A Two-Dimensional Brightness Distribution of the Visible Zodiacal Light

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作者：
SMKwon SSHong JLWeinberg Dept of Science Education Kangwon Nat Univ Chunchon KOREA Department of Astronomy Seoul Nat Univ Seoul KOREA Technology Care Givers SnellvilleG A USA [1 ,2 ,3 ,1 ,200 ,701 ,2 ,151 ,742 ,3 ,30039 ]
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云南天文台台刊 | 1999年 / S1期
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P183 [地球];
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摘要：
By adopting a recently developed semi empirical methodology for removing the atmospheric diffuse light and an improved technique of individual star subtraction, we have newly reduced the distribution of the visible zodiacal light (ZL) brightness from almucantar scan observations of the night sky brightness at Mt. Haleakala, Hawaii. The resulting two dimensional map of the ZL brightness covers the sky over 40°≤λ-λ ⊙≤320° and -40°≤β≤40° and its angular resolution 2°×2°is fine enough to reveal optical counterparts of the structures in the zodiacal emission first found from the IRAS space observations.
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页码：269 / 273
页数：5
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