The ALFA laser guide star: Operation and results

被引:18
作者
Davies, R [1 ]
Eckart, A
Hackenberg, W
Ott, T
Butler, D
Kasper, M
Quirrenbach, A
机构
[1] Max Planck Inst Extraterr Phys, D-37075 Garching, Germany
[2] Max Planck Inst Astron, D-69117 Heidelberg, Germany
[3] Univ Calif San Diego, San Diego, CA 92103 USA
关键词
Abell Galaxy Clusters; adaptive optics; atmospheric turbulence; Herbig Ae/Be stars; laser guide star; sodium profile;
D O I
10.1023/A:1008165517543
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The importance of laser guide stars to the practical usefulness of adaptive optics cannot be understated, and yet there are very few working systems. This contribution discusses the current status of the ALFA laser guide star, with regard to the particular difficulties encountered while observing as well as both the expected performance and that so far achieved from scientific observations. A description is given of a number of experiments involving ALFA which aim to determine the atmospheric turbulence and sodium layer charateristics, and demonstrate the possibility for tilt recovery from laser guide stars.
引用
收藏
页码:103 / 121
页数:19
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