High altitude wind velocity at San Pedro Martir and Mauna Kea

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dc.creatorCarrasco, Esperanza
dc.creatorSarazin, Marc
dc.date2003-08-29
dc.date2003-09-03
dc.date.accessioned2026-07-07T02:09:21Z
dc.date.available2026-07-07T02:09:21Z
dc.descriptionWe analyze the monthly average wind velocity at about 12 km above sea level, between 1980 to 1995, for San Pedro Martir, Mauna Kea, another existing observatorie and some sites of interest. We compare the results obtained from two different data sets, the GGUAS and NCEP. Our results show that San Pedro Martir and Mauna Kea are comparable and are amongst the most suitable sites to apply slow wavefront corrugation correction techniques
dc.description5 pages, 1 figure. To appear in "San Pedro Martir: AStronomical Site Evaluation (2003)", Rev Mex AA (SC)
dc.identifierhttps://arxiv.org/abs/astro-ph/0309002
dc.identifierhttp://arxiv.org/abs/astro-ph/0309002
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6403
dc.subjectAstrophysics
dc.titleHigh altitude wind velocity at San Pedro Martir and Mauna Kea
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