Hostname: page-component-78c5997874-dh8gc Total loading time: 0 Render date: 2024-11-08T02:11:54.375Z Has data issue: false hasContentIssue false
  • English
  • Français

Fibre Optic Development at the AAO

Published online by Cambridge University Press:  25 April 2016

P. M. Gray ,
M. M. Phillips ,
A. J. Turtle  and
R. Ellis
P. M. Gray
Affiliation:
Anglo-Australian Observatory
M. M. Phillips
Affiliation:
Cerro Tololo Interamerican Observatory
A. J. Turtle
Affiliation:
University of Sydney
R. Ellis
Affiliation:
Durham University
Get access Rights & Permissions [Opens in a new window]

Extract

Work on the development and use of optical fibres as light guides in astronomical spectroscopy has been underway at the AAO for over a year now. The fibres used are step-index polymer-clad silica with a core size of 200 microns giving an aperture size of 1.3 arcsec at the AAT f/8 focus. They are optimised for data transmission with losses below 5dB/km at a wavelength of 800 nm. The blue transmission is somewhat lower, typically 500dB/km at 300nm and 90dB/km at 400nm but over the short 2m length used these attenuations give transmissions of 79% and 96% respectively.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 4 , Issue 4 , 1982 , pp. 477 - 479
Copyright
Copyright © Astronomical Society of Australia 1982

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)