What is the difference between echelle and Echellette?

Difference Between Echelle and Echellette Gratings

The terms echelle and echellette both refer to types of diffraction gratings used in spectroscopy, but they are designed with different groove profiles and are optimized for different spectroscopic applications. Below are detailed differences between them.

Echelle Gratings

Echelle gratings are a type of diffraction grating that have very high groove densities, typically several hundreds to a few thousands lines per millimeter. They are characterized by their blaze angle, which is significantly larger than that of conventional diffraction gratings. This results in more efficient diffracting at high orders, enabling high dispersion and resolution over a narrow wavelength range at any one time, making them suitable for high-resolution spectroscopy.

Echelle gratings operate in high diffraction orders (m), which allows them to separate wavelengths very finely. They are often used in arrangements where they are crossed with another grating, like a prism or another diffraction grating, to separate the overlapping higher orders and enhance spectral resolution.

These gratings are primarily used in astronomy and other fields where high-resolution spectral analysis is required. They are often found in advanced spectrometers and echelle spectrographs.

Echellette Gratings

Echellette gratings, on the other hand, are a type of ruled grating that has a lower density of grooves, typically tens to a few hundreds lines per millimeter. Their blaze angle is also lower than that of echelle gratings, which orients the spectral dispersion more towards the first-order diffraction maxima.

Echellette gratings are designed to operate primarily in first order, where they achieve high efficiency. Because of their low groove density, they have the advantage of dispersing light over a wider wavelength range than echelle gratings in a single spectral order, which is beneficial for applications that require spectral coverage across broad wavelengths.

They are suitable for medium-resolution spectroscopy and are commonly utilized in educational or laboratory environments, where broad wavelength coverage with moderate resolution is adequate.

Comparison Table

Feature Echelle Echellette
Groove Density High (hundreds to thousands/mm) Lower (tens to hundreds/mm)
Blaze Angle Large Smaller
Diffraction Orders High Primarily First
Resolution High Medium
Wavelength Coverage Narrow Broad
Typical Applications High-resolution spectroscopy (e.g., astronomy) Medium-resolution spectroscopy (e.g., educational labs)


In summary, echelle gratings are optimized for high-resolution spectroscopy and operate at high diffraction orders, while echellette gratings are suited for medium-resolution spectroscopy with broader wavelength coverage at primarily the first diffraction order.

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