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Turbulence and Seeing measurements at Dome C A collaboration UNSW, CTIO and the University of Nice
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What did we learn at the South Pole?
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South Pole 2001……and Dome C 2003
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The boundary layer cycle
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The cycle in the Dome C Summer 00:0006:0012:0000:0018:0006:0012:0000:0018:00 1.0 0.8 0.0 0.4 1.2 1.6 Best seeing when: 1) Minimum radiation from the Sun 2) Minimum Thermal gradient
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The cycle in the Dome C Summer
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Free atmosphere turbulence
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Effect of the high altitude wind: Paranal
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MASS first data 24/03
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Seeing Mauna Kea Paranal
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Isoplanatic Angle Paranal
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Coherence Time
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Conclusion Already spectacular Seeing values, expected to improve in winter Very advantageous ground level turbulence profile Need more data to conclude on the isoplanatic angle and coherence time
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