Correcting for Circumsolar and Near-Horizon Errors in Sky Cover Retrievals from Sky Images

C. Long
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引用次数: 29

Abstract

Fractional sky cover amounts retrieved from sky imagery are overestimated significantly at times due to occurrences of “whitening” near the sun, and near the horizon for low sun, in the images. This phenomenon occurs due to forward scattering of visible light by aerosols and haze, and the intensity range limitations of the detectors of the cameras used to record the sky images. Our results suggest that when the problem occurs, the magnitude of the overestimate is typically on the order of about 10% to 20% fractional sky cover. To help alleviate this problem, a statistical analysis of the time series of the areas in the image near the sun position and along the horizon centered on the solar azimuth angle has been developed. This statistical analysis requires that images be captured frequently, at least once per minute. For times when the overestimation is detected as occurring, a correction is applied to the retrieved sky cover amounts. When the sky cover amount correction is applied, analysis indicates that the result better matches the actual sky conditions present, as noted by visual inspection of the sky images in question. In addition, frequency-of-occurrence histogram comparisons show that the adjusted results improve the agreementmore » with other methodologies and expectations. Thus, the methodology presented here helps produce more accurate fractional sky cover retrievals.« less
从天空图像中反演天空覆盖物的周日和近地误差校正
由于图像中太阳附近和低太阳时地平线附近出现的“白化”现象,从天空图像中检索到的部分天空覆盖量有时会被明显高估。这种现象的发生是由于气溶胶和雾霾对可见光的前向散射,以及用于记录天空图像的相机探测器的强度范围限制。我们的结果表明,当问题发生时,高估的幅度通常在10%到20%的天空覆盖分数的量级上。为了缓解这个问题,对图像中太阳位置附近和以太阳方位角为中心的地平线上的区域的时间序列进行了统计分析。这种统计分析要求经常捕获图像,至少每分钟捕获一次。当检测到出现高估时,对检索到的天空覆盖量进行校正。当应用天空覆盖量校正时,分析表明结果更符合实际的天空条件,正如对所讨论的天空图像的目视检查所指出的那样。此外,出现频率直方图比较表明,调整后的结果与其他方法和期望的一致性更高。因此,这里提出的方法有助于产生更准确的天空覆盖检索分数。«少
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