What is the process to illuminate the moon with earth-based sources using initial waist sizes of 0.5 mm and 0.5 m, and how can we find the Rayleigh range, far field divergence angle, and spot size at the moon for each initial beam waist when using different sources?

Question

Jared · Answer

Calculation Process

To illuminate the moon with earth-based sources, we need to consider different initial beam waist sizes and use various sources like helium-neon laser beam, carbon dioxide laser, and an X-ray laser. The Rayleigh range, far-field divergence angle, and spot size at the moon vary based on the initial waist sizes and the wavelength of each source. By applying the formula for Rayleigh range, we can determine these parameters for each scenario.

Formula Used

The formula to find the Rayleigh range is given as: Rayleigh range (Z_R) = (π * w_0^2) / λ, where w_0 represents the initial beam waist, and λ is the wavelength of the source.

Specific Calculations

Helium-neon laser beam:
Initial beam waist = 0.5 mm = 0.5 x 10^-3 m
Rayleigh range ≈ 1.24 x 10^3 m
Far-field divergence angle ≈ 0.40 degrees
Spot size at the moon ≈ 1.31 x 10^6 m

Carbon dioxide laser:
Initial beam waist = 0.5 m
Rayleigh range ≈ 7.85 x 10^6 m
Far-field divergence angle ≈ 6.37 x 10^-5 degrees
Spot size at the moon ≈ 1.63 x 10^4 m

X-ray laser:
Initial beam waist = 0.5 m
Rayleigh range ≈ 3.37 x 10^7 m
Far-field divergence angle ≈ 9.39 x 10^-8 degrees
Spot size at the moon ≈ 1.39 x 10^4 m

These calculations provide insights into how different earth-based sources and initial waist sizes impact the Rayleigh range, far-field divergence angle, and spot size at the moon. Each scenario offers unique parameters and considerations based on the source used and the initial beam waist size.

Calculate Rayleigh Range, Far-field Divergence Angle, and Spot Size at the Moon

Calculation Process

Formula Used

Specific Calculations

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