Published July 14, 2008 | Version Published
Book Section - Chapter Open

Telluric sodium layer temporal variations

  • 1. ROR icon University of Hawaii at Manoa
  • 2. ROR icon Durham University
  • 3. ROR icon National Autonomous University of Mexico

Abstract

We present observations of the high-speed variations of the altitude of the telluric sodium layer. In this experiment we observed the Gemini-North sodium laser guide star from approximately 80 meters off-axis using the UH-2.2m telescope on Mauna Kea, Hawaii. Observations were made using an electron-multiplying camera at a rate of about 100Hz. The temporal power spectrum of the layer centroid follows a power law between 0.001 and 1Hz and we find that the exponent of the power law (α=-1.8) is similar to that found at lower temporal frequencies from lidar experiments. This data set taken with the lidar results shows that the power spectrum of the sodium layer mean altitude follows a simple power law over 5 orders of magnitude from 10^(-4.5) Hz to 1Hz. The approach taken in this experiment is difficult due to telescope jitter in any of the three telescopes (Gemini-N, Gemini-N LGS launch telescope, or from the observing UH2.2m) and atmospheric tip/tilt wave front aberrations. We circumvented these problems by analyzing the differential motion between two distinct features that appeared in the sodium layer during that night.

Additional Information

© 2008 Society of Photo-Optical Instrumentation Engineers.

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Eprint ID
91870
Resolver ID
CaltechAUTHORS:20181217-141800632

Dates

Created
2018-12-18
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Updated
2021-11-16
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Caltech groups
Thirty Meter Telescope
Series Name
Proceedings of SPIE
Series Volume or Issue Number
7015