Ronchi test
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In optical testing a Ronchi test is a method of determining the figure of a mirror used in telescopes and other optical devices.
[edit] Description
Described in a 1922 published work by Italian physicist Vasco Ronchi, the Ronchi test is a variation of the Foucault test that uses simple equipment in the testing of optics, especially concave mirrors. [1]. A "Ronchi tester" consists of:
- A light source
- A diffuser
- A Ronchi grating
Light is emitted through the Ronchi grating (or a single slit), reflected by the mirror being tested, then passes through the Ronchi grating again and is observed by the person doing the test. The observer's eye is placed close to the centre of curvature of the mirror under test looking at the mirror through the grating. The Ronchi grating is a short distance (less than 2cm) closer to the mirror.
The observer sees the mirror covered in a pattern of stripes that reveal the shape of the mirror. The pattern is compared to a mathematically generated diagram (usually done on a computer today) of what it should look like for a given figure. Inputs to the program are line frequency of the Ronchi grating, focal length and diameter of the mirror, and the figure required. If the mirror is spherical, the pattern consists of straight lines.
[edit] Applications
The Ronchi test is used in the testing of mirrors for Reflecting telescopes especially in the field of Amateur telescope making. It is much faster to set up than the standard Foucault test but, unlike the Foucault tester, the Ronchi test requires a piece of specialized equipment (the Ronchi grating) and is more subjective. It offers a quick glimpse at the mirrors shape and condition, and can quickly identify a 'turned edge' (rolled down outer diameter of the mirror), a common fault that can develop in objective mirror making.
