Holmarc’s grating spectrometer consists of a holographic concave diffraction grating and a one-dimensional CCD detector array. It delivers excellent thermal stability with low stray light for wide range of research and OEM applications. The concave gratings accomplish the task of two optical elements in a single, easily integrated component. It has one micrometer controlled variable input slit with LED holder.
The spectral power distribution of the optical radiation emitted by LED differs in many ways from other radiation sources. It is neither monochromatic like a laser nor broadband like a Tungsten lamp but rather lies between these two extremes. The spectrum of LED has a specific peak wavelength depending on the manufacturing process where the FWHM is typically a couple of tens of nanometres. Holmarc’s grating spectrometer gives fast and reliable LED spectral characterization.
Spectrometer interfaces with a computer via Type-B USB 2.0. The entire power requirement is drawn through the 2.0 type-B USB connector. Spectra QSR software gives the output plot of intensity versus wavelength.
Peak wavelength λp:
Peak wavelength λp is the wavelength at the maximum intensity of the spectrum. The peak wavelength is easy to define and is therefore generally given in LED data sheets. owever, the peak wavelength has little significance for practical purposes since two LEDs may have the same peak wavelength but different colour perceptions.
Spectral Band width FWHM:
The spectral bandwidth at half intensity, Δλ is calculated from the two wavelengths λ and λ on either side of λp
Δλ = λ1 – λ2
Other parameters like Centre wavelength, Centroid wavelength, Dominant wavelength, etc can be studied.
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