ACTIVE OPTICS, ADAPTIVE OPTICS, AND LASER GUIDE STARS

被引:51
作者
HUBIN, N
NOETHE, L
机构
[1] European Southern Observatory, 85748 Garching
关键词
D O I
10.1126/science.262.5138.1390
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
Optical astronomy is crucial to our understanding of the universe, but the capabilities of ground-based telescopes are severely limited by the effects of telescope errors and of the atmosphere on the passage of light. Recently, it has become possible to construct inbuilt corrective devices that can compensate for both types of degradations as observations are conducted. For full use of the newly emerged class of 8-meter telescopes, such active corrective capabilities, known as active and adaptive optics, are essential. Some physical limitations in the adaptive optics field can be overcome by artificially created reference stars, called laser guide stars. These new technologies have lately been applied with success to some medium and very large telescopes.
引用
收藏
页码:1390 / 1394
页数:5
相关论文
共 61 条
[1]   SOLAR IMAGING WITH A SEGMENTED ADAPTIVE MIRROR [J].
ACTON, DS ;
SMITHSON, RC .
APPLIED OPTICS, 1992, 31 (16) :3161-3169
[2]  
ANGEL R, IN PRESS 48 ESO C WO
[3]  
[Anonymous], 1992, LINCOLN LAB J, V5, P1
[4]  
Babcock H. W., 1953, PUBL ASTRON SOC PAC, V65, P229, DOI DOI 10.1086/126606
[5]  
BECKERS JM, IN PRESS ANN REV AST
[6]  
BECKERS JM, 1988, UNDERSTANDING GALAXI, P319
[7]  
Boyer C., 1990, P SOC PHOTO-OPT INS, V1237, P63
[8]  
CHASSAT F, 1989, P SOC PHOTO-OPT INS, V1130, P33
[9]   CONTROL OF OPTICAL SURFACE OF A THIN, DEFORMABLE PRIMARY MIRROR WITHAPPLICATION TO AN ORBITING ASTRONOMICAL OBSERVATORY [J].
CREEDON, JF ;
LINDGREN, AG .
AUTOMATICA, 1970, 6 (05) :643-&
[10]   WAVE-FRONT SENSING DECONVOLUTION AND ADAPTIVE OPTICS [J].
FONTANELLA, JC .
JOURNAL OF OPTICS-NOUVELLE REVUE D OPTIQUE, 1985, 16 (06) :257-268