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Global Characterization of CO2 Column Retrievals from Shortwave-Infrared Satellite Observations of the Orbiting Carbon Observatory-2 Mission

机译:轨道碳观测站2号任务的短波红外卫星观测中的CO 2 列检索的全局表征

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The global characteristics of retrievals of the column-averaged CO2 dry air mole fraction, XCO2, from shortwave infrared observations has been studied using the expected measurement performance of the NASA Orbiting Carbon Observatory-2 (OCO-2) mission. This study focuses on XCO2 retrieval precision and averaging kernels and their sensitivity to key parameters such as solar zenith angle (SZA), surface pressure, surface type and aerosol optical depth (AOD), for both nadir and sunglint observing modes. Realistic simulations have been carried out and the single sounding retrieval errors for XCO2 have been derived from the formal retrieval error covariance matrix under the assumption that the retrieval has converged to the correct answer and that the forward model can adequately describe the measurement. Thus, the retrieval errors presented in this study represent an estimate of the retrieval precision. For nadir observations, we find single-sounding retrieval errors with values typically less than 1 part per million (ppm) over most land surfaces for SZAs less than 70° and up to 2.5 ppm for larger SZAs. Larger errors are found over snow/ice and ocean surfaces due to their low albedo in the spectral regions of the CO2 absorption bands and, for ocean, also in the O2 A band. For sunglint observations, errors over the ocean are significantly smaller than in nadir mode with values in the range of 0.3 to 0.6 ppm for small SZAs which can decrease to values as small as 0.15 for the largest SZAs. The vertical sensitivity of the retrieval that is represented by the column averaging kernel peaks near the surface and exhibits values near unity throughout most of the troposphere for most anticipated scenes. Nadir observations over dark ocean or snow/ice surfaces and observations with large AOD and large SZA show a decreased sensitivity to near-surface CO2. All simulations are carried out for a mid-latitude summer atmospheric profile, a given aerosol type and vertical distribution, a constant windspeed for ocean sunglint and by excluding the presence of thin cirrus clouds. The impact of these parameters on averaging kernels and XCO2 retrieval errors are studied with sensitivity studies. Systematic biases in retrieved XCO2, as can be introduced by uncertainties in the spectroscopic parameters, instrument calibration or deficiencies in the retrieval algorithm itself, are not included in this study. The presented error estimates will therefore only describe the true retrieval errors once systematic biases are eliminated. It is expected that it will be possible to retrieve XCO2 for cloud free observations and for low AOD (here less than 0.3 for the wavelength region of the O2 A band) with sufficient accuracy for improving CO2 surface flux estimates and we find that on average 18% to 21% of all observations are sufficiently cloud-free with only few areas suffering from the presence of persistent clouds or high AOD. This results typically in tens of useful observations per 16 day ground track repeat cycle at a 1° × 1° resolution. Averaging observations acquired along ~1° intervals for individual ground tracks will significantly reduce the random component of the errors of the XCO2 average product for ingestion into data assimilation/inverse models. If biases in the XCO2 retrieval of the order of a few tenth ppm can be successfully removed by validation or by bias-correction in the flux inversion, then it can be expected that OCO-2 XCO2 data can lead to tremendous improvements in estimates of CO2 surface-atmosphere fluxes.
机译:利用NASA轨道的预期测量性能,研究了短波红外观测获得的列平均CO 2 干燥空气摩尔分数X CO2 的全局特征。 Carbon Observatory-2(OCO-2)任务。这项研究的重点是最低点和最低点的X CO2 提取精度和平均内核及其对关键参数(例如太阳天顶角(SZA),表面压力,表面类型和气溶胶光学深度(AOD))的敏感性。阳光观察模式。已经进行了现实的模拟,并且假设检索已经收敛到正确的答案,并且正向模型可以将X CO2 的单一探测检索误差从形式检索误差协方差矩阵导出,充分描述测量结果。因此,本研究中提出的检索错误代表了检索精度的估计。对于天底观测,对于小于70°的SZA,我们发现在大多数陆地表面上单声音取回误差的值通常小于百万分之一(ppm),对于较大的SZA,其误差高达2.5 ppm。在雪/冰和海洋表面发现较大的误差,这是由于在CO 2 吸收带的光谱区域中反照率低,对于海洋,在O 2 一个乐队。对于日照观测,海洋上的误差明显小于天底模式,小型SZA的值在0.3至0.6 ppm范围内,最大SZA的值可减小至0.15 ppm。取回的垂直灵敏度由列平均表示,该取平均值是对最接近的场景在整个对流层中的大部分对流层表面附近的核峰进行平均,并显示出接近于1的值。在黑暗的海洋或雪/冰表面的天底观测以及具有大AOD和大SZA的观测表明对近地表CO 2 的敏感性降低。所有模拟都针对夏季中纬度的大气廓线,给定的气溶胶类型和垂直分布,海洋日照的恒定风速以及排除了薄卷云的存在而进行。通过敏感性研究研究了这些参数对平均内核和X CO2 取回误差的影响。检索到的X CO2 的系统偏差(如光谱参数的不确定性,仪器校准或检索算法本身的缺陷所导致)不包括在本研究中。因此,一旦消除了系统偏差,提出的误差估计将仅描述真实的检索误差。预期将有可能获取X CO2 用于无云观测和低AOD(此处O 2 波段的波长区域小于0.3)准确度足以改善CO 2 表面通量估计值,我们发现平均所有观察结果中有18%至21%完全没有云,只有极少数地区存在持续的云或高AOD 。这通常导致在16°地面轨道重复周期中以1°×1°分辨率进行数十次有用的观测。沿大约1°间隔获取的单个地面轨迹的平均观测值将显着减少X CO2 平均乘积误差的随机分量,以吸收到数据同化/逆模型中。如果通过验证或通量反转中的偏差校正可以成功消除十分之几的X CO2 检索中的偏差,那么可以预期OCO-2 X CO2 数据可以大大改善CO 2 表面大气通量的估算。

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