Test environment running 7.6.6

Cultural advice

The Australian National University acknowledges, celebrates and pays our respects to the Ngunnawal and Ngambri people of the Canberra region and to all First Nations Australians on whose traditional lands we meet and work, and whose cultures are among the oldest continuing cultures in human history.

Aboriginal and Torres Strait Islander peoples are advised that ANU Library collections may include images, names, voices, and other representations of deceased persons.

Material in the collection may contain terms, language or views that reflect the period in which the item was created and may be considered inappropriate today.

Coupled waveguide integrated optic segment piston sensor for the GMT

Abstract

Integrated optic segment piston sensor (IOPS) for the Giant Magellan Telescope (GMT) uses single mode laser written waveguides to measure segment piston (axial alignment) of the GMT primary mirrors. Light in the H-band (from 1.5 to 1.6 μm) incident on each segment originating from an off-axis guide star is coupled into separate laser written single mode waveguides in a fused silica substrate. The waveguide inputs are positioned at the focus of a lenslet array with the same hexagonal geometry as the GMT pupil. Light from neighbouring segments is interfered in several coupling regions where waveguides are in spatial proximity allowing coupling, in order to produce an interference signal at the output. The output signal magnitude is directly related to the phase difference at the waveguide input, originating from the segment piston. Three coupling regions achieve this by splitting the light into one reference, and two signal lines. The reference provides a measurement of the amount of light coupled into the input waveguide, while each signal line is passed on to other couplers to be interfered with light from two neighbouring segments.

Description

Keywords

Citation

Source

Type

Book Title

Entity type

Access Statement

License Rights

Restricted until