Bibcode
Tapia, M.; Cruz-González, I.; Avila, R.
Referencia bibliográfica
The 3rd Mexico-Korea Conference on Astrophysics: Telescopes of the Future and San Pedro Mártir (Eds. Stan Kurtz, José Franco, Seungsoo Hong, Guillermo García-Segura, Alfredo Santillán, Jongsoo Kim, & Inwoo Han) Revista Mexicana de Astronomía y Astrofísica (Serie de Conferencias) Vol. 28, pp. 9-15 (2007) (http://www.astroscu.unam.mx/~rmaa/)
Fecha de publicación:
6
2007
Número de citas
7
Número de citas referidas
3
Descripción
The Observatorio Astronómico Nacional at San Pedro Mártir
is located 31°02'40'' N and 115°28'00'' W on the summit of the
Sierra San Pedro Mártir in the Baja California peninsula, Mexico,
at 2800 m above sea level. The results of nearly three decades of site
characterization work are summarized. These cover the following aspects:
weather, cloud coverage, local meteorology, atmospheric optical
extinction, millimetric opacity, seeing, optical turbulence profiles,
wind profiles and 3D simulations of atmospheric turbulence. Overall, San
Pedro Mártir is one the most favorable sites in the world for
astronomical observations. Its excellent turbulence and local wind
conditions, to mention but two characteristics, make it particularly
well suited for large telescopes. Long-term monitoring of the site is
being undertaken by the National Autonomous University of Mexico and
other international institutions.