Université de Fribourg

Site selection for OWL using past, present, and future climate information

Graham, Edward ; Sarazin, Marc S. ; Beniston, Martin ; Collet, Claude ; Hayoz, Michael ; Neun, Moritz ; Goyette, Stéphane

In: Proceedings of SPIE, 2004, vol. 5489, p. 102

Selection of an ideal site for the new generation of Overwhelmingly Large (OWL) telescopes is dependent on many climatological and meteorological parameters. Among these are cloud cover, atmospheric humidity, aerosol content, air temperature, airflow direction, strength and turbulence. Even relatively minor changes in weather patterns can have a significant effect on seeing conditions. A...

Université de Fribourg

Homogenisation of a Canadian surface pressure database

Graham, Edward ; Slonosky, Victoria

This paper describes the collection, checking and homogenisation of a Canadian atmospheric surface pressure database. The object of the exercise was to create a database of monthly mean surface pressure for as many stations as possible across Canada as far back in time as possible. Data sources included the World Weather Records, Monthly Climatic Data for the World Bulletins, the Global...

Université de Fribourg

Canadian pressure observations and circulation variability: links to air temperature

Slonosky, Victoria C. ; Graham, Edward

In: International Journal of Climatology, 2005, vol. 25(11), p. 1473

A set of 71 station series of surface pressure from Canada and Greenland have been examined for quality control and homogeneity. These records range in length from 50 to 130 years. The object of this exercise was to investigate station-based surface pressure series and atmospheric circulation on a decadal time scale, and to examine the effects of the atmospheric circulation on climate. The data...

Université de Fribourg

Climate-based site selection for a very large telescope using GIS techniques

Graham, Edward ; Sarazin, Marc S. ; Beniston, Martin ; Collet, Claude ; Hayoz, Michael ; Neun, Moritz ; Casals, Paula

In: Meteorological Applications, 2005, vol. 12, p. 77

Astronomical research at present requires that a telescope with an aperture diameter of between 50 and 100 metres be constructed within the next 10 years or so. This new generation of telescopes will be called OWL (Overwhelmingly Large), and it represents one order of magnitude increase in size over today's telescopes. Selection of an ideal site for this giant telescope is dependent on many...