CAN THE LIDAR BE PLACED ON A SHIP OR ON AN AIRCRAFT?
Yes, thanks to its compacity the ALS can easily be put on a light
aircraft, on a light boat and a ship. In order to obtain the same results than
on the ground, the are two solutions to put the Lidar in a mobile
configurations:
-To put it on a mobile plate that conserve the horizontality anytime
-To record the rolling and pitching data (inertial central) during the
measurements so that the user can post correct the Lidar data with the aiming
angle.
CAN YOUR LIDAR BE USED FOR DAYTIME OBSERVATIONS? WHAT DETECTION (PHOTON
COUNTING OR ANALOG) ARE USED?
Of course our ALS can be used for daytime observations, and I want to point
out that compared to some micro joules Lidar systems, the ALS has a much
better efficiency. Indeed, with or without photon counting channel our Lidar
can be used with almost the same performances during day or night.
Leosphere's engineers managed to solve this daytime observation problem by
applying a multiple-step filtering method which reduces the background signal
down to a few percents. As a result, the ALS lidar provides data of almost the
same accuracy during daytime and night time.
This point is very important because daytime observation allows the user the
follow the PBL diurnal evolution and other parameter continuously, it also
allows to couple the Lidar with a photometer.
CAN I GET THE MASS CONCENTRATION OF THE AEROSOL?
Yes, thanks to nephelometers or in situ instruments, we can know the
specificities of reflection and absorption of the local particle volume.
Coupled to the Lidar extinction data, there is a scientific relation that has
been proved, which allows to get the mass concentration. If you need further
information please contact Laurent Sauvage: lsauvage@leosphere.fr .
WHAT PARAMETERS DOES THE SOFTWARE PROVIDE?
We do provide both processed and raw data.
The sequence that our software performs in quasi real time is the following:
From the raw signal, we compute a range corrected signal showing the structures
of aerosol and clouds. Then we calibrate the signal against a molecular
reference found in a clear sky area (without any cloud nor aerosols). We
eventually retrieve individual profiles for raw data, range corrected data
(PR2), extinction, optical depth, cloud & BL height. It can also display
the temporal evolution of PR2 data, cloud & BL and extinction against
height.