Advanced Siloxane Waveguide Devices for Telecommunications. This project will develop new methods for fabricating compact, high performance photonic integrated circuits (PICs) for use in future telecommunications networks in films of proprietary Inorganic Polymer Glasses (IPGs) commercialised by RPO Pty Ltd. New fabrication methods are required to overcome limitations of the current approach to patterning IPGs used by RPO Pty Ltd. Research will concentrate on hard contact lithography in conjunct ....Advanced Siloxane Waveguide Devices for Telecommunications. This project will develop new methods for fabricating compact, high performance photonic integrated circuits (PICs) for use in future telecommunications networks in films of proprietary Inorganic Polymer Glasses (IPGs) commercialised by RPO Pty Ltd. New fabrication methods are required to overcome limitations of the current approach to patterning IPGs used by RPO Pty Ltd. Research will concentrate on hard contact lithography in conjunction with dry (plasma) etching as well as ion beam milling; laser machining or UV writing for grating production. IPGs present special challenges for these technologies. The project outcomes will include new approaches to processing and the demonstration of the fabrication of innovative PICs in IPGs.Read moreRead less
A Laser Guide Star using a High Power, Synchronously Pumped Optical Parametric Oscillators. We will develop a novel high power source of 589nm coherent (laser) light to be used to create a laser guide star by exciting sodium atoms in the earth's upper atmosphere (the mesosphere). This is needed to determine the distortion caused by the atmosphere on an optical beam propagating through it and generate the information needed to correct those distortions using an adaptive optics telescope. This pr ....A Laser Guide Star using a High Power, Synchronously Pumped Optical Parametric Oscillators. We will develop a novel high power source of 589nm coherent (laser) light to be used to create a laser guide star by exciting sodium atoms in the earth's upper atmosphere (the mesosphere). This is needed to determine the distortion caused by the atmosphere on an optical beam propagating through it and generate the information needed to correct those distortions using an adaptive optics telescope. This project focuses on the development of a novel high power 589nm source based on a synchronously pumped optical parametric oscillator.Read moreRead less