The JOSE atmospheric seeing monitor at the William Herschel Telescope

被引：13

作者：

StJacques, D

Cox, CC

Baldwin, JE

Mackay, CD

Waldram, EM

Wilson, RW

机构：

[1] UNIV CAMBRIDGE,INST ASTRON,CAMBRIDGE CB3 0HA,ENGLAND

[2] ROYAL GREENWICH OBSERV,CAMBRIDGE CB3 0EZ,ENGLAND

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1997年 / 290卷 / 01期

关键词：

atmospheric effects; site testing; telescopes;

D O I：

10.1093/mnras/290.1.66

中图分类号：

P1 [天文学];

学科分类号：

0704 [天文学];

摘要：

We have installed a Shack-Hartmann wavefront sensor at the William Herschel Telescope. The sensor has 8x8 subapertures and operates at frame rates up to 865 Hz. It is used to monitor those aspects of the seeing relevant to the design and optimization of the future WHT adaptive optics system. Here we describe its implementation and present some sample results.

引用

页码：66 / 74

页数：9

共 7 条

[1]

BECKERS JM, 1993, ARA A, V13, P62

[2]

OPTICAL RESOLUTION THROUGH A RANDOMLY INHOMOGENEOUS MEDIUM FOR VERY LONG AND VERY SHORT EXPOSURES [J].