X-ray Mirror to be used by telescope

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SUMMARY

The discussion centers on the design of an X-ray mirror system utilizing a combination of parabolic and hyperbolic mirrors, inspired by Hans Wolter's design. The user, James, proposes a mathematical approach to eliminate blurring caused by off-axis rays by adjusting the lengths of the mirrors. He derives equations to determine the focal points and conditions for optimal ray focusing, emphasizing the need for precise measurements between the two mirror types. The conversation highlights the challenges in achieving effective X-ray focusing and suggests layering mirrors as a potential solution.

PREREQUISITES
  • Understanding of geometric optics, specifically parabolic and hyperbolic mirror properties.
  • Familiarity with X-ray optics and the challenges of focusing X-rays.
  • Basic knowledge of mathematical equations related to optics, including focal points and ray tracing.
  • Experience with optical design software or tools used in telescope mirror design.
NEXT STEPS
  • Research the principles of X-ray optics and the specific challenges associated with off-axis ray focusing.
  • Study Hans Wolter's mirror design and its applications in modern X-ray telescopes.
  • Explore mathematical modeling techniques for optical systems, focusing on ray tracing algorithms.
  • Investigate materials and technologies used for X-ray mirrors, including multilayer coatings.
USEFUL FOR

Astronomers, optical engineers, and researchers involved in X-ray telescope design and development will benefit from this discussion, particularly those focused on improving the performance of X-ray mirrors.

Jam132
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Hey all!,
I'm working on a project in which I have to design the shape of a mirror to focus X-rays. This is basically what I've done so far so far.

I've found that if you use a parabola mirror it will focus parallal rays, but not off-axis ones. If you then add a second mirror in the form of a hyperbola mirror it will also focus paralellel rays but not off-axis rays. This is the problem. From my research I know that in practice scientists use a design develped by Hans Wolter. What he did was stick a parabola onto a hyperbola mirror, but I can't work out how he got rid of the blurring. I've came up with an idea but I'm not sure if its correct, I was wondering if anyone here who knows anything about this subject can help me out.

Heres my method for getting rid of the blur:

I have devived an equation giving the point at which rays cross the focal plane:

y(c) = (Pheta)x(a)[x(b) - L] / x(b)

Where L equals the focus point of the two mirros combined, Pheta is the angle by which the ray if off axis, x(a) is the point the ray hits the parabola mirror, and x(b) is the point the ray hits the hyperbola, y(c) is where the ray crosses the focal plane.

A ray hitting the front of the parabola mirror will focus at the point:

x(a) = x(1) = x(2) + (delta)x(1) = 2L + (delta)x(1)

So, y(c) = (pheta)L[1 + (delta)x(1)/2L - (delta)x(2)/2L] eqn (1)

Where, (delta)x(1) = length of the parabola mirror, (delta)x(2) = length of the hyperbola mirror. We have also set the point at which the two mirrors join equal to 2L.

If the rays are to focus equation(1) must equal zero:

y(c) = (Pheta)L[ 1 + ... - ...] = 0

For this to happen either Pheta must equal zero, in other words, the rays must be parallel, which I've already proven. Or, the sum of everything inside the square brackets must equal zero:

So,
1+ (delta)x(1)/2L - (delta)x(2)/2L = 0

The only way this can happen is if:

(delta)x(1)/2L - (delta)x(2)/2L = -1

When you rearrange this equation you find that:

(delta)x(1) = (delta)x(2) - x(2) and (delta)x(2) = (delta)x(1) + x(2)

So, (delta)x(2) - (delta)x(1) = x(2)

Where (delta)x(1), is the length of the parabola mirror, and (delta)x(2) is the length of the hyperbola mirror and x(2) is the point at which the two mirrors join.

Therefore, if we set the mirrors lengths so that the diffence in the length between the two mirrors is equal to the point at which the two mirrors join the rays should focus. Example - If we set x(2) equal to 2L, then that would mean that the length of the hyperbola mirror must be longer than the parabola mirror by 2L.

This will focus rays hitting the front of the parabola mirror and I asume will work for rays hitting all parts of the mirror, apart form the point at which the two mirrors meet.
For the back of the parabola mirror, the point at which the two mirrors join, x(2):

x(a) = x(b) = x(2) = 2L
Since we have set x(2) = 2L.

So, y(c) = (pheta)L eqn (2) for the back of the parabola mirror.
The only way eqn(2) will equal zero (focus), is if pheta = 0 , in other words only for parallel rays. Off axis rays will cause a blur. To get round this problem you can layer the mirrors like in the XMM Newton, this will collect more X-rays, but can also be used to block rays hitting the point x(2) off axis.

Thanks for your time and reading all of this, hope I made it clear enough.
Thanks James.
 
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There is no currently existing material that acts like a mirror under x-rays.
 
Nickidemic said:
There is no currently existing material that acts like a mirror under x-rays.
Please don't necropost to these old threads. The OP was posted almost ten years ago!
 

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