Published August 25, 2017
| Version v1
Journal article
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Using paraxial approximation to describe the optical setup of a typical EARLINET lidar system
Authors/Creators
- 1. Institute of Astronomy, Astrophysics, Space Applications and Remote Sensing, National Observatory of Athens, 15236, Greece
Description
The mathematical formulation for the optical setup of a typical
EARLINET lidar system is given here. The equations describing a lidar system
from the emitted laser beam to the projection of the telescope aperture on
the final receiving unit (i.e., photomultiplier or photodiode) are presented,
based on paraxial approximation and geometric optics approach. The receiving
optical setup includes a telescope, a collimating lens, an interference
filter and the ensemble objective eyepiece. The set of the derived equations
interconnects major parameters of the optical components (e.g., focal lengths,
diameters, angles of incidence), revealing their association with the
distance of full overlap of the system. These equations may used
complementarily with an optical design software, for the preliminary design
of a system or can be used as a quick check up tool of an existing lidar
system. The evaluation of the formulation on a real system is performed with
ray-tracing simulations, revealing an overall good performance with relative
differences of the order of 5 % mainly attributed to the limitations of the
thin lens approximation.
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