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History of the daylight criteria conditions influencing new methods for the determination of interior daylighting

机译:日光标准的历史条件影响着确定室内日光的新方法

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Determination of sunlight and skylight availability and utilization may be based only on the characteristics of the sun and sky as natural sources of daylight. Sun as a primary source of light has been studied for centuries with gradually accumulating knowledge concerning the sun position on the sky vault in different geographical locations and various time periods. Extraterrestrial solar energy flow towards the Earth's atmosphere was determined in the form of the Solar Constant and horizontal sunlight illuminance under various changes in time, solar altitude and atmospheric conditions. Skylight from the whole sky vault is the largest spacious source of diffuse daylighting in building interiors. Historic achievements of its determination by sky luminance patterns was first defined by Lambert with unity uniform sky luminance as the simplest standard with the possibility of determining relative Sky Factor criterion. Modelling of the whole range of sky types is possible by applying gradation luminance patterns and determination of their gradation functions, with scattering of sun beams in different space directions and is determined by indicatrix functions. Relative luminance sky patterns of different sky types is now standardized and normalized by zenith luminance. However, it is possible to define zenith luminance and horizontal illuminance in absolute physical units, thus to change daylight criteria from relative values of the Daylight Factor to interior physical illuminance in lux. This paper shows the historical progress, developments in measuring sunlight and skylight sources and the current state of art.
机译:确定日光和天窗的可用性和利用率可能仅基于作为自然日光源的太阳和天空的特征。关于太阳作为主要光源的研究已有数百年之久,并逐渐积累了有关不同地理位置和不同时间段的天穹上太阳位置的知识。在时间,太阳高度和大气条件的各种变化下,以太阳常数和水平太阳照度的形式确定了流向地球大气层的地外太阳能流。整个穹顶的天窗是建筑物内部弥散采光的最大空间。兰伯特首先以天空亮度模式确定其历史性成就,以统一的均匀天空亮度为最简单的标准,并有可能确定相对的天空因子标准。通过应用灰度亮度模式并确定其灰度函数,以及在不同空间方向上散射太阳光束,可以对整个天空类型进行建模,并由指示函数确定。现在,通过天顶亮度对不同天空类型的相对亮度天空模式进行标准化和标准化。但是,可以以绝对物理单位定义天顶亮度和水平照度,从而将日光标准从“日光因子”的相对值更改为以勒克斯为单位的内部物理照度。本文介绍了在测量日光和天光源方面的历史进展,发展以及当前的技术水平。

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