烛光与织女星可见距离的一种新方法及其在室外照明中的应用

Uthayakaren (Uthayan) Thurairajah
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引用次数: 0

摘要

了解人类视觉系统的夜间表现对于设计夜间行车的安全照明至关重要。能见度是一个复杂的评估过程,但我们目前对眼睛如何接收和处理光线以及眼睛在不同光照水平和距离下区分物体的能力的了解还很低。目前计算室外照明水平要求的方法很复杂,仅限于照度和亮度测量,并且不允许设计师评估能见度。本文的目的是建立一个简单的室外照明能见度计算,使用光子每秒。将该计算方法应用于烛光的可见距离和银河系织女星的可见性,验证了该计算方法的正确性。本文将帮助研究人员、科学家、工程师、顾问、建筑师、照明设计师和政府机构寻求改善室外照明,以提高建筑环境中的安全、健康、福祉和生活质量。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
A Novel Method to Prove the Visibility Distance of Candlelight and the Milky Way’s Vega Star and Apply this Knowledge to Outdoor Lighting Applications
Understanding the human visual system’s night-time performance is essential for designing safe lighting for night-time travel. Visibility is a complex assessment process, but our current understanding of how the eye receives and processes light and how well the eye can distinguish objects in different lighting levels and distances are low. The current approach for calculating outdoor lighting level requirements is complicated and limited to illuminance and luminance measurements and does not allow designers to evaluate visibility. This paper aims to develop a simple outdoor lighting visibility calculation using the photons per second. This novel calculation method is applied to the candlelight's visibility distance and the milky way’s Vega star visibility to validate the calculation approach. This paper will help researchers, scientists, engineers, consultants, architects, lighting designers, and government agencies seeking to improve outdoor lighting for safety, health, well-being, and quality of life in the built environment.
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