I have got a parabolic mirror 4" in size. I need to use it in an
optics experiment but am having trouble aligning it properly. Namely,
I have not been able to ascertain when the laser beam is hitting its
center. Would be grateful for any input.
Nutan
What precision is required?
cm, mm, µm ?
w.
One could use an aperture
on the mirror with a small hole in the center.
(An early and cheap version may be made of black paper) .
The diameter of the hole should be slightly bigger than the diameter
of the laser bundle.
If the light is going back to the source, the tilt alignment is
correct.
Harald
If the collimated laser diameter is large say 2 to 6" diameter, or use
the beam from an interferometer, like a 4" diameter zygo, wyko, etc
you can place a retroreflecting sphere near the focus.
The collimated beam will reflect off of the mirror and go toward the
focus at the center of the retroreflecting sphere (or hemisphere as
you only need the front diameter to reflect the beam back).
If the beam is not centered you will see an aberrated return wavefront
in the interferometer, or simply a returned beam with an angle to the
input beam.
You could also use this method with an alignment telescope as well.
If you are using a laser pointer type small laser, as one other poster
said, poke a hole in a piece of paper and look for the returned beam
to be centered on the hole in the paper. To be clear this technique
with the laser pointer does not use a retro sphere.
You may enjoy this short course DVD on optical alignment, or others in
the industry that are delivered 1-2 times per year.
http://www.oscintl.com/Short_Course_DVDs/intro__oa_dvd.htm
Michael
To Helmut;
Thanks for the response. I am using the mirror in an interferometric
setup and as such it should be better than mm.
To Harald;
Yes in theory it should work, but the distance between the mirror and
the source is small and it seems that I can have the beam go to the
source at off center positions too. Any idea what can solve the
problem.
This is a two sided problem: detection versus control. How to you control
the alignment?
> Yes in theory it should work, but the distance between the mirror and
> the source is small and it seems that I can have the beam go to the
> source at off center positions too. Any idea what can solve the
> problem.
For the 4" = 101.6 mm diameter of an astro-telescope mirror one may
expect a focal lenght of about 1 m.
What is your focal length?
Harald
> > Yes in theory it should work, but the distance between the mirror and
> > the source is small and it seems that I can have the beam go to the
> > source at off center positions too. Any idea what can solve the
> > problem.
I use a second aperture with a hole of a few millimeters on the
interferometer output (e.g. a 4" reference flat).
So I have two small apertures (one at the interfeometer, defining the
optical axis, and the other one at the mirror),
which makes it easy to to center the mirror on the optical axis.
Harald
I have translational freedom along all the axes and freedom of yaw and
pitch for rotation. Because of this the aperture concept does not seem
to work for I can always make the incident beam almost perpendicular
to the mirror as such the beam can be made to go to the source even if
it is not hitting the center of the mirror.
Find the center of the mirror by dropping a sphere onto it and
observing the Newton's rings. Make sure that you check the center for
different azimuths (roll) of the sphere to eliminate errors introduced
by wedge in your test sphere. View from an "on axis" direction to
eliminate errors due to the test and reference surfaces being
separated.
Once you have located the center it should be easy to align your
laser.
Rough align the system, then put a ground glass screen into the beam at
the center of curvature to create a speckle cone out to the parabola and
back. Move inside and outside the center of curvature (along the
caustic) and observe the returned pattern on the ground glass. Adjust
for a concentric pattern.
Jeff Lowe
--
Bob May
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