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Diffraction Grating Resolving Power & Dispersion Calculator

Diffraction gratings disperse polychromatic light into constituent wavelengths via constructive interference across periodic grooves.

Number of ruled or holographic grooves per millimeter.

Spectral diffraction order (integer, e.g. 1 or 2).

Width of light beam spot illuminating the grating.

Incident light wavelength (e.g. Sodium doublet).

Calculated Result
48,000

Theoretical Resolving Power (R)

Min Resolvable Δλ

12.271 pm

Diffraction Angle (θ)

44.98°

Illuminated Grating Lines (N)

48,000 lines

Calculation Breakdown

  1. Resolving PowerR = |m| · N = |1| · (1200 · 40) = 48,000
  2. Wavelength ResolutionΔλ_min = λ / R = 589 nm / 48,000 = 12.271 pm

What Is the Diffraction Grating Resolving Power & Dispersion Calculator?

A diffraction grating is an optical component with a periodic structure that splits and diffracts light into several beams traveling in different directions.

How Does the Diffraction Grating Resolving Power & Dispersion Calculator Work?

Diffraction orders constructively interfere according to the grating equation d * sin(theta) = m * lambda.

Diffraction Grating Resolving Power & Dispersion Calculator Formula & Variables

The core mathematical equation utilized by this calculator is expressed as:

R = |m| cdot N, quad Deltalambda_{min} = rac{lambda}{R}, quad sin heta_m = rac{m lambda}{d}

Theoretical grating resolving power from Rayleigh criterion and grating equation at normal incidence.

How to Use the Diffraction Grating Resolving Power & Dispersion Calculator

  1. Enter groove density, diffraction order, illuminated grating width, and target wavelength.

Step-by-Step Example Calculation

Sodium D-Line Spectrometer

Input Values:

grooveDensityLinesPerMm:1200
diffractionOrderM:1
totalIlluminatedWidthMm:40
wavelengthNm:589
Worked Steps: Resolving power R = 48,000, capable of resolving lines separated by only 12.3 pm at 44.97° diffraction angle.

Understanding Your Result

Higher R allows resolving closely spaced spectral emission lines (such as isotope splitting).

Factors That Affect the Result

  • Ghost rulings, groove profile blaze angle, and aberrations from optical focus lenses.

When Should You Use This Calculator?

  • Astronomical spectrograph design, monochromator instrument development, and Raman spectroscopy.

Assumptions & Limitations

  • Assumes normal incidence illumination and a collimated plane wave.

Frequently Asked Questions

Calculation Accuracy & Reference Note

Standard Fraunhofer grating diffraction theory.

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