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by Synaesthesia
477 days ago
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Yeah I read that, and upon re-reading it I have some vague idea on how that might work, but I would still need to read the paper and see some illustrations to really get it. Sounds like this may enable full-colour astrophotography (always wondered why it's all in B&W!) and/or make achromatic telescopes a lot lighter. |
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In conventional diffractive optics, the focal plane (where the sensor should be placed for a focused image) is wavelength-dependent. This means that you receive an in-focus image of the scene for a specific wavelength λ_i when your sensor is located a distance d_i from the lens [0]. By varying d_i you can scan the scene for all wavelengths even if your sensor is monochromatic. You get blurry versions of all other wavelengths as well, but the idea is to use computational techniques to separate these out.
Here, they've designed an optic which tries to eliminate the wavelength dependence of the lens focal plane. Instead of you place an RGB sensor at this one focal plane to get all the wavelengths.
0: https://ieeexplore.ieee.org/abstract/document/9191355?figure...