National Institute of R&D for Optoelectronics INOE 2000
Remote Sensing Department

 

Report 2007: Study of the Cloud Albedo Related to Microphysical Properties of Clouds

 

LiSA System description

 

LiSA system is a backscattering Lidar. It can work separately or simultaneous on two wavelengths. The operating principle consists in emitting of a short pulse of light in the atmosphere, followed by the registration of backscattered radiation as function of distance.
The system is useful to study the lower troposphere, including the planetary boundary layer.

The main component of the emission block is a pulsed, Q-switched YAG:Nd laser, which produces short pulses (6 ns length) in a beam with 0.5 mrad divergence. A part of emitted laser pulse is utilized as marker of ‘zero’ time (the reference signal to normalize the return signal, when the reproducibility of laser emission is not proper). The backscattered field collected by the receiver optics is passed through a spectrum analyzer, which selects only the specific wavelength interval of interest for the application, in order to minimize the background radiation contribution.  The electric signal generated by photodetectors is electronically synchronized, amplified and converted in digital signal, which is finally delivered to a PC for processing. 

 

Technical Data

Emitter

YAG:Nd laser

Working wavelengths

1064, 532 nm

Pulse energy at 1064 nm

up to 100mJ

Pulse energy at 532 nm

up to 50 mJ

Pulse repetition rate

max. 20 Hz

Pulse length

10 - 12 ns

Angular beam divergence

1.5 mrad

Receiver

Quasi-Cassegrain type telescope

Main mirror diameter

260 mm

Field of view

2.5 - 18 '

Focal length

1054 mm

Halfwidth of interference filters

2.6 nm (at 1064 nm), 2.5 nm (at 532 nm)

Spatial resolution

6 m

Length of sensing path

10 Km