RONCHI 

Grating/Grating mode

Setting up the Grating/Grating arrangement.

Copyright – P. J. Smith

But permission is given to distribute this material in unaltered form as long as it is not sold for profit.

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General

Some test situations, where the source is close to the grating, allow the same grating to be extended in front of a light and diffuser.  Thus part of the grating acts as the source and part of the same grating as the occulter.

In the majority of test situations this is impossible because source and image are widely separated.

But in the case of testing a concave mirror at centre of curvature, or of testing a lens by autocollimation, the arrangement becomes possible.  Since testing concave mirrors at Centre of Curvature is all most ATM’s ever do, some seem to think this is the only way a Ronchi test can ever be done.  For a variety of other test situations see Advanced set-ups and Null testing.

Porter and Anderson seem to be the first to use this mode.  The following is an extract from their original article[1]

Before deciding on this mode of operation you should study the photographs comparing performance between Grating/Grating and Slit/Grating set-ups using different types of gratings. See Grating/Grating V Slit/Grating comparison.  Then decide if a Grating/Grating mode is best for you.


Simple Implementation

Area source

An incandescent source with a filament arranged in a line is an obvious choice and it does work well behind a diffuser.  This is probably best if you want really intense illumination.  For sheer brute force a 12 V Quartz Iodide headlight bulb is hard to beat but is seldom needed unless more than one unsilvered surface are in the test beam.  Excess heat may be a problem[2]. 

A simple, perfectly adequate light source which will evenly illuminate an area of grating is a bright LED with its collimating front lens left intact.  A small flashlight bulb also works but LED’s are small and cool.

This produces an area rather than a line source of light but the extremely high efficiency of a grating source as opposed to a pinhole or even a slit makes this entirely adequate for visual work.  A diffuser (see Diffuser) is placed just in front of the LED with the grating just in front of this. The reason it is best to leave the collimating lens surface in place on the LED is because this produces more even illumination over the area of the grating.

LEDs of 5 and 10 mm diameter are readily available.  5 mm is usually sufficient and is easier to mount close to the axis but for special cases a 10 mm one would have advantages.  A larger grating source is easier to locate and makes for more tolerant set-up. Be careful when using a very large illuminated grating as source since it is easy to use an active portion of source and occulter that is separated by more than the minimum distance. Sometimes you will stray off axis more than you would like.  Extremely simple set-ups using this arrangement are the Basic and Emergency rigs. The Basic rig also is suited to a slit although the Deluxe rig is better in this role.

Since the Viewing Grating is the same as the Source Grating, there is no alignment to be done and the grating is always in position.  The main problem is allowing for unobstructed head and eye access .

With some ingenuity and blue-tac it is easy to conceive other simple systems.


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[1] 1929 J. A. Anderson and R.W Porter, Astrophys. J. 70, 175, 175, (1929),    "Ronchi's Method of Optical Testing"

 

 

[2] The beam may be folded so the heat source is at one side and the bulb may be run on reduced voltage as required to reduce excess heat.