Measurements of nighttime atmospheric optical depth preliminary data from a mountain site in southern Italy

被引：14
|
作者：
Esposito, F
Serio, C
Pavese, G
Auriemma, G
Satriano, C
机构：
[1] Univ Basilicata, Dipartimento Ingn & Fis Ambiente, I-85100 Potenza, Italy
[2] CNR Tito, Ist Metodol Avanzate Anal Ambientali, Potenza, Italy
[3] Ist Nazl Fis Nucl, Sez Roma, Rome, Italy
[4] Univ Basilicata, Potenza, Italy
来源：
JOURNAL OF AEROSOL SCIENCE | 1998年 / 29卷 / 10期
关键词：
D O I：
10.1016/S0021-8502(98)00011-1
中图分类号：
TQ [化学工业];
学科分类号：
0817 ;
摘要：
A grating spectrometer equipped with a photomultiplier was used to measure atmospheric optical depth with the moon as an extraterrestrial light source. Measurements are presented in the window regions in the spectral range 0.32-0.64 mu m, with a resolution of about 3 nm. The Langley method was applied to estimate atmospheric optical depth. Measurements have been performed at a mountain site in southern Italy, at 1247 m above sea level in the context of the Gamma-ray Air-Cherenkov Multi Telescope experiment. (C) 1998 Elsevier Science Ltd. All rights reserved.
引用
收藏
页码：1213 / 1218
页数：6
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