LIDAR system of CLF

被引：0
作者：
Oku, D. [1 ]
Tomida, T. [1 ]
机构：
[1] Univ Yamanashi, Interdisciplinary Grad Sch Med & Engn Mech Syst E, Kofu, Yamanashi 4008511, Japan
来源：
INTERNATIONAL SYMPOSIUM ON THE RECENT PROGRESS OF ULTRA-HIGH ENERGY COSMIC RAY OBSERVATION | 2011年 / 1367卷
关键词：
UHECR; Fluorescence; Atomspheric minitoring; LIDAR; Central Laser Facility;
D O I：
10.1063/1.3628735
中图分类号：
O59 [应用物理学];
学科分类号：
摘要：
UV fluorescence light generated by an air shower is scattered and lost along the path of propagation to the telescope. The cause of the main scattering is due to the atmospheric molecule and the aerosol. The calibration of a decrease in the photocount by scattering the atmosphere is very important as well as the calibration of the Fluorescence Detectors (FD). Two atmospheric scattered monitoring devices (LIDAR and CLF) have already been operating in the Telescope Array (TA) experiment. New LIDAR system is constructed at CLF and concentrated the advantage of two current atmospheric transparency monitoring devices. It reports on the upgrade of an existing atmospheric scattered monitoring device in TA in this paper.
引用
收藏
页码：161 / 164
页数：4
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