当前位置:
X-MOL 学术
›
J. Quant. Spectrosc. Radiat. Transf.
›
论文详情
Our official English website, www.x-mol.net, welcomes your
feedback! (Note: you will need to create a separate account there.)
Quantifying the visual impact of wind farm lights on the nocturnal landscape
Journal of Quantitative Spectroscopy and Radiative Transfer ( IF 2.3 ) Pub Date : 2024-09-25 , DOI: 10.1016/j.jqsrt.2024.109203 Salvador Bará, Raul C․ Lima
Journal of Quantitative Spectroscopy and Radiative Transfer ( IF 2.3 ) Pub Date : 2024-09-25 , DOI: 10.1016/j.jqsrt.2024.109203 Salvador Bará, Raul C․ Lima
Wind farm lights are a conspicuous feature in the nocturnal landscape. Their presence is a source of light pollution for residents and the environment, severely disrupting in some places the aesthetic, cultural, and scientific values of the pristine starry skies. In this work we present a simple model for quantifying the visual impact of individual wind turbine lights, based on the comparison of their brightness with the brightness of well-known night sky objects. The model includes atmospheric and visual variables, and for typical parameters it shows that medium-intensity turbine lights can be brighter than Venus up to ∼4 km from the turbine, brighter than α CMa (the brightest star on the nighttime sky) until about ∼10 km, and reach the standard stellar visibility limit for the unaided eye (m v = +6.00) at ∼38 km. These results suggest that the visual range of wind farms at nighttime may be significantly larger than at daytime, a factor that should be taken into account in environmental impact assessments.
中文翻译:
量化风电场灯光对夜间景观的视觉影响
风电场灯是夜间景观中的一个显着特征。它们的存在是居民和环境的光污染源,在一些地方严重破坏了原始星空的美学、文化和科学价值。在这项工作中,我们提出了一个简单的模型,基于它们的亮度与众所周知的夜空物体的亮度的比较,量化单个风力涡轮机灯的视觉影响。该模型包括大气和可见变量,对于典型参数,它表明中等强度涡轮灯在距离涡轮机约 4 公里处可能比金星更亮,在大约 ∼10 公里处比 α CMa(夜空中最亮的恒星)更亮,并在 ∼38 公里处达到肉眼的标准恒星能见度极限 (mv = +6.00)。这些结果表明,风电场在夜间的视野范围可能明显大于白天,这是环境影响评估中应考虑的一个因素。
更新日期:2024-09-25
中文翻译:
量化风电场灯光对夜间景观的视觉影响
风电场灯是夜间景观中的一个显着特征。它们的存在是居民和环境的光污染源,在一些地方严重破坏了原始星空的美学、文化和科学价值。在这项工作中,我们提出了一个简单的模型,基于它们的亮度与众所周知的夜空物体的亮度的比较,量化单个风力涡轮机灯的视觉影响。该模型包括大气和可见变量,对于典型参数,它表明中等强度涡轮灯在距离涡轮机约 4 公里处可能比金星更亮,在大约 ∼10 公里处比 α CMa(夜空中最亮的恒星)更亮,并在 ∼38 公里处达到肉眼的标准恒星能见度极限 (mv = +6.00)。这些结果表明,风电场在夜间的视野范围可能明显大于白天,这是环境影响评估中应考虑的一个因素。