Optics & Resolution: Can I See the Peak?

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To determine if a peak at 100 MHz can be observed with a resolution of Δλ 0.5 nm, first convert the FWHM into a wavelength range by converting 500 nm into frequency and adjusting for ±50 MHz. This allows for a direct comparison with the spectrometer's wavelength resolution. It's important to note that detecting the peak differs from resolving its width, requiring Δf/f to be greater than Δλ/λ for resolution. The relationship Δf/f = λ·Δf/c is valid in vacuum and approximately in air, with adjustments for the medium's refractive index. Understanding these conversions and relationships is crucial for accurate peak observation.
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Hi

Say I have a peak of about 100 MHz, and my apparature has a resolution of about Δλ 0.5 nm. How can I find out whether I will see the peak or not?
 
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It's not clear from your post: is the peak located at 100MHz, or is that the full width half maximum? You have a certain wavelength resolution, but what is the mean wavelength?
 
100 MHz is the FWHM. We are in the visible range, so λ ~ 500 nm (sorry, I should have specified that first).
 
Ok.

Here's what I would do: convert the FWHM into a wavelength range: do this by converting 500nm into frequency, then add +/- 50 MHz, and convert back to wavelengths. Then you can compare directly with the wavelength resolution of your spectrometer.

Something to keep in mind- detecting the peak is different than resolving the peak width.
 
I would compare Δf/f (=λ·Δf/c) with Δλ/λ (=0.001).

You need Δf/f > Δλ/λ in order to resolve the peak.

(In case it's not clear from the context of this thread, Δf is the FWHM of the peak, and Δλ is the spectrometer resolution.)
 
Thanks to both of you. Redbelly98, isn't Δf/f =λ·Δf/c only valid in vacuum?
 
Strictly speaking, yes. It's a reasonable approximation in air as well. What medium does your spectrometer operate in?
 
In air. But what is the general version of λf =c?
 
The speed of light in a medium is c/n, so
λf =c/n
where λ is the wavelength in the medium.
 

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