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首页> 外文期刊>Plant Production Science >Testing Polarization Measurements with Adjusted View Zenith Angles in Varying Illumination Conditions for Detecting Leaf Orientation of Wheat Canopy
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Testing Polarization Measurements with Adjusted View Zenith Angles in Varying Illumination Conditions for Detecting Leaf Orientation of Wheat Canopy

机译:在不同的照明条件下使用调整后的视图天顶角测试偏振测量,以检测小麦冠层的叶片方向

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The previous work revealed that the polarization of light reflected from heading wheat canopies allowed the detection of changes in the canopy structure, i.e., the leaf inclination angle. Accordingly, in order to improve measurement accuracy in this study we examined the effects of the solar zenith angle (=90°-solar elevation) and weather conditions at the time of polarization measurements for the light reflected from wheat canopies that were fertilized by different means. We measured polarization in the 660 nm spectral band from the heading canopies of wheat, which were grown in plots fertilized with a basal dressing and then top-dressed at the jointing and booting stages. The radiometric measurements were carried out at various solar zenith angles: 22°-41° on two proximal days, one overcast and the other clear. An empirical method for the adjustment of view zenith angle, based on the solar position at the time of measurement, was effective for the measurement of the degree of polarization (i.e., ratio of the polarized part of reflected light to the total reflected light energy) to eliminate interference due to the change in solar zenith angle. Although the mean values of polarization degree measured in overcast conditions were significantly lower than those measured under clear conditions, the plots top-dressed at the jointing stage could be detected via the polarized reflected light measured under both conditions of illumination.
机译:先前的工作表明,从抽穗的小麦冠层反射的光的偏振允许检测冠层结构的变化,即叶片倾斜角。因此,为了提高这项研究中的测量精度,我们对通过不同方式施肥的小麦冠层反射的光进行极化测量时,考察了太阳天顶角(= 90°-太阳能仰角)和天气状况的影响。 。我们测量了来自抽穗小麦冠部的660 nm光谱带中的极化,该冠层生长在施有基肥的地块中,然后在拔节和孕穗期进行追肥。辐射测量是在各种太阳天顶角下进行的:在近日的22天至41度,一次阴天,另一次晴天。基于测量时太阳位置的经验天顶角度调整的经验方法对于测量偏振度(即反射光的偏振部分与总反射光能量之比)是有效的消除由于太阳天顶角变化而产生的干扰。尽管在阴暗条件下测得的偏振度平均值明显低于在晴天下测得的偏振度平均值,但是在接合阶段处于最上层的图可以通过在两种照明条件下测得的偏振反射光来检测。

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