Is starlight a TEM00 gaussian beam or plane wave?

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Discussion Overview

The discussion revolves around the appropriate model for simulating starlight in a radio telescope context, specifically whether to use a TEM00 Gaussian beam or a plane wave. The scope includes theoretical considerations and practical implications for simulation tools.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • Robin questions whether to simulate starlight as a TEM00 Gaussian beam or a plane wave for a radio telescope simulation.
  • Some participants suggest that at astronomical distances, the wavefront from stars can be approximated as spherical, and thus the portion received by the telescope can be treated as a plane wave, citing the van Cittert-Zernike theorem for spatial coherence.
  • Others argue against modeling starlight as a Gaussian beam, noting that Gaussian optics assumes monochromatic light with perfect coherence, which does not hold true for starlight due to its inherent incoherence at distances near the star.
  • A participant mentions that a Gaussian beam can be approximated as a plane wave at infinite distances, but expresses concerns about awkward results when simulating this in Zemax.
  • Another participant acknowledges the incoherence of starlight and the need for a different simulation tool, as Zemax does not provide a plane wave simulation for long wavelengths.

Areas of Agreement / Disagreement

Participants express differing views on whether starlight should be modeled as a Gaussian beam or a plane wave, indicating that multiple competing perspectives remain unresolved.

Contextual Notes

Limitations include the assumptions about coherence and the applicability of Gaussian optics to starlight, as well as the constraints of simulation tools like Zemax.

Robin Lee
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I am simulating a radio telescope and confused on what kind of source should I setup to simulate a star. Should it be a TEM00 gaussian beam or simply a plane wave?Cheers,
Robin
 
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At astronomically far distances, the wavefront from stars can be well approximated as being spherical. Since the size of radiotelescope is much smaller than the radius of the wavefront which impinges on it, the wavefront portion received by the telescope can further be assumed as a plane wave. This wave will also be spatially coherent, as granted by van Cittert-Zernike theorem, which constitutes the fact that radiotelescope works (i.e. it does detect interference).
 
blue_leaf77 said:
At astronomically far distances, the wavefront from stars can be well approximated as being spherical. Since the size of radiotelescope is much smaller than the radius of the wavefront which impinges on it, the wavefront portion received by the telescope can further be assumed as a plane wave. This wave will also be spatially coherent, as granted by van Cittert-Zernike theorem, which constitutes the fact that radiotelescope works (i.e. it does detect interference).
Thank you! A gaussian beam can be assumed to be a plane wave when the distance it has traveled has become infinitely far since its radius of curvature increases proportionally to the distance it travels. Simulating a star as an infinitely far Gaussian beam in Zemax gives an awkward result though, I digress.
 
I don't think it's a good idea to simulate the beam profile from stars to follow Gaussian nature, remember Gaussian optics was derived under the assumption that the beam is monochromatic and hence has perfect coherence everywhere. This is obviously not true in the case of starlight because the light emitted from stars is very incoherent at some distance near the star. The wavefront becomes coherent after it has traveled tremendous distance from the source star, e.g. on earth.
 
blue_leaf77 said:
I don't think it's a good idea to simulate the beam profile from stars to follow Gaussian nature, remember Gaussian optics was derived under the assumption that the beam is monochromatic and hence has perfect coherence everywhere. This is obviously not true in the case of starlight because the light emitted from stars is very incoherent at some distance near the star. The wavefront becomes coherent after it has traveled tremendous distance from the source star, e.g. on earth.
You're right. Thanks for pointing that out. Now Zemax doesn't really offer a plane wave simulation for long wavelength simulation. I need to find a new tool.
 

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