Efficiency of off-axis astronomical adaptive systems: Comparison of experimental data for different astronomical sites


Por: Sanchez L.J., VOYTSEKHOVICH, VALERY, Orlov V.G., Avila R., Cuevas S.

Publicada: 1 ene 2000
Resumen:
The efficiency of off-axis adaptive astronomical systems is estimated for four astronomical sites: Paranal (Chili), Roque de los Muchachos (Canary Islands), San Pedro Matrtir (Mexico) and Observatoire de Haute Provence (France). The efficiency of interest is considered through the Strehl ratio of the corrected image calculated for V, J and K bands and for 8-m class telescopes. The experimental optical turbulence strength Cn 2(z) profiles necessary for calculations have been measured with balloon flights and with the Generalized Scidar. It is found that this efficiency depends mainly on the Cn 2(Z) profile layered structure and on the turbulence strength.

Filiaciones:
Sanchez L.J.:
 UNAM, Mexico, Mexico

Orlov V.G.:
 UNAM, Mexico, Mexico

Avila R.:
 UNAM, Mexico, Mexico

Cuevas S.:
 UNAM, Mexico, Mexico
ISSN: 0277786X
Editorial
SPIE-INT SOC OPTICAL ENGINEERING, 1000 20TH ST, PO BOX 10, BELLINGHAM, WA 98227-0010 USA, Estados Unidos America
Tipo de documento: Conference Paper
Volumen: 4007 Número:
Páginas:

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