| 1. | Commonly, a microscope objective is used to collect the object wave front.
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| 2. | Which is also the equation for spherical wave fronts of light.
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| 3. | This is like the photons moving as a wave front.
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| 4. | Thus the wave fronts will refract, changing direction like light passing through a prism.
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| 5. | But it's less of a wave front with each reflection.
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| 6. | The new wave front is found by constructing the surface tangent to the secondary wavelets.
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| 7. | Einstein asks what makes each electron's wave front " collapse " at its respective location.
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| 8. | Both theories describe one-dimensional and steady wave fronts.
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| 9. | The distance between successive wave fronts is then increased, so the waves " spread out ".
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| 10. | For instance, the tsunami that hit Hawaii in 1946 had a fifteen-minute interval between wave fronts.
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