Characterization of the sodium layer at Cerro Pachon, and impact on laser guide star performance
Benoit Neichel (1), Celine D'Orgeville (2), Joseph Callingham (3),, Francois Rigaut (2), Claudia Winge (1), Gelys Trancho (4) ((1) Gemini, Observatory (2) Australian National University Research School of Astronomy

TL;DR
This study analyzes mesospheric sodium layer variations at Cerro Pachon using data from 2001 and GeMS operations, revealing significant temporal fluctuations affecting laser guide star performance and highlighting differences in laser efficiency over a decade.
Contribution
It provides a comprehensive comparison of sodium layer characteristics over a decade, linking sodium layer variability to laser guide star performance and efficiency.
Findings
Sodium photon return varies by a factor of 3-4 annually.
Sodium layer altitude shows large temporal variations.
Laser format efficiency has significantly changed over ten years.
Abstract
Detailed knowledge of the mesopheric sodium layer characteristics is crucial to estimate and optimize the performance of Laser Guide Star (LGS) assisted Adaptive Optics (AO) systems. In this paper, we present an analysis of two sets of data on the mesospheric sodium layer. The first set comes from a laser experiment that was carried out at Cerro Tololo to monitor the abundance and altitude of the mesospheric sodium in 2001, during six runs covering a period of one year. This data is used to derive the mesospheric sodium column density, the sodium layer thickness and the temporal behavior of the sodium layer mean altitude. The second set of data was gathered during the first year of the Gemini MCAO System (GeMS) commissioning and operations. GeMS uses five LGS to measure and compensate for atmospheric distortions. Analysis of the LGS wavefront sensor data provides information about the…
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