共查询到18条相似文献，搜索用时 171 毫秒
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本文通过比较太阳直射表和太阳光度计探测的大气柱气溶胶光学厚度，分析了从太阳直射表探测的全波段太阳直射光强信息确定大气柱气溶胶光学厚度的误差，并应用北京观象台的太阳直射表观测资料，反演得到了 1990—1993年北京大气柱气溶胶光学厚度，分析了该光学厚度月与年变化规律以及1991年菲律宾皮纳图博火山爆发对北京大气气溶胶含量的影响。本文还提出了关于有效水汽含量的一个经验关系式，用于确定水汽对太阳辐射的吸收率。 相似文献
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本文介绍一个简单、经济的适用于各种多层大气环流模式中计算臭氧加热率的参数化方案,利用这一方案,可根据臭氧总量气候观测值及其垂直分布资料计算臭氧加热率,也可以在模式中加入臭氧方程,用预报的臭氧含量计算臭氧加热率.用此方案对单站气候资料试算,结果指出,随着高度的增加,臭氧吸收太阳辐射对大气太阳加热率的贡献逐渐接近、达到并在平流层50hPa附近明显超过其它物质如水汽的贡献.此方案用于九层大气环流模式时,对其辐射加热率的计算有较理想的改进,并使模拟的大气温度垂直分布更符合观测事实. 相似文献
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卫星遥感地面紫外辐射的参数化方法 总被引：6，自引：2，他引：6
提出了一个从卫星观测推算地面UVB辐射通量密度和红斑生物紫外辐射剂量的新的参数化方法。该方法基于一个简单的模式:大气辐射传输介质被简化成三个等效层:臭氧单独构成的吸收层，空气分子、云和气溶胶粒子组成的散射层，以及地面反射层。地面紫外辐射通量密度和生物紫外辐射剂量可以由臭氧层的等效透过率、散射层和地面的联合反射率计算。臭氧层的等效透过率可由大气臭氧总量计算。散射层和地面的联合反射率可由不存在臭氧吸收的紫外或可见光通道的反射辐射强度测量得到。该反演算法形式简单，只包含很少几个可从卫星测量获得的参数。它通过了一个可靠而相对复杂的基于DISORT的紫外辐射传输模式的检验。在广泛的计算条件下，包括晴天、云天、以及混浊大气，用这个简单算法计算的地面紫外辐射通量密度和红斑生物紫外辐射剂量与精确算法的结果相差无几。另外，还实际运用这个算法利用卫星观测资料反演地面紫外辐射通量密度，与地面实际观测资料做了比较，符合较好。 相似文献
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本文提出了一种由地面观测的太阳光谱确定某些大气成分含量的方法。这种方法不需要预先知道观测光谱的基线,从而可避开复杂的观测定标手续。以实验室测量资料和吸收气体的谱线资料为基础计算待定大气成分的透过率,并用当时的探空测量为基础对水汽吸收进行了订正。利用1978年10月在香河观测的太阳光谱计算了二氧化碳的混合比和垂直气柱内臭氧总含量,证明这种方法是可行的。 相似文献
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大气臭氧总量的经验计算方法 总被引：1，自引：0，他引：1
白建辉 《南京气象学院学报》2006,29(6):799-805
依据臭氧生消与紫外辐射(UV)能量利用相互作用的观点,考虑与臭氧有关的主要因子UV、大气中物质在化学和光化学反应中对UV能量的吸收、气溶胶粒子的散射等,在分析1990—1992年臭氧总量、太阳辐射、气象资料的基础上,建立了计算臭氧总量的经验模式,其优点是所用资料均可由常规气象站获得。结果表明,计算值与观测值符合得比较好。利用该经验模式计算了北京地区1979年1月—1996年6月的臭氧总量,计算值与观测值同样比较一致,二者相对偏差的最大值、最小值、平均值分别为15.2%、0.05%和4.9%,相对偏差在±10%之内的比例为91.4%,因而该经验模式是合理、可行的。1991年之后北京地区臭氧的下降与Pinatubo火山气溶胶的影响有关。 相似文献
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平流层臭氧变化对大气加热率及到达地面紫外辐射的影响 总被引：2，自引：2，他引：2
平流层臭氧的变化对平流层的温度结构，整个大气环流以及到达地面的紫外辐射均有影响。本文采用一个计算臭氧吸收太阳辐射的参数化方法和有关资料，研究了臭氧变化对大气最大加热率和到达地面的紫外辐射通量密度的影响情况。文中给出的参数化方法可直接应用于大气环流模式计算臭氧吸收太阳辐射的加热率。 相似文献
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从全波段太阳直射辐射确定大气气溶胶光学厚度 I. 理论 总被引：3，自引：1，他引：3
本文提出了从全波段太阳直射辐射信息确定0.7μm波长大气柱气溶胶光学厚度的一种新方法。数值试验表明，对各类气溶胶谱分布，在水汽含量±0.2cm的误差、臭氧总量±0.1cm的误差、太阳直射辐射的±1%的观测误差以及太阳常数的±2%误差范围内，对小于0.1的0.7μm波长气溶胶光学厚度，它的解误差一般小于0.017，对大于0.1并小于0.6的光学厚度，它的解误差一般小于10%。 相似文献
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《大气与海洋》2013,51(1):159-184
Abstract One of the main concerns regarding a decrease in stratospheric ozone is the consequential increasein the amount of ultraviolet (UV) radiation that reaches the lower atmosphere and the Earth's surface. Radiationat UV wavelengths where ozone absorbs strongly is detrimental to most biological species, including humanbeings, so a decrease in stratospheric ozone could have a significant impact on the biosphere. This concern hasled to a significant increase in surface UV radiation research over the last two decades since the ratification ofthe Montreal Protocol. Studies include investigations into understanding the complicated absorption and scatteringprocesses involved in the radiative transfer of UV through the atmosphere as well as research on theimpacts of changes in UV radiation. Factors affecting surface UV radiation will be discussed, resources used tostudy surface UV radiation will be described and progress made in our understanding of surface UV radiationover the past two decades will be reviewed. 相似文献
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漠河地区臭氧的观测和计算 总被引：2，自引：0，他引：2
1997年3月上旬,在黑龙江漠河地区对地面和整层臭氧、太阳辐射等进行了短期观测,以初步了解该地区臭氧和辐射的变化规律以及它们之间的相互关系.研究发现,漠河地区近地面臭氧日变化明显,其峰值出现在每日10:00(北京时间)左右,并早于紫外辐射(UV)峰值出现时间.整层大气臭氧总量的日变化特征不明显.基于UV能量守恒,建立了臭氧与其影响因子-光化学、散射、UV等因子之间较好的定量关系和经验模式,并将其用于计算地面、整层大气臭氧小时值和日平均值.结果表明,计算值与观测值吻合的都比较好,它们相对偏差的平均值分别为:地面臭氧小时值(11.9%)和日平均值(9.0%);整层大气臭氧小时值和日平均值-7.4%、1.8%.因此,地面和整层臭氧的经验算法是合理和可行的.利用散射辐射/直接辐射(D/S)和散射辐射/总辐射(D/Q)可以描述大气中的物质如气溶胶、云等的散射作用.采用D/Q表示散射作用可以提高地面臭氧和整层大气臭氧计算的准确度,特别是对云量较大的情况.
相似文献
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气溶胶大气对太阳辐射的吸收 总被引：15，自引：5，他引：15
大气气溶胶对大气吸收太阳辐射的影响有许多人研究过。目前计算大气吸收太阳辐射的数值模式多数仍忽略大气气溶胶的作用。大气气溶胶一方面本身吸收太阳辐射;一方面对太阳辐射多次散射,使阳光在大气中传输更长的路程,增加了吸收物质对太阳辐射的吸收。计算表明:大气气溶胶对大气吸收太阳辐射的作用是显著而不能忽略的。 相似文献
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D.G. Kaskaoutis H.D. Kambezidis Shailesh Kumar Kharol K.V.S. Badarinath 《Atmospheric Research》2007,86(3-4):286-296
This study focuses on the determination of optical depths caused by ozone and trace gases absorption in the Chappuis band, 500–700 nm, and the contribution to the Total Minus Rayleigh Optical Depth (TMROD). The optical depths were derived using the transmission functions implemented in the SMARTS parametric model, while the Total Optical Depths (TODs) were derived by solar extinction measurements obtained in Athens during May 1995. From the data analysis it is obvious that both the ozone and trace gases contribute significantly to TMROD in the Chappuis band. More specifically, the trace gases contributions are higher for air with high pollution levels, while ozone's contribution can be significant under clear-sky conditions. Therefore, the correction in TMROD due to ozone and trace gases optical depths is necessary for an accurate determination of the Aerosol Optical Depth (AOD) in the Chappuis band. The optical depth of ozone is generally removed during the process of the AOD retrievals, since the significance of its absorption in the Chappuis band is well understood. Nevertheless, the optical depth of the trace gases (mainly NO2) is not always taken into account in the AOD retrievals, though its contribution can be significant in urban polluted atmospheres. In this respect, the present study attempts to quantify the ozone and trace gases contributions in an urban environment and to provide some new functions that help estimate the contribution of ozone to the TMROD in the Chappuis band. 相似文献
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Joonsuk Lee Won Jun Choi Deok Rae Kim Seung-Yeon Kim Chang-Keun Song Jun Suk Hong Youdeog Hong Sukjo Lee 《Asia-Pacific Journal of Atmospheric Sciences》2013,49(3):271-278
Surface erythemal UV radiation is mainly affected by total column ozone, aerosols, clouds, and solar zenith angle. The effect of ozone on the surface UV radiation has been explored many times in the previous studies due to the decrease of ozone layer. In this study, we calculated the effect of aerosols on the surface UV radiation as well as that of ozone using data acquired from Ozone Monitoring Instrument (OMI). First, ozone, aerosol optical depth (AOD), and surface erythemal UVB radiation measured from satellite are compared with those from ground measurements. The results showed that the comparison for ozone was good with r 2 of 0.92. For aerosol, there was difference between satellite measurements and surface measurements due to the insufficient information on aerosol in the retrieval algorithm. The r 2 for surface erythemal UV radiation was high (～0.94) but satellite measurements showed about 30% larger values than surface measurements on average by not considering the effect of absorbing aerosols in the retrieval process from satellite measurements. Radiative amplification factor (RAF) is used to access the effect of ozone and aerosol quantitatively. RAF for ozone was 0.97～1.49 with solar zenith angle. To evaluate the effect of aerosol on the surface UV radiation, only clear-sky pixel data were used and solar zenith angle and total column amount of ozone were fixed. Also, RAF for aerosol was assessed according to the single scattering albedo (SSA) of aerosols. The results showed that RAF for aerosol with smaller SSA (< 0.90) was larger than that for with larger SSA (> 0.90). The RAF for aerosol was 0.09～0.22 for the given conditions which was relatively small compared to that for ozone. However, considering the fact that aerosol optical depth can change largely in time and space while the total column amount of ozone does not change very much, it needs to include the effect of aerosol to predict the variations of surface UV radiation more correctly. 相似文献
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Sensitivity Studies for Monitoring Tropospheric Ozone from Space Using the Ultraviolet,Visible,and Polarization Bands 
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下载免费PDF全文 The authors analyzed the retrieval sensitivity of tropospheric ozone using simulated the Global Ozone Monitoring Experiment-2 （GOME-2） measurements. The retrieval sensitivity was evaluated by the degree of free- dom for signal （DFS）. The combination of the ultraviolet （UV）, UV polarization （UVPOL）, and visible （VIS） bands enhances DFS of tropospheric ozone and improves the vertical resolution of the retrieved ozone profile. UVPOL reduces the dependence on solar zenith angle, mainly in- creases the sensitivity in upper troposphere. Polarization increased the DFS by 20% on the eastern side of the GOME-2 orbit, with little improvement on the western side because the increase in DFS due to polarization is depend- ent on the relative azimuth angle. The inclusion of the visi- ble band reduces significantly the dependence on viewing geometry, and mainly increases the DFS in the lower tro- posphere （0-6 kin） by a factor of two. It was possible to retrieve several independent pieces of tropospheric ozone information from GOME-2 UV/UVPOL/VIS measure- ments, especially in the lower troposphere. 相似文献
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比较分析了2017年南极中山站3种仪器测量地面太阳紫外B（UVB）波段和紫外A（UVA）波段的辐照度。以Brewer光谱仪测值为参考,国产宽波段FSUVB日射表在UVB（波段280~315 nm）的辐照度相对误差为（55±75）%,误差随大气臭氧总量的增加呈上升趋势,但在南极“臭氧洞”期间偏低。Yankee UVB宽波段日射表在UVB（波段280~320 nm）的辐照度相对误差为（-31±22）%;国产宽波段FSUVA日射表在UVA（波段315~400 nm）的辐照度相对误差为（23±5.9）%。太阳天顶角低于80°的晴天以Tropospheric Ultraviolet Visible（TUV）辐射模式计算结果为参考时,FSUVB,Yankee UVB和FSUVA辐照度的平均相对误差分别为（30±37）%,（-22±19）%和（27±6.4）%,而Brewer相对误差未超过3.5%。国产宽波段UV日射表测值偏高,反映出波长较长的杂散光对太阳辐照度测值影响明显。 相似文献
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K. V. S. Badarinath Shailesh Kumar Kharol V. Krishna Prasad Anu Rani Sharma E. U. B. Reddi H. D. Kambezidis D. G. Kaskaoutis 《Journal of Atmospheric Chemistry》2008,59(3):219-236
Measurements of total ozone column and solar UV radiation under different atmospheric conditions are needed to define variations
of both UV and ozone and to study the impact of ozone depletion at the Earth’s surface. In this study, spectral and broadband
measurements of UV-B irradiance were obtained along with total ozone observations and aerosol optical depth measurements in
the tropical urban region of Hyderabad, south India. We specifically used an Ultra-Violet Multifilter Rotating Shadow band
Radiometer (UVMFR-SR), to measure UV irradiance in time and space. To assess the aerosol and O3 effects on ground-reaching UV irradiance, we used measurements from a Microtops II sun photometer in addition to the Tropospheric
Ultraviolet Visible radiation (TUV) model. We also assessed the Defense Meteorological Satellite Program – Operational Line
Scanner (DMSP-OLS) night time satellite data for inferring biomass burning fires during the study period. Results clearly
suggested a negative correlation between the DMSP-OLS satellite derived fire count data and UVMFR-SR data suggesting that
aerosols from biomass burning are directly attenuating UV irradiance in the study region. Also, correlation analysis between
UV index and ozone measurements from sun photometer and TOMS-Ozone Mapping Instrument (OMI) indicated a clear decrease in
ground reaching UV-B irradiance during higher ozone conditions. The higher levels are attributed to photochemical production
of O3 during the oxidation of trace gases emitted from biomass burning. Results also suggested a relatively high attenuation in
UV irradiance (~6% higher) from smoke particles than dust. We also found a relatively good agreement between the modeled (TUV)
and measured UV irradiance spectra for different atmospheric conditions. Our results highlight the factors affecting UV irradiance
in a tropical urban environment, south India. 相似文献