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          Institute: MPI für Astronomie     Collection: Publikationen_mpia     Display Documents



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ID: 198520.0, MPI für Astronomie / Publikationen_mpia
3D optical turbulence characterization at San Pedro Mártir
Authors:Masciadri, E.; Avila, R.; Sánchez, L. J.; Cuevas, S.; Garfias, F.; Agabi, A.; Azouit, M.; Vernin, J.
Date of Publication (YYYY-MM-DD):2003
Title of Journal:Revista Mexicana DE Astronomia y Astrofisica. Conference Series
Journal Abbrev.:Revista Mexicana de Astronomia y Astrofisica. Conference Series
Volume:19
Start Page:63
End Page:71
Sequence Number of Article:2003RMxAC..19...63M
Review Status:not specified
Audience:Experts Only
Abstract / Description:Many instruments are able to provide local (in
space and time) estimations of all the
astroclimatic parameters that depend on the
optical turbulence. The numerical technique is,
at the present time, the only approach that can
provide 3D characterization of the optical
turbulence. Since a few years, many efforts have
been dedicated to increase the reliability of the
atmospherical meso-scale model called Meso-Nh in
simulating C[N]2 profiles above astronomical
sites. The most recent and promising results have
been obtained above the San Pedro Mártir site. In
this paper these results are summarized.
Free Keywords:Atmospheric effects; Instrumentation: adaptive
; optics; Site testing; Turbulence
External Publication Status:published
Document Type:Article
Version Comment:Automatic journal name synchronization
Communicated by:N. N.
Affiliations:MPI für Astronomie
Identifiers:URL:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bi... [ID No:1]
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