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Second Backaskog Workshop on Extremely Large Telescopes
Numerical simulations of airflow over various potential sites for extremely large telescopes have been performed. Information such as wind speed, turbulence levels (fluctuating velocity RMS), wake lengths, boundary (ground) layer thickness and the effects of topographically induced turbulence on "seeing" can be retrieved, thus providing an essential evaluation tool in the site selection process. We present a sample set of simulations carried out over possible site locations for adoi:10.1117/12.566346 fatcat:rzd3f7hkhfadjp5vkvufqmfc2y