A Blazed Gratings and Littrow Mounting

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Blazed gratings enhance the spectral throughput of spectrometers by redirecting diffracted light energy into higher order spectra, which increases efficiency. The key mechanism involves the interference of multiple sources, where the intensity is influenced by the angle of incidence and reflection. While the literature often mentions the benefits of blazed gratings, detailed mathematical analyses and ray-trace sketches are scarce. The diffraction pattern from a single reflector peaks at specific angles, and the blaze angle shifts this peak away from the m=0 order, improving signal intensity. Resources such as the Richardson Grating Labs handbook and a referenced paper by Loewen may provide additional insights into this phenomenon.
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How do blazed gratings improve efficiency in spectrometer
I cannot for the life of me find any concise information on how blazed gratings improve the spectral throughput of a spectrometer system. The blazed grating structure and how it redirects spectral reflection is itself understandable- but any information I have indicates that it somehow "concentrates" the diffracted light energy into a higher order spectrum. What I see is that the specular output is indeed reflected away from the m=0 order, but beyond this I do not see how the specular content leads to an enhanced diffraction/ spectrum. In fact it would seem as those this light would obscure the higher order into which it is reflected.
I have consulted the ubiquitous Born & Wolfe on this (no information at all!), Hecht (meager information with no mathematical analysis) and Jenkins & white, not to mention a half dozen books on spectrometers. All simply state that the blaze, when mounted at the Littrow angle for the wavelength, mysteriously enhances the signal. I need the math here, or at least a ray-trace sketch to figure out how this happens.

I am trying to track down the 1916 paper by Wood and Trowbridge but meantime does anyone know a textbook (or even an online white paper) working through this problem?

Thanks
Fritz
 
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The diffraction intensity is given by the formula for the interference of ## N ## sources, ## I=I_o \frac{\sin^2(N \phi / 2)}{\sin^2(\phi / 2)} ##, (##\phi=\frac{2 \pi d ( \sin{\theta_i}+\sin{\theta_r})}{\lambda} ##), multiplied by the diffraction pattern of a single slit, (or Huygens reflector). It is this second term where the blazed grating offers higher efficiency. The diffraction pattern from a single reflector peaks where angle of incidence=angle of reflection. Here it is a reflective type grating (rather than transmissive). The blaze makes it so that this peak occurs at some other angle than the m=0 maximum.
 
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fsonnichsen said:
Summary:: How do blazed gratings improve efficiency in spectrometer

I cannot for the life of me find any concise information on how blazed gratings improve the spectral throughput of a spectrometer system.

Richardson Grating Labs has a 'handbook' that may be of help:
https://www.gratinglab.com/Information/Handbook/Handbook.aspx

In particular, there is a chapter on designing gratings for maximum efficiency. That handbook references a paper by Loewen:

https://www.osapublishing.org/ao/abstract.cfm?uri=ao-16-10-2711

that may have some useful details.
 
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