共查询到20条相似文献,搜索用时 15 毫秒
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Tom X.-P. Zhao Hongbin Yu Istvan Laszlo William C. Conant 《Journal of Quantitative Spectroscopy & Radiative Transfer》2008,109(7):1162-1186
A two-step approach is proposed to derive component aerosol direct radiative forcing (ADRF) at the top of atmosphere (TOA) over global oceans from 60°S to 60°N for clear-sky condition by combining Terra CERES/MODIS-SSF shortwave (SW) flux and aerosol optical thickness (AOT) observations with the fractions of component AOTs from the GSFC/GOCART model. The derived global annual mean component ADRF is +0.08±0.17 W/m2 for black carbon, −0.52±0.24 W/m2 for organic carbon, −1.10±0.42 W/m2 for sulfate, −0.99±0.37 W/m2 for dust, −2.44±0.84 W/m2 for sea salt, and −4.98±1.67 W/m2 for total aerosols. The total ADRF has also been partitioned into anthropogenic and natural components with a value of −1.25±0.43 and −3.73±1.27 W/m2, respectively. The major sources of error in the estimates have also been discussed. The analysis adds an alternative technique to narrow the large difference between current model-based and observation-based global estimates of component ADRF by combining the satellite measurement with the model simulation. 相似文献
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ARTS, the atmospheric radiative transfer simulator, version 2 总被引:2,自引:0,他引:2
P. Eriksson S.A. Buehler C.P. Davis O. Lemke 《Journal of Quantitative Spectroscopy & Radiative Transfer》2011,112(10):1551-1558
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Gabriele P. Stiller Thomas von ClarmannBernd Funke Norbert GlatthorFrank Hase Michael HöpfnerAndrea Linden 《Journal of Quantitative Spectroscopy & Radiative Transfer》2002,72(3):249-280
The accuracy of trace gas abundances retrieved from spectrally resolved infrared limb emission measurements relies, among other things, on the appropriate modelling of radiative transfer through the actual atmosphere. We quantify the mapping of several commonly applied simplifications in radiative transfer modelling on the trace gas abundances retrieval error at the example of the Michelson interferometer for passive atmospheric sounding (MIPAS)/environmental satellite (ENVISAT) space borne Fourier transform infra-red limb emission experiment. The Karlsruhe optimized and precise radiative transfer algorithm (KOPRA) which was used as a tool for this study will be introduced. KOPRA supports accurate modelling of the particular instrument requirements of MIPAS and the observation scenarios during the ENVISAT mission, in particular with respect to its viewing direction and its altitude coverage of the atmosphere. We show that disregarding of horizontal temperature inhomogeneities and non-local thermodynamic equilibrium effects, insufficient accuracy in modelling of field-of-view and apodisation effects, and disregarding individual profiles of isotopic species play the key roles in radiative transfer modelling and lead to systematic retrieval errors which can by far exceed the expected random retrieval error caused by measurement noise. 相似文献
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Vijay Natraj Run-Lie Shia Yuk L. Yung 《Journal of Quantitative Spectroscopy & Radiative Transfer》2010,111(5):810-816
Radiative transfer is computationally expensive. However, it is essential to many applications, in particular remote sensing retrievals. Principal component analysis of the optical depth and single scattering albedo profiles has been proposed as a possible method to help ease the computational burden. Here we show how the technique could be applied to a practical problem of CO2 retrievals from high spectral resolution measurements of reflected sunlight in three near infrared bands. We obtain a speed improvement of more than 50 fold (compared to monochromatic computations), while reproducing the radiances to better than 0.1% accuracy. 相似文献
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矢量辐射传输方程定量描述了辐射在地表-大气耦合介质中的传输过程,是定量遥感的基础.在处理辐射和离散介质相互作用时,如何处理多次散射、辐射偏振效应和耦合地表模型是研究的重点,直接影响定量化遥感反演的精度.文中基于逐次散射近似法求解了矢量辐射传输方程,求解过程中耦合典型地表的非偏双向反射(BRDF)模型和偏振双面反射(BPDF)模型.采用相对误差因子定量分析了地表双向反射效应和大气偏振效应对天基矢量辐射的影响.为进一步研究地表-大气耦合介质系统的偏振特性及地表大气参数的定量遥感反演提供理论支持.
关键词:
矢量辐射传输方程
逐次散射近似
定量遥感
偏振遥感 相似文献
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由于大气环境的变化,大气气溶胶污染对光学遥感器成像品质的影响越来越受到载荷研制部门的重视。天基光学遥感系统成像过程中,受到大气气溶胶退化的影响使得光学遥感器成像品质的恶化。大气导致图像质量降低主要原因之一是气溶胶混浊介质引起的前向光散射。根据气溶胶辐射特性,利用混浊介质辐射传输方程,推导了包含气溶胶光学特性的大气点扩散函数模型。根据此模型,定量化分析与评价其对光学遥感器成像的大气模糊效应。研究发现气溶胶介质除了对遥感器成像过程中大气透过率能量衰减影响外,更重要的是由于散射对成像质量产生退化作用,大气气溶胶光学厚度的增加使得气溶胶散射强度的增强,气溶胶光学厚度的变化同样强烈的影响着点扩散函数的空间分布范围,正是因为气溶胶在空间域内对图像产生的退化作用,使得遥感图像质量降低,尤其是图像清晰度的下降。同时,该模型也为遥感图像仿真中,大气链路环节的优化与改进提供了参考依据与模型方法。 相似文献
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Satellite observations of polar stratospheric clouds (PSCs) in the mid-infrared by high resolution limb emission spectrometers like the Michelson Interferometer for Passive Atmospheric Sounding have been simulated. For particles with radius the scattered tropospheric radiance accounts for a significant part of the continuum signal and leads to absorption line features overlaid over the stratospheric emission spectrum. The scattered radiance shows a strong dependence on particle size up to about radius with a maximum around 3-4. The contribution of scattered radiation depends heavily on tropospheric cloud coverage and earth surface temperature. Distinction of PSCs of different composition is possible for small particles due to differences in the imaginary part of the refractive index. For particles with radii between 1 and the simulated spectra for various PSC compositions differ due to different real parts of the refractive index. For larger particles no distinction is possible any more. Solar radiance scattered by PSCs is important for wavenumbers larger than about . For a forward scattering geometry with 30° between the position of the sun and the limb viewing direction solar contribution exceeds the terrestrial scattered radiation by about a factor of 10. 相似文献
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辐射压是影响大质量恒星结构和演化不可忽视的重要物理因素. 根据辐射压对非同步转动的洛希势函数的影响, 数值计算了洛希瓣的大小和3个拉格朗日点的位置和相应的势函数, 并与同步转动的洛希模型计算的结果做了对比. 结果发现: 辐射压可以整体地减小大质量恒星表面的重力加速度, 而转动离心力能最大减少赤道附近的重力加速度. 辐射压和非同步转动均可以明显地改变洛希瓣的大小和3个拉格朗日点的位置和势函数, 影响双星系统物质交换的时间. 因此, 研究辐射压, 非同步转动等物理因素对大质量双星系统洛希势函数的影响, 对密近双星的演化具有重要意义.
关键词:
恒星结构与演化
转动
辐射压 相似文献
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在二硫化碳(CS2)和苯(C6H6)的二元溶液中,随着相对体积浓度而变化,C6H6的基频ν1(992 cm-1) 的拉曼散射系数随浓度减小而增加,而CS2的基频ν1(656 cm-1)的拉曼散射系数则随浓度增加而增加。文章测量了这二元溶液相对不同体积浓度的拉曼光谱。结果表明,尽管CS2和C6H6的基频ν1的强度都随着浓度变化而发生较大变化,但C6H6的基频ν1对其参与的ν1+ν6~ν8费米共振几乎没有影响,而CS2的基频ν1强度的变化不仅对ν1~2ν2费米共振产生较大影响,还使基频ν2发生变化。文章给出了实验结果,并用Bertran费米共振理论和群论给予了解释。 相似文献
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偏振相函数是气溶胶重要的光学参数之一,它对气溶胶复折射指数、粒子尺度和形状都十分敏感。多角度多光谱偏振遥感可以有效获取气溶胶偏振相函数信息。新一代CIMEL太阳-天空偏振辐射计CE318-DP作为高精度地基气溶胶偏振遥感仪器已被引入全球气溶胶自动观测网AERONET(AErosol RObotic NETwork),并作为扩展多波长偏振测量的太阳-天空辐射计观测网SONET(Sun/sky-radiometer Observation NETwork)的主要仪器,已在不同类型气溶胶观测站点积累了多年的偏振数据。但目前偏振反演仅能利用线偏振度或偏振辐亮度。与线偏振度和偏振辐亮度相比,Stokes参数Q和U不仅包含天空光线偏振强度信息还包含偏振方向信息。利用CE318-DP多光谱多角度测量的天空光Stokes参数Q和U反演气溶胶偏振相函数的方法。针对CE318-DP标准主平面偏振观测模式PPP(Polarized Principal Plane)下Stokes参数U对气溶胶特性变化不敏感、信息难以利用的不足,测试了新的平纬圈偏振扫描模式ALMP(ALMucantar Polarization)获取Stokes参数Q和U,并成功应用于偏振相函数的反演。系统分析了340~1 640 nm多光谱通道上典型生物质燃烧型气溶胶和水溶性气溶胶的-P12/P11反演结果并测试了反演方法在晴朗和灰霾不同大气条件下的适用性。无论在主平面还是平纬圈观测几何下,反演结果在可见光和近红外通道上均与真实值具有较好的一致性。进一步讨论了模型中基于气溶胶参数初始值和大气气溶胶参数真实值计算的“大气单次散射/大气散射”的比值近似相等的假设条件在短波通道不能很好地满足是造成紫外波段反演结果偏差较大的原因之一。后续有待进一步提高反演模型在短波通道的适用性,为利用不同光谱通道上-P12/P11的变化特征改进气溶胶微物理参数反演奠定了基础。 相似文献
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Anton Sokolov Gueorgui Khomenko 《Journal of Quantitative Spectroscopy & Radiative Transfer》2008,109(9):1685-1692
Sensitivity of the solutions of forward and inverse problems of the atmospheric-surface parameters retrieval to spectral shifts of channels is considered. The solution of the forward problem is obtained by radiative transfer simulation. The retrieval (solution of the inverse problem) is obtained by linear (optimal interpolation) and non-linear (variational) techniques. It is shown that atmospheric temperature profiles exhibit high sensitivity to the spectral shift, while the humidity profiles are moderately sensitive while the sea surface temperatures retrievals are insensitive. Two approaches are proposed to reduce the effect of channel spectral shift, one is based on channel selection and the other approach is related to proper calibration of the cost function. We performed the numerical simulations using the parameters of AIRS spectrometer to illustrate the sensitivity of forward and inverse problems. The results of the simulation show that the inversion error can be significantly reduced by the proposed techniques. 相似文献
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以平面波为例,分别针对较弱和较强的湍流模型,通过计算到达角起伏讨论了高空光学遥感系统由大气湍流引起的地面图像分辨力问题。结果表明,对于给定的遥感系统口径和高度,较强湍流引起的图像分辨力的1cm左右;而较强湍流引起的图像分辨力则可达10cm量级。对于自身的地面分辨力具有m的量级的传统光学遥感系统,上述影响并不明显。对于现代高辨力光学遥感系统,这种影响便不容忽略,特别是对较强的湍流,往往需要用自适应光学等方法加以补偿。 相似文献
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采用考虑Davidson修正的内收缩多参考组态相互作用(icMRCI+Q)方法结合相关一致基组aug-cc-pV5Z和aug-cc-pV6Z首次计算了一氟化碳(CF)11个Λ-S 态(X2Π , a4Σ-, A2Σ+, B2Δ, 14Π, 12Σ-, 24Π, 1{4}Δ , 14Σ+, 22Σ-和24Σ-) 所产生的25个Ω 态的势能曲线. 计算中考虑了旋轨耦合效应、核价相关和标量相对论修正以及将参考能和相关能分别外推至完全基组极限. 基于得到的势能曲线, 获得了束缚和准束缚的Λ-S态和Ω 态的光谱常数, 与已有的实验结果非常符合. 分析了束缚和准束缚的Λ-S态在各自平衡核间距Re处的主要电子组态. 由于14Π 和24Π态的避免交叉, 发现准束缚态24Π. 由Λ-S态势能曲线的交叉现象, 借助于计算的旋轨耦合矩阵元, 分析了a4Σ-和B2Δ 态的预解离机理. 计算了25个Ω 态的离解关系, 给出了它们的离解极限. 最后研究了A2Σ+-X2Π 跃迁特性, 本文计算得到的A2Σ+-X2Π跃迁的Frank-Condon 因子和辐射寿命与已有实验值也符合得非常好. 相似文献
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Rached Salhi Carmen JimenezPatrick Chaudouët Ramzi MaalejMohieddine Fourati Jean-Luc Deschanvres 《Applied Surface Science》2012,258(7):2591-2596
The effect of deposition temperature, relative humidity of carrier gas and UV-assistance on the growth of Erbium-doped aluminium oxide films has been studied. The films were prepared from aluminium acetylacetonate (Al(C5H7O2)3) and erbium (III) Tris(2,2,6,6-tetramethyl-3,5-heptanedionate) (Er(TMHD)3) by UV and aerosol-assisted metal-organic chemical vapour deposition, using air with controlled humidity as carrier gas. Amorphous transparent films were deposited between 350 and 460 °C. It was observed that UV assistance allows a large decrease down to 5 kJ/mol of the activation energy of the deposition reaction for deposition temperatures lower than 420 °C. More over, depositing under high air humidity induced higher deposition rate, lower level of organic contamination and higher film density. Under these conditions Er-doped aluminium oxide films with a refractive index value of 1.71 were obtained at 460 °C. 相似文献
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本文用遥感FTIR光谱 ,测定了固体推进剂燃烧火焰在光谱范围为 4 5 0 0~ 70 0cm- 1 处的红外发射光谱 ,利用HCl分子转振基带 (3 4 6 μm)精细结构的P 分支光谱 ,准确测定了固体推进剂燃烧火焰温度 ,并对含有不同材料固体推进剂 ,如有机化合物对燃烧温度的影响 ,作了讨论。 相似文献
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采用考虑Davidson修正的内收缩多参考组态相互作用(icMRCI+Q)方法结合相关一致基组aug-ccpV5Z和aug-cc-pV6Z计算了CF~+离子第一离解极限C~+(~2p_u)+F(~2P_u)对应的12个∧-S态(X~l∑~+,a~3∏,1~3∑~+,1~3Δ,1~1∑~-,1~1∑~-,1~3∑~-,2~1∑~+,1~1∏,2~3∏,2~1∏和2~3∑~+)所产生的23个Ω态的势能曲线.计算中考虑了旋轨耦合效应、核价相关和标量相对论修正以及将参考能和相关能分别外推至完全基组极限.基于得到的势能曲线,获得了束缚和准束缚的9个∧-S态和16个Ω态的光谱常数,并且X~1∑~+,a~3∏~(势阱一)∧-S态的光谱常数与已有的实验结果非常符合.此外,计算了CF自由基X~2∏态到CF~+离子束缚和准束缚的9个∧-S态的垂直电离势和绝热电离势,并且CF~+(X~1∑~+)←CF(X~2∏)和CF~+(a~3∏(势阱一))←CF(X~2∏)的垂直电离势和绝热电离势与相应的实验结果也非常符合.由a~3∏,1~1∏态和其他激发∧-S态势能曲线的交叉现象,借助于计算的旋轨耦合矩阵元,分析了a~3∏~(势阱一),1~1∏~(势阱一)和2~1∑~+态的预解离机理.计算的23个Ω态离解极限处的相对能量与实验结果十分吻合.最后计算了(2)0+~(势阱一)(v'=0-5),(1)1~(势阱一)(v'=0-5)和(2)1~(势阱一)(v'=0)到X0~+态跃迁的Franck-Condon因子和辐射寿命. 相似文献