Spectral Distributions of Clear Sky Light and Their Chromaticities
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- Sekine Seishi
- Faculty of Engineering, Niigata University
Bibliographic Information
- Other Title
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- 晴天空光の分光分布と色度
- セイテンクウコウ ノ ブンコウ ブンプ ト シキド
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Abstract
The spectral power distribution of clear sky light varies mainly from the following factors: density of aerosol, solar altitude and angular distance from the sun, and reflected light from ground surface. This paper investigates these factors and effects about variation of clear sky light. The spectral power distributions of clear skies are not measured but calculated theoretically.<BR>The following is found out:<BR>(1) The chromaticities of daylight in high latitudes are distributed up to the higher range of correlated color temperature (CCT) than in low latitudes and many chromaticities of daylight in low latitudes are distributed at the low range of CCT compared with in high latitudes.<BR>(2) The chromaticities of north sky light in low latitudes are distributed slightly to green side at high CCT and a little to purple side at low CCT compared with the chromaticities of north sky light in high latitudes.<BR>(3) The difference between the distributions of chromaticities of daylight falling on a horizontal surface in high latitudes and is low latitudes is much smaller than the difference between distributions of chromaticities of north sky light in high latitudes and in low latitudes.
Journal
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- JOURNAL OF THE ILLUMINATING ENGINEERING INSTITUTE OF JAPAN
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JOURNAL OF THE ILLUMINATING ENGINEERING INSTITUTE OF JAPAN 73 (2), 39-45, 1989
The Illuminating Engineering Institute of Japan
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Details 詳細情報について
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- CRID
- 1390001204085504128
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- NII Article ID
- 130006766525
- 40004319974
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- NII Book ID
- AN00268860
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- ISSN
- 1349838X
- 21851506
- 00192341
- http://id.crossref.org/issn/00192341
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- NDL BIB ID
- 3216221
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- Data Source
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- JaLC
- NDL
- Crossref
- CiNii Articles
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- Abstract License Flag
- Disallowed