Multiple field of view layer-oriented adaptive optics - Nearly whole sky coverage on 8 m class telescopes and beyond

被引:78
作者
Ragazzoni, R
Diolaiti, E
Farinato, J
Fedrigo, E
Marchetti, E
Tordi, M
Kirkman, D
机构
[1] Osserv Astrofis Arcetri, INAF, I-50125 Florence, Italy
[2] Max Planck Inst Astron, D-69117 Heidelberg, Germany
[3] Univ Padua, Dept Astron, I-35122 Padua, Italy
[4] European So Observ, D-85748 Garching, Germany
[5] Osserv Astron Padova, INAF, I-35122 Padua, Italy
[6] Univ Calif San Diego, Ctr Astrophys & Space Sci, La Jolla, CA 92093 USA
关键词
telescopes; instrumentation : adaptive optics; techniques : high angular resolution;
D O I
10.1051/0004-6361:20021406
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In layer-oriented adaptive optics, multiconjugation is performed in a much more efficient way than conventional wavefront sensing. This improved efficiency is impressive for high altitude layers and moderate for ground ones. On the other hand, high altitude layers can be covered with only a limited field of view (where one can search for natural guide stars) while for ground layers the usable field of view is limited essentially by practical reasons. We introduce the further concept of multiple field of view layer-oriented adaptive optics where a combination of sampling and covered field leads easily to sky coverages for 8 m class telescopes that nearly approach the whole sky with the usage solely of natural guide stars. The extension of the concept to much larger apertures is also discussed.
引用
收藏
页码:731 / 744
页数:14
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