Add to ORKGThe turbulence structure of the atmosphere is the primary limitation to adaptive optics system performance on extremely large telescopes — driving current world-wide site testing campaigns. The potential for adaptive optics correction on extremely large telescopes located at Dome C station on the Antarctic plateau is investigated here. Due to the unique atmospheric characteristics of this site it is found that a natural guide star adaptive optics system with a single deformable mirror should outperform a multi-conjugate multi-laser guide star system at a mid-latitude site
Modeling of astronomically important atmospheric parameters, and the impact these parameters have on...
The high plateau that covers half of the continent of Antarctica contains the best astronomical obse...
From the South Pole, microthermal turbulence within a narrow surface boundary layer some 200 m thic...
The turbulence structure of the atmosphere is the primary limitation to adaptive optics system perfo...
Abstract. The turbulence structure of the atmosphere is the primary limitation to adaptive optics sy...
The performance of natural guide star adaptive-optics systems for telescopes located on the Antarcti...
The unique atmospheric characteristics found at Dome C on the Antarctic plateau offer significant ad...
The unique atmospheric characteristics found at Dome C on the Antarctic plateau offer significant ad...
The unique atmospheric characteristics found at Dome C on the Antarctic plateau offer significant ad...
The internal antarctic plateau revealed in the last years to be a site with interesting potentialiti...
Turbulence in the earth’s atmosphere severely limits the resolution and sensitivity of astronomical ...
International audienceDuring the austral winter 2005, the first astronomical site testing campaign w...
International audienceDuring the austral winter 2005, the first astronomical site testing campaign w...
International audienceDuring the austral winter 2005, the first astronomical site testing campaign w...
Modeling of astronomically important atmospheric parameters, and the impact these parameters have on...
Modeling of astronomically important atmospheric parameters, and the impact these parameters have on...
The high plateau that covers half of the continent of Antarctica contains the best astronomical obse...
From the South Pole, microthermal turbulence within a narrow surface boundary layer some 200 m thic...
The turbulence structure of the atmosphere is the primary limitation to adaptive optics system perfo...
Abstract. The turbulence structure of the atmosphere is the primary limitation to adaptive optics sy...
The performance of natural guide star adaptive-optics systems for telescopes located on the Antarcti...
The unique atmospheric characteristics found at Dome C on the Antarctic plateau offer significant ad...
The unique atmospheric characteristics found at Dome C on the Antarctic plateau offer significant ad...
The unique atmospheric characteristics found at Dome C on the Antarctic plateau offer significant ad...
The internal antarctic plateau revealed in the last years to be a site with interesting potentialiti...
Turbulence in the earth’s atmosphere severely limits the resolution and sensitivity of astronomical ...
International audienceDuring the austral winter 2005, the first astronomical site testing campaign w...
International audienceDuring the austral winter 2005, the first astronomical site testing campaign w...
International audienceDuring the austral winter 2005, the first astronomical site testing campaign w...
Modeling of astronomically important atmospheric parameters, and the impact these parameters have on...
Modeling of astronomically important atmospheric parameters, and the impact these parameters have on...
The high plateau that covers half of the continent of Antarctica contains the best astronomical obse...
From the South Pole, microthermal turbulence within a narrow surface boundary layer some 200 m thic...