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Database: 365,228(8 Aug 2026)
daylight-cie standard general sky scopethis standard clear sky patchy cloudy sky spatial distribution sky additive δ-undecalactone ministerial-level transportation safety emergency platform prebaked blocks
GB/T 20148-2006 in English

GB/T 20148-2006 in English

VALID

Spatial distribution of daylight-CIE standard general sky

  • Issued on:2006-03-06
  • Implemented on:2006-11-01
  • File Format:PDF
  • Delivery:Via email within 1~3 business days
Price(USD): $130.00
$127.00
Standard No: GB/T 20148-2006
Document status: VALID
Title in English: Spatial distribution of daylight-CIE standard general sky
Title in Chinese: 日光的空间分布 CIE一般标准天空
Language: English
File Format: Electronic (PDF)
Delivery: Via email within 1~3 business days
Issued on: 2006-03-06
Implemented on: 2006-11-01
ICS Classification: 17.180.20-Colours and measurement of light
Chinese Classification: K70-Electric lighting in general
Professional Classification: GB-National Standard
Related Keywords: daylight-cie standard general sky scopethis standard
clear sky
patchy cloudy sky
spatial distribution
sky
Related Topics: sunlight
sky
GB/t 20148-2006
Sky
Spatial distribution
Standard Daylight Spectrum
Spatial distribution
Guangguang Day Index Formula
distribution of space
space version
Spatial distribution of secondary electrons
electron spatial distribution
Confined Space One Point One Volume
daytime accuracy
light space
day+
GBT20148
GBT20148-2006
Flash distribution standard average
general standard sky
air quality standards japan
gbt20148
gbt20148-2006

《GB/T 20148-2006日光的空间分布 CIE一般标准天空》由TC224(全国照明电器标准化技术委员会)归口,TC224SC4(全国照明电器标准化技术委员会照明基础分会)执行,主管部门为中国轻工业联合会。
本标准规定了一组从理论和实际应用上均与太阳光和天棚照明有联系的室外日光条件。 所给定的亮度分布具有下述特性: i)它们都对称于太阳子午线,并且均为太阳和天顶之间的角距离ZS的函数。 ii)它们被定义为平滑连续的函数。 iii)天空中任一点的相对亮度取决于该天空的面与太阳之间的角度x以及该天空面与天顶之间的角度Z。


Scope

This standard specifies a set of outdoor daylight conditions that are theoretically and practically related to sunlight and ceiling lighting. The given luminance distributions have the following characteristics: 1) They are all symmetrical about the solar meridian and are a function of the angular distance ZS between the sun and the zenith. 2) They are defined as smooth continuous functions. This distribution of brightness is typical of a clear sky, characterized by clouds that are monochromatic. They provide an approximation of a patchy cloudy sky that is accurate enough for many practical daylight calculations. 3) The relative brightness of any point in the sky depends on the angle x between the bin of the sky and the sun and the angle Z between the bin of the sky and the zenith. This relative brightness is given by two functions: the relative scattering characteristic curve f(x) and the brightness hue Φ(Z) between the viewing distance and the zenith.

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