合参数a2,a1,尝试找到一种结合α,a2,a1判断粒子大小的方法。结果表明:当气溶胶为粗粒子时 (Vfine/Vtotal＜0.2),α均小于0.75,仅用α就可以较好地判断粒子大小,但当气溶胶以细粒子为主时 (Vfine/Vtotal＞0.7),该方法会有较大出入,此时a2,a1可以有效地辅助α判断粒子大小,α＞0.75,a2＜-0.5或a2＜-0.5,a1＜-1.0是较好的判据。此外,分析发现国外研究提出的用a2-a1判断粒子大小的方法效果并不理想,尤其在1＜a2-a1＜2的情况下,粒子的组成有多种可能。 相似文献
6.
In this paper, the characteristics of eastern Asian dust storm are examined with emphasis on the satellite measurements of aerosol optical thickness. The reflectivity of solar radiation from the earth’s atmosphere depends on the optical thickness. The satellite measurement of radiance of sunlight, scattered by the earth and its atmosphere, is used to derive the properties of aerosol on oceanic surfaces. This paper involves the following: (1) investigation of the measurement of dust storm over the oceanic surface by GMS satellite; (2) investigation of the measurement of dust storm over the land surface by ground-based instruments such as actinometer, lidar, etc.; (3) for comparison, de-riving an atmospheric aerosol size distribution over the oceanic surface of calm weather through measurements of NOAA satellite; and (4) the weather process and its mass load of eastern Asian dust storm. 相似文献
7.
Multi-spectrai observations of solar radiation using a Volz sun-photometer have been carried out during February 24-March 2, 1995 in the vicinity of the blow-out of the gas well at Pasarlapudi, Andhra Pradesh, India. These unique and special observations have been utilized to study the aerosol, Rayleigh molecular and gaseous optical thicknesses. The re-sults of the analysis of the observations indicated, besides low gas concentrations well below their background values, sig-nificant variations in aerosol optical thickness (AOT) at visible and neat-infrared wavelength regions. The wavelength de-pendence of AOT revealed wide variations in the Junge aerosol size exponent from 0.98 to 6.70 indicating the presence of both sub-micron and coarse-mode aerosol particles over the observational site. A close correspondence between AOT and surface-level meteorological parameters during the period of observations was also noticed. 相似文献
8.
大气气溶胶的卫星遥感及其在气候和环境研究中的应用 总被引：2，自引：1，他引：1
卫星遥感可以获得全球范围的大气气溶胶光学特性,目前国内外已有多颗卫星观测能够提供气溶胶特性的资料。本文综述性介绍国内外卫星遥感气溶胶特性方面的研究进展和成果,并讨论了卫星遥感资料在气候和环境研究领域中的应用。主要内容包括:极轨/静止卫星平台搭载的被动遥感传感器及其反演气溶胶特性的方法;星载激光雷达获取气溶胶光学特性的方法;国内外正在研发的新一代卫星主、被动气溶胶遥感探测器;卫星气溶胶产品在气溶胶辐射强迫、气候效应、大尺度污染输送、区域空气质量监测等研究中的应用。 相似文献
9.
陆地上空标量辐射对地表反射率和大气气溶胶散射都具有很强的敏感性,而偏振反射只对大气气溶胶敏感,对地表不敏感。根据这个原理并结合POLDER(POLarization and Directionality of Earth Reflectance)资料的特点,作者提出综合利用标量辐射和偏振反射信息来实现陆地上空大气气溶胶和地表反照率的同时反演。首先,利用多角度偏振辐射观测提取大气气溶胶光学参数,再利用标量辐射测量对偏振反演结果作进一步筛选和订正,同时获得地表反射率。数值模拟试验结果证明,仅利用偏振信息只能获取大气气溶胶信息,而且其结果误差较大,特别是对于散射作用较强的短波长通道如670 nm误差更大,但经过标量辐射订正后的结果得到明显改善,气溶胶光学厚度和地表反射率与真实值之间相关系数都达到0.99以上。为提高查找表的计算效率,提出并建立了反演方案所需要的半参数化数值表,利用内插方法寻求气溶胶光学厚度和地表反射率的数值解的反演方法。 相似文献
10.
Retrieval of aerosol optical properties over a vegetation surface using multi-angular,multi-spectral,and polarized data 总被引：1，自引：0，他引：1
An algorithm to retrieve aerosol optical properties using multi-angular,multi-spectral,and polarized data without a priori knowledge of the land surface was developed.In the algorithm,the surface polarized reflectance was estimated by eliminating the atmospheric scattering from measured polarized reflectance at 1640 nm.A lookup table （LUT） and an iterative method were adopted in the algorithm to retrieve the aerosol optical thickness （AOT,at 665 nm） and the （A）ngstr（o）m exponent （computed between the AOTs at 665 and 865 nm）.Experiments were performed in Tianjin to verify the algorithm.Data were provided by a newly developed airborne instrument,the Advanced Atmosphere Multi-angle Polarization Radiometer （AMPR）.The AMPR measurements over the target field agreed well with the nearby ground-based sun photometer.An algorithm based on Research Scanning Polarimeter （RSP） measurements was introduced to validate the observational measurements along a flight path over Tianjin.The retrievals were consistent between the two algorithms.The AMPR algorithm shows potential in retrieving aerosol optical properties over a vegetation surface. 相似文献
11.
大气气溶胶的垂直非均一对向上亮度和卫星遥感地表反射率的效应 总被引：1，自引：0，他引：1
均一模式和两层模式是两个忽略气溶胶垂直非均一、并广泛用于卫星遥感的辐射模式。通过两个模式的数值模拟，分析了气溶胶的垂直非均一对向上天空亮度和卫星遥感地面反射率的效应。数值模拟选用了２４个有代表性的气溶胶模式。对于具有强分子散射的卫星短波通道，由于分子和气溶胶散射性的明显不同，应用均一和两层模式计算的向上亮度往往存在较大误差。对长波通道，如果气溶胶的光学特性随高度变化不大，该亮度误差较小，但如果存在不同散射相函数和一次散射反照率的气溶胶层，该误差仍可能较大。对于干净的大气，由均一和两层模式计算的亮度误差可分别高达３１．４％和３１．５％，而对于混浊的大气，该误差可分别高达６７．８％和５９．２％。该亮度误差可以引起地表反射率解存在大的不确定性，特别是对于短波通道和强吸收的气溶胶。对于包含强吸收气溶胶的混浊大气，均一和两层模式不适合于大气订正应用。 相似文献
12.
北京地区大气气溶胶光学特性监测研究 总被引：23，自引：1，他引：23
该文依据气溶胶光学厚度测量原理,利用CE318太阳光度计,于2000年7月～2001年7月期间对北京地区大气气溶胶光学厚度进行观测试验,计算得到约50天的气溶胶光学厚度和Junge参数等大气光学特性数据,给出了北京地区气溶胶光学特性分布特征.计算统计得到北京城区晴空条件下的Junge参数为3
15、2001年3月份沙尘天气状况下急剧下降为2.28,而北京郊区顺义县的测量结果介于二者之间为2.65.分析表明,由试验获得的气溶胶光学特性数据对于分析和监测北京地区大气污染、改善北京地区空气质量具有一定的意义. 相似文献
13.
黄山大气气溶胶浓度和尺宽谱分布特征 总被引：1，自引：0，他引：1
1988年9月与1989年5月,我们用DL-8318型多道光学粒子计数器在黄山光明顶气象站进行了大气气溶胶的观测。初步得出:黄山大气气溶胶粒子浓度较低,其谱分布模式符合Junge提出的幂指数律谱分布函数,平均相对误差为19%,相关系数为0.99。 相似文献
14.
JINHUAN QIU 《Tellus. Series B, Chemical and physical meteorology》2001,53(1):72-82
The equivalent wavelength ( λ E ), at which the aerosol optical depth (AOD) is equal to broadband AOD (BAOD), can change in a wide range from 0.619 μm to 1.575 μm in the usual aerosol conditions. By using the least squares technique and some empirical corrections, a parameterized relationship of λ E with BAOD, Ångström wavelength exponent ( α ), solar zenith angle ( θ 0 ) and H2 O amount is developed. Using this relationship, and based on the strong sensitivity of BAOD on θ 0 when θ 0 >70°, the broadband extinction method to derive the spectral AOD and α is further proposed. As shown in comparative simulations to retrieve AOD by the present, Molineaux et al. and Gueymard methods, the present method has the best accuracy in most simulations using Junge, MODTRAN, log‐normal and Deirmendjian aerosol models. A key question of the pyrheliometer method to determine wavelength-dependent AODs is the effect of uncertainty in the aerosol size istribution. It is found that the AOD solution around λ E is less sensitive to the uncertainty. The wavelength exponent α is derived using an assumption of the stable atmospheric turbidity. If the pyrheliometer data from θ 0 =85° to 70° are used and the change of the turbidity is ±10%, the error of solution α is usually within ±0.32. If the variation of the turbidity is random, the mean value of a lot of the measurements of α would be very reasonable. 相似文献
15.
R.T. Pinker G. Pandithurai B.N. Holben T.O. Keefer D. Goodrich 《Atmospheric Research》2004,71(4):243-252
Characterization of aerosol optical properties, such as aerosol optical depth, Angstrom exponent, and volume size distribution at the semiarid site of Tombstone Arizona (31°23′N, 110°05′W, 1408 m) will be presented for one annual cycle. In this region, extensive observations of selected optical parameters such as aerosol optical depth (AOD) have been made in the past and reported on in the literature. Less is known about other optical characteristics that are important in climate modeling and remote sensing. New observational techniques and inversion methods allow for the expansion of the earlier information. Observations have been taken with a state of the art sun photometer for a 1-year period and their analysis will be presented here. Monthly mean AODs at 500 nm were found to be in the range of 0.03–0.12; the monthly mean Angstrom exponent ranged from 0.9 to 1.6, being higher in spring and summer and lower in late fall and winter. Volume size distributions exhibit clear dominance of smaller particles, with a gradual increase in size from winter to spring and into summer. Annual variation of the radii of the smaller and the larger particles ranged between 0.05–0.4 and 4–8 μm, respectively. Radiance measurements at 940 nm were used to estimate precipitable water. The retrieved values compared within limits of uncertainty with independently derived estimates from the National Center for Environmental Prediction (NCEP) regional weather forecast model. An interesting outcome from this study was the consistency found in aerosol optical depths as observed in this study and those derived about two decades ago. 相似文献
16.
尝试以单星多角度卫星观测数据同时反演晴空陆地的气溶胶光学厚度和地表反射率,并选取2009年5月的MODIS(Moderate Resolution Imaging Spectroradiometer)1B资料进行了反演试验.结果表明:单星多角度法反演得到的气溶胶光学厚度结果与MODIS气溶胶产品(MOD04)平均值的相关系数为0.7914;反演的地表反射率结果与MODIS地表反射率产品(MOD09)也具有较好的一致性.对直接利用单星多角度观测数据反演获得一段时间内平均的气溶胶光学厚度进行了有益的尝试. 相似文献
17.
本文利用NASA发布的MODIS气溶胶光学厚度产品,对西南地区2001～2016年气溶胶光度厚度空间分布和时间演变特征进行了分析,研究发现:(1)西南地区年均气溶胶光学厚度空间分布特征整体表现为东部高于西部,海拔低的地区气溶胶光学厚度高于海拔高的地区。高值中心位于四川盆地南部,低值区位于川西高原和云南北部地区。(2)西南地区季节气溶胶光学厚度空间分布特征与年均相似。(3)就西南各地区而言,重庆气溶胶光学厚度最大,其次是四川盆地和贵州地区,再次是云南地区,川西高原地区气溶胶光学厚度最小。(4)2001～2016年,西南地区年均气溶胶光学厚度呈显著减少趋势。夏季和秋季气溶胶光学厚度年际变化浮动较大,也具有显著的减少趋势。 相似文献
18.
本文在1986年6月西藏拉萨市十通道太阳光度计六天观测工作基础上，计算了高原地区的整层大气垂直光学厚度，与北京西郊1981年6月的资料对比表明，在可见和近红外波段，拉萨市的大气光学厚度只有北京的一半，甚至更小。分析了在高原地区利用臭氧的Chappuis吸收带反演大气臭氧总量的可行性、方法、结果及其合理性。接着，本文讨论了双通道法和多通道法计算水汽光学厚度的差别，并简要分析了影响水汽总量变化的原因。本文还讨论了拉萨地区六月份大气浑浊度的时变规律及其变化机制。大气浑浊度不仅与地面大气状况（对流、地面风速等）有关，而且取决于大气的湍流结构。最后，本文利用Philips—Twomey方法反演了气溶胶的谱分布，结果表明，高原六月份气溶胶谱形大多接近Junge分布形式。另外，文中还简单讨论了折射率对反演气溶胶谱的影响。 相似文献
19.
Continuous data of aerosol optical thickness monitored using differential optical absorption spectroscopy (DOAS) are correlated with the concentration of ground-measured suspended particulate matter (SPM). A high correlation is found between the DOAS and the ground SPM data, making it possible to calculate the mass extinction efficiency of the aerosols in the atmosphere. It is found that the value of mean mass extinction efficiency (MEE) varies over a range of 2.6–13.7m2 g?1, with smaller and larger values occurring for size distributions dominated by coarse and fine particles, respectively. 相似文献
20.
天空辐射计观测2006年春季北京地区气溶胶光学特性的研究 总被引：2，自引：0，他引：2
利用2006年3～5月天空辐射计观测数据反演得到北京地区春季大气气溶胶光学性质参数,包括大气气溶胶光学厚度(0.5μm)、Angstrm指数、单次散射反射比和粒子谱分布特征。结果表明:北京地区春季气溶胶平均光学厚度0.67,Angstrm指数0.54,单次散射比0.88,粒子吸收性质较弱,粒子谱呈双峰形,以粗粒子为主,粗、细模态粒子粒径分别集中在0.17μm和7.7μm左右。相比2004年此次观测期间气溶胶粒径较大,粒子体积浓度较高,散射作用在其消光特性中的比重略有下降。光学厚度日变化呈单峰型,日间单次散射比随时间逐渐递减,Angstrm指数在上午递减趋势明显,午后变得稳定。对同时观测的天空辐射计与CE-318不同波长光学厚度结果进行比较,结果显示两者得到的光学厚度相关性很好,各波长小时平均结果的相对误差小于7%。 相似文献