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首页> 外文期刊>Journal of the Atmospheric Sciences >Cellular Statistical Models of Broken Cloud Fields. Part IV: Effects of Pixel Size on Idealized Satellite Observations
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Cellular Statistical Models of Broken Cloud Fields. Part IV: Effects of Pixel Size on Idealized Satellite Observations

机译:破碎云场的蜂窝统计模型。 第四部分:像素尺寸对理想卫星观测的影响

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In the fourth part of our "Cellular Statistical Models of Broken Cloud Fields" series we use the binary Markov processes framework for quantitative investigation of the effects of low resolution of idealized satellite observations on the statistics of the retrieved cloud masks. We assume that the cloud fields are Markovian and are characterized by the "actual" cloud fraction (CF) and scale length. We use two different models of observations: a simple discrete-point sampling and a more realistic "pixel" protocol. The latter is characterized by a state attribution function (SAF), which has the meaning of the probability that the pixel with a certain CF is declared cloudy in the observed cloud mask. The stochasticity of the SAF means that the cloud-clear attribution is not ideal and can be affected by external or unknown factors. We show that the observed cloud masks can be accurately described as Markov chains of pixels and use the master matrix formalism (introduced in Part III of the series) for analytical computation of their parameters: the "observed" CF and scale length. This procedure allows us to establish a quantitative relationship (which is pixel-size dependent) between the actual and the observed cloud-field statistics. The feasibility of restoring the former from the latter is considered. The adequacy of our analytical approach to idealized observations is evaluated using numerical simulations. Comparison of the observed parameters of the simulated datasets with their theoretical expectations showed an agreement within 0.005 for the CF, while for the scale length it is within 1% in the sampling case and within 4% in the pixel case.
机译:在我们的第四部分“破碎云域”系列的“蜂窝统计模型”系列中,我们使用二元马尔可夫工艺进行定量调查对未检索的云面具的统计数据的低分辨率对理想化卫星观测的影响。我们假设云字段是马尔可夫,并且是“实际”云分数(CF)和比例长度的特征。我们使用两种不同的观察模型:一种简单的离散点采样和更现实的“像素”协议。后者的特征在于状态归因函数(SAF),其具有概率的含义,其具有特定CF的像素在观察到的云掩模中被声明多云。 SAF的随机性意味着云明确的归属并不理想,可能受到外部或未知因素的影响。我们表明观察到的云面罩可以准确地描述为像素的像素链,并使用主矩阵形式主义(在系列第III部分引入)进行分析计算参数:“观察到”CF和比例长度。该过程允许我们在实际和观察到的云场统计数据之间建立定量关系(这是依赖于像素大小)。考虑了从后者恢复前者的可行性。使用数值模拟评估我们分析方法对理想化观察的充分性。模拟数据集的观察参数与其理论期望的观察参数的比较显示了CF的0.005内的协议,而对于比例长度,在采样情况下在1%内,在像素盒中以4%内。

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