Estimating light environment in forests with a new thresholding method for hemispherical photography

被引:13
|
作者
Zhao, Kangning [1 ,2 ]
He, Fangliang [1 ,2 ,3 ]
机构
[1] Sun Yat Sen Univ, State Key Lab Biocontrol, SYSU Alberta Joint Lab Biodivers Conservat, Guangzhou 510275, Guangdong, Peoples R China
[2] Sun Yat Sen Univ, Sch Life Sci, Guangzhou 510275, Guangdong, Peoples R China
[3] Univ Alberta, Dept Renewable Resources, Edmonton, AB T6G 2H1, Canada
基金
加拿大自然科学与工程研究理事会;
关键词
sky illumination; gap fraction; light availability; indirect site factor; exposure; LEAF-AREA; GAP FRACTION; EFFICIENT METHOD; CANOPY; EXPOSURE; INDEX;
D O I
10.1139/cjfr-2016-0003
中图分类号
S7 [林业];
学科分类号
0829 ; 0907 ;
摘要
Light environment estimates derived from hemispherical photography are known to be affected by variations in sky illumination. During photo acquisition, rapid changes in sky illumination can occur and will result in changes in detected canopy gap size and frequency. Any resulting problems in image consistency will become more serious with increased time lags between setting the reference exposure and hemispherical photograph acquisition. We showed that if the camera exposure setting was kept constant during photo acquisition, the estimated diffuse transmittance would be greatly influenced by sky illumination change. We developed a new pixel thresholding method that calculated the optimal threshold value for the separation of sky and plant pixels as a function of the above-canopy photosynthetic photon flux density (PPFD). We tested the performance of our method for estimating transmittance against two established methods that assume exposure to be held constant to two stops higher than the reference exposure. Our method compensates for changes in sky illumination, producing a smaller pixel threshold value when sky illumination decreases and a larger pixel threshold value when photographs are taken under increased sky illumination. The new method achieved accurate and reproducible results, even in situations where under-or over-exposure was caused by changes in sky illumination during photo acquisition.
引用
收藏
页码:1103 / 1110
页数:8
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