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Update Angular resolution.md
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It seems that in astronomy, there is a relationship between the image resolution $\theta$ and the wavelength $\lambda$ giving by
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$\theta = 1.22 \frac{\lambda} {D}$
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$$\int_\Omega \nabla u \cdot \nabla v~dx = \int_\Omega fv~dx$$
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- Where $D$ is the diameter of the telescope.
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- to get better resolution (small $\theta$), we need:

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