Lobster Eye Optics

Welcome to Lobster Eye Optics

The lobster eye consists of square channels arranged into a spherical array. Light reflecting down the channels forms a cross shaped image. The geometry behind the reflections is shown below.

The principle behind lobster eye reflections In order to apply lobster eye optics to x-rays, we must make a spherically curved array of square channels. It is also convenient if the size of individual channels is small.

Microchannel plates (MCP's) typically consist of an array of small circular channels. Using the same technology, square channel MCP's are now being made with channel sizes down to 10 microns. Square channel MCP

Why is Lobster eye optics useful for x-ray optics?

In the lobster eye geometry it is possible to arrange for the x-ray reflections to occur at very small angles. At these angles the reflectivity is high so less incident flux is lost.

The intensity in the central region of the cross can be thousands of times greater than that of the incident x-ray flux.

Any application which will benefit from an increase in x-ray intensity in a small area could potentially benefit from using a lobster eye arrangement.

How well do MCP's work?

At the University of Melbourne we have been testing MCP's and comparing their performance with theoretical predictions.

A typical experimental arrangement uses a point source of x-rays, for instance, from a laser produced plasma. An intense laser pulse is focused onto a target. The resulting plasma is a strong emitter of x-rays which are then focused through the MCP onto film. Focal plane intensity for a 200 micron pore MCP

The best results to date show the focused intensity to be about one third of that for a perfect MCP. When we incorporate realistic geometric deformation parametres into our theory we obtain excellent agreement between the experiment and theory.

Would you like to work with us?

Anyone interested in these areas of x-ray optics at The University of Melbourne should contact:

There have been accesses to this page since October 20, 1995.

Optics Group


Chris. Chantler, Chris_Chantler.physics@muwayf.unimelb.edu.au
Last modified: 20 October 1995
Copyright © 1995 The University of Melbourne