Automatically guiding a telescope to a laser beam on a biaxial antarctic light detection and ranging system

The operating principle of atmospheric Rayleigh LIDAR (light detection and ranging) systems is that the range-corrected return-backscatter signal is directly related to atmospheric density. For this to be the case full overlap is required between the backscattered laser signal and the field of view...

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Published in:Optical Engineering
Main Authors: Innis, J., Cunningham, A., Graham, A., Klekociuk, A.
Format: Article in Journal/Newspaper
Language:English
Published: SPIE 2007
Subjects:
Online Access:http://hdl.handle.net/2440/89873
https://doi.org/10.1117/1.2801411
id ftunivadelaidedl:oai:digital.library.adelaide.edu.au:2440/89873
record_format openpolar
spelling ftunivadelaidedl:oai:digital.library.adelaide.edu.au:2440/89873 2023-12-17T10:20:40+01:00 Automatically guiding a telescope to a laser beam on a biaxial antarctic light detection and ranging system Innis, J. Cunningham, A. Graham, A. Klekociuk, A. 2007 http://hdl.handle.net/2440/89873 https://doi.org/10.1117/1.2801411 en eng SPIE Optical Engineering, 2007; 46(11):16001-1-16001-8 0091-3286 1560-2303 http://hdl.handle.net/2440/89873 doi:10.1117/1.2801411 Klekociuk, A. [0000-0003-3335-0034] © 2007 SPIE http://dx.doi.org/10.1117/1.2801411 LIDAR LIDAR alignment autoguiding telescopes Journal article 2007 ftunivadelaidedl https://doi.org/10.1117/1.2801411 2023-11-20T23:17:38Z The operating principle of atmospheric Rayleigh LIDAR (light detection and ranging) systems is that the range-corrected return-backscatter signal is directly related to atmospheric density. For this to be the case full overlap is required between the backscattered laser signal and the field of view of the receive telescope. Time-dependent errors in this alignment compromise the experimental method, and confuse the interpretation of geophysical signals present in the data. We describe a means of locking the alignment of a small LIDAR telescope to the backscattered laser beam, using images obtained with a commercial charge-coupled device camera, to reduce the effects of relative movement of telescope and laser on field overlap. This “autoguiding” system is implemented on a biaxial Rayleigh LIDAR in operation in Antarctica. We achieve a positional precision near 3 camera pixels (1 pixel ~ 1 arc) across the beam, and 7 camera pixels along the beam. Positional corrections are generated once per minute. The system is capable of removing medium- and long-term drifts in the relative alignment of our telescope and laser during an observing run. John Innis, Andrew Cunningham, Anthony Graham, Andrew Klekociuk Article in Journal/Newspaper Antarc* Antarctic Antarctica The University of Adelaide: Digital Library Antarctic Optical Engineering 46 11 116001
institution Open Polar
collection The University of Adelaide: Digital Library
op_collection_id ftunivadelaidedl
language English
topic LIDAR
LIDAR alignment
autoguiding
telescopes
spellingShingle LIDAR
LIDAR alignment
autoguiding
telescopes
Innis, J.
Cunningham, A.
Graham, A.
Klekociuk, A.
Automatically guiding a telescope to a laser beam on a biaxial antarctic light detection and ranging system
topic_facet LIDAR
LIDAR alignment
autoguiding
telescopes
description The operating principle of atmospheric Rayleigh LIDAR (light detection and ranging) systems is that the range-corrected return-backscatter signal is directly related to atmospheric density. For this to be the case full overlap is required between the backscattered laser signal and the field of view of the receive telescope. Time-dependent errors in this alignment compromise the experimental method, and confuse the interpretation of geophysical signals present in the data. We describe a means of locking the alignment of a small LIDAR telescope to the backscattered laser beam, using images obtained with a commercial charge-coupled device camera, to reduce the effects of relative movement of telescope and laser on field overlap. This “autoguiding” system is implemented on a biaxial Rayleigh LIDAR in operation in Antarctica. We achieve a positional precision near 3 camera pixels (1 pixel ~ 1 arc) across the beam, and 7 camera pixels along the beam. Positional corrections are generated once per minute. The system is capable of removing medium- and long-term drifts in the relative alignment of our telescope and laser during an observing run. John Innis, Andrew Cunningham, Anthony Graham, Andrew Klekociuk
format Article in Journal/Newspaper
author Innis, J.
Cunningham, A.
Graham, A.
Klekociuk, A.
author_facet Innis, J.
Cunningham, A.
Graham, A.
Klekociuk, A.
author_sort Innis, J.
title Automatically guiding a telescope to a laser beam on a biaxial antarctic light detection and ranging system
title_short Automatically guiding a telescope to a laser beam on a biaxial antarctic light detection and ranging system
title_full Automatically guiding a telescope to a laser beam on a biaxial antarctic light detection and ranging system
title_fullStr Automatically guiding a telescope to a laser beam on a biaxial antarctic light detection and ranging system
title_full_unstemmed Automatically guiding a telescope to a laser beam on a biaxial antarctic light detection and ranging system
title_sort automatically guiding a telescope to a laser beam on a biaxial antarctic light detection and ranging system
publisher SPIE
publishDate 2007
url http://hdl.handle.net/2440/89873
https://doi.org/10.1117/1.2801411
geographic Antarctic
geographic_facet Antarctic
genre Antarc*
Antarctic
Antarctica
genre_facet Antarc*
Antarctic
Antarctica
op_source http://dx.doi.org/10.1117/1.2801411
op_relation Optical Engineering, 2007; 46(11):16001-1-16001-8
0091-3286
1560-2303
http://hdl.handle.net/2440/89873
doi:10.1117/1.2801411
Klekociuk, A. [0000-0003-3335-0034]
op_rights © 2007 SPIE
op_doi https://doi.org/10.1117/1.2801411
container_title Optical Engineering
container_volume 46
container_issue 11
container_start_page 116001
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