What are the practical limits of constructive interference?

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Constructive interference in wave sources can create complex interference patterns, often resulting in infinitely extending lobes that complicate the targeted delivery of energy, whether acoustic or electromagnetic. Arranging sources in specific geometric formations, like a triangle, may help create spatially constrained maxima. However, there are no simple rules of thumb to effectively manage these patterns without advanced techniques such as Fourier analysis. The challenge of directing energy with a narrow beam width necessitates a larger aperture, as dictated by diffraction principles. Techniques like 'Supergain Arrays' offer limited improvements, which is why large structures like radiotelescopes are required for effective energy direction.
rumborak
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The "wireless power" thread made me think of this, but I have pondered it before when it comes to microphone arrays etc
You can easily find documentation on the interference patterns N in-line sources of waves generate. E.g.

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The annoying thing here is that you have infinitely extending lobes, which would be undesirable for something that tries to pinpoint delivery of (acoustic/EM) energy.
It would seem to me that for example a source arrangement in a triangle would allow some spatially constrained Maxima inside it; but are there simple rules of thumb for this type of thing that constrain the patterns? I can imagine that with a complete ring of sources you could probably reverse engineer any pattern with a Fourier analysis, but that's also overkill on the other end.
 
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rumborak said:
The annoying thing here is that you have infinitely extending lobes, which would be undesirable for something that tries to pinpoint delivery of (acoustic/EM) energy.
This is a consequence of Diffraction. To direct energy in a specified direction with a certain required beam width you need an extended source. The narrower the required beam θ, the wider the necessary Aperture, d. (roughly θ = λ/2d) There are techniques for doing a bit better than the diffraction limit with 'Supergain Arrays' but there is not a lot of juice in that lemon. This is one of the reasons why Radiotelescopes are so enormous.
 

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