LBTI Software Architecture

被引：0

作者：

Vaitheeswaran, Vidhya ^{[1
]}

Hinz, Phil ^{[1
]}

Kraus, Joseph ^{[1
]}

Breuninger, Andrew ^{[2
]}

机构：

[1] Univ Arizona, Steward Observ, 933 N Cherry Ave, Tucson, AZ 85721 USA

[2] South African Large Telescope, Karoo, South Africa

来源：

ADVANCED SOFTWARE AND CONTROL FOR ASTRONOMY II, PTS 1 & 2 | 2008年 / 7019卷

关键词：

Interferometer; Software;

D O I：

10.1117/12.790265

中图分类号：

TP [自动化技术、计算机技术];

学科分类号：

0812 ;

摘要：

LBTI is a thermal imager and a nulling interferometer to be installed on the Large Binocular Telescope (LBT). Here, we present the distributed component architecture model and its simple yet powerful software structure designed to complement the LBTI hardware model that comprises pyramid wave front sensors with its control electronic universal beam combiner, phase sensor, science imager, and all housekeeping duties to run the cryogenics, compressors, vibration monitors and the interface to the telescope control systems.

引用

页数：8