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LINKS TO GLOBAL DATA |
Potential astronomical sites are of interest for ESO and other institutions in the frame of the site surveys for ELT class telescopes. These telescopes might have particular requirements excluding some of the best existing observatories (eg. seismology: the current OWL design cannot survive the earthquakes foreseen during the next 50 years in northern Chile). For this reason the first phase of the site survey shall be global: state of the art databases in meteorology, geography, seismology and climatology shall be merged to build a specific tool capable to extract all locations fulfilling a given set of minimum characteristics determined by the project. The validity of the underlying assumptions shall be demonstrated on existing observatories (eg: is climatology capable to explain the climate change of the last decade at Paranal?). The site extraction tool, a Geographical Information System (GIS) shall be used in the course of the OWL design phase to reflect the consequence of engineering and operation parameters onto the density of available sites and their relative quality. For example, if OWL can produce science ONLY when operated with adaptive optics assisted by laser guide stars, it will not work in slightly cloudy (so-called spectroscopic) sky because of the laser backscattering. Only in the last phase of the site survey should field measurements be conducted on a few selected sites. In this phase, data collected previously by other teams are of course of high interest provided that the instruments used are of acknowledged accuracy. See the summary power point presentation: "A Nest for OWL"
Cloud Cover
Sub-tropical Jet Stream
Aerosols
Sky Background
Climate variability
Intertropical Convergence Zone
South American Monsoon System (SAMS)
El Nino Southern Oscillation
The ESPAS LIBRARY
contains data on particular sites of interest.
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