Using the ${C_{n}^{2}}$ and wind profiler method with wide-field laser-guide-stars adaptive optics to quantify the frozen-flow decay-Reference-Cited by-同舟云学术

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Using the ${C_{n}^{2}}$ and wind profiler method with wide-field laser-guide-stars adaptive optics to quantify the frozen-flow decay

Published:2014-04-03 Issue:3 Volume:440 Page:1925-1933
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Guesalaga Andrés¹,Neichel Benoit²³,Cortés Angela¹,Béchet Clémentine¹,Guzmán Dani¹

Affiliation:

1. Pontificia Universidad Católica de Chile, 4860 Vicuña Mackenna, Casilla 7820436, Santiago, Chile

2. Gemini Observatory Southern Operations Center, Colina el Pino s/n, Casilla 603, La Serena, Chile

3. Aix Marseille Université, CNRS, Laboratoire d'Astrophysique de Marseille (LAM) UMR 7326, F-13388 Marseille, France

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/440/3/1925/23991353/stu366.pdf

Reference30 articles.

1. Modelling the optical turbulence boiling and its effect on finite-exposure differential image motion

3. Determination of the profile of atmospheric optical turbulence strength from SLODAR data

4. Wave-front temporal spectra in high-resolution imaging through turbulence

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