A dynamically ranged pulsed Rayleigh beacon using sensed wavefronts
across a system’s pupil plane is proposed for tomographic
quantification of the atmospheric turbulence strength. This method
relies on relaying light from a telescope system’s pupil plane to a
wavefront sensor and having precise control of the light-blocking
mechanisms to filter out scattered light from the unwanted scattering
regions along the propagation path. To accomplish this, we tested and
incorporated design features into the sensing system that we believe,
to the best of our knowledge, are unique. Dynamically changing the
range of the beacon source created focal shifts along the optical axis
in the telescope sensing system. This effect induced polarization
degradation in the optical pupil. As a result, polarization
nonuniformity within the Pockels cell resulted in light leakages that
corrupted the sensed data signals. To mitigate this unwanted effect,
an analysis of the polarization pupil had to be completed for the
range of possible Rayleigh beacon source distances, relating the
change in polarization to the ability of a Pockels cell to function as
an optical shutter. Based on the resultant polarization pupil
analysis, careful design of the light relay architecture of the
sensing system was necessary to properly capture sensed wavefront data
from a series of intended ranges. Results are presented for the
engineering design of the Turbulence and Aerosol Research Dynamic
Interrogation System sensing system showing the choices made within
the trade space and how those choices were made based on an analysis
of the polarization pupil. Based on what we learned, recommendations
are made to effectively implement a polarization-based Pockels cell
shutter system as part of a dynamically ranged Rayleigh beacon
system.