Beam Spread
Beam spread, or angular width, defines how light from a source diverges and distributes in space. It's crucial in photometry, lighting design, and optical engin...
Beam divergence is the angular measure of how much a collimated light beam spreads as it travels. It affects how light is transmitted, focused, and applied in communication, metrology, industry, and science.
Beam divergence is a fundamental concept in optics and photonics, describing the angular spread of a collimated beam of light—such as that produced by lasers, LEDs, or other focused sources—as it propagates through space. It is central to the design and analysis of optical systems, directly influencing how efficiently light can be transmitted, focused, or directed over a distance.
Beam divergence is typically expressed as an angle (half-angle or full-angle), in units of milliradians (mrad) or degrees. It quantifies how rapidly the beam diameter (or radius) increases as it moves away from the beam waist—the narrowest point along the beam’s axis. Due to the wave nature of light and the phenomenon of diffraction, no real beam can remain perfectly parallel indefinitely. As a result, understanding and controlling beam divergence is vital in a wide range of applications, from free-space optical communication and laser material processing to alignment, metrology, and scientific imaging.
For example, in free-space communication, a low-divergence beam is necessary to keep the signal strong over long distances, minimizing loss and ensuring the beam fits within the receiver’s aperture. In industrial laser cutting or welding, divergence influences how small and intense the focus spot can be. In scientific instruments, it affects spatial resolution and measurement accuracy.
Most laser beams exhibit small divergences, so the angle is often quoted in milliradians (1 mrad = 0.0573°).
Geometric (far-field) definition:
When beam diameters ( D_1 ) and ( D_2 ) are measured at positions ( z_1 ) and ( z_2 ):
$$ \theta = \arctan\left(\frac{D_2 - D_1}{2(z_2 - z_1)}\right) $$
For small angles, ( \arctan(x) \approx x ) (in radians).
For a Gaussian beam:
The minimum (diffraction-limited) half-angle divergence is:
$$ \theta = \frac{\lambda}{\pi w_0} $$
Where:
Beam Parameter Product (BPP): $$ \text{BPP} = w_0 \cdot \theta $$
This value is constant for a given wavelength and beam quality and is a key metric for how well a beam can be focused or collimated.
For non-Gaussian beams (such as those from LEDs or multimode lasers), divergence may be defined by the Full Width at Half Maximum (FWHM) of the intensity profile, or by the angular width where intensity falls to half its maximum.
Diffraction inherently limits the minimum divergence for any beam of finite size. For a perfectly collimated Gaussian beam, the lower bound is:
$$ \theta_\text{min} = \frac{\lambda}{\pi w_0} $$
A smaller waist implies greater divergence, and vice versa—a direct consequence of the uncertainty principle and Fourier optics.
The beam quality factor ( M^2 ) (M-squared) quantifies how closely a real beam approximates an ideal Gaussian beam:
The divergence for a real beam becomes:
$$ \theta = M^2 \frac{\lambda}{\pi w_0} $$
A higher M² means the beam spreads more quickly and cannot be focused as tightly.
Measure beam diameter at two (or more) distant points; calculate divergence from the change in diameter over distance.
$$ \theta = \frac{D_2 - D_1}{2(z_2 - z_1)} $$
Collimate the beam with a lens of known focal length ( f ); measure the spot size ( w_f ) at the focus:
$$ \theta = \frac{w_f}{f} $$
Record beam size at multiple points along propagation; fit to the propagation equation to extract waist, divergence, and M² (per ISO 11146).
Advanced tools (Shack–Hartmann sensors, spatial Fourier analysis) can derive divergence from the phase and amplitude profile in a single plane.
| Term | Definition |
|---|---|
| Beam Waist | The location where the beam diameter is smallest; reference point for divergence and Rayleigh range. |
| Rayleigh Range | Distance from waist to where beam area doubles; marks transition from near to far field. |
| M² Factor | Quantifies beam quality; indicates how close the beam is to an ideal Gaussian. |
| Collimated Beam | Beam with minimal divergence, maintaining nearly constant diameter over long distances. |
| Beam Parameter Product (BPP) | Product of waist radius and divergence half-angle; sets fundamental focus/collimation limit for a given beam. |
| Parameter | Symbol | Formula | Units |
|---|---|---|---|
| Beam Waist Radius | ( w_0 ) | — | m, mm, µm |
| Wavelength | ( \lambda ) | — | m, nm |
| Divergence Half-Angle | ( \theta ) | ( \lambda / (\pi w_0) ) (ideal) | rad, mrad, ° |
| M² Factor | ( M^2 ) | — | dimensionless |
| Beam Parameter Product (BPP) | BPP | ( w_0 \theta ) | m·rad |
| Rayleigh Range | ( z_R ) | ( \pi w_0^2 / (\lambda M^2) ) | m, mm, µm |
Online Calculators:
Beam divergence is the angular rate at which a beam radius increases with distance from the beam waist. For a diffraction-limited Gaussian beam, the half-angle divergence is ( \theta = \lambda / (\pi w_0) ).
Divergence affects how tightly a beam can be focused, how far it can travel before spreading, and how much energy reaches a distant point—all critical considerations in communications, processing, and scientific applications.
It can be measured by direct far-field diameter measurement, by focusing with a lens and measuring spot size, or by analyzing beam propagation and extracting M².
No. All real beams with finite waist must diverge due to diffraction. Perfectly non-divergent beams are not physically possible.
A higher M² means more divergence for the same waist, and a reduced ability to focus or collimate the beam.
Beam divergence is a key parameter for any application involving focused or collimated light, underpinning the performance, safety, and feasibility of modern optical technologies.
Beam divergence is most commonly defined as the angular rate at which a beam’s radius grows with distance from its narrowest point (beam waist). For a diffraction-limited Gaussian beam, the divergence half-angle θ (in radians) is θ = λ / (π w₀), where λ is the wavelength and w₀ is the waist radius. For real beams, divergence includes the beam quality factor M²: θ = M²·λ / (π w₀).
Beam divergence determines how tightly a beam can be focused, how far it can travel before spreading significantly, and how much energy reaches a distant target. It’s crucial in applications such as free-space communications, laser cutting, microscopy, and laser safety, affecting performance, precision, and design constraints.
Beam divergence can be measured using direct far-field diameter measurements, by focusing the beam with a lens and measuring the spot size at the focal plane, or by characterizing the beam’s propagation (including M²) over several points. Standards such as ISO 11146 outline best practices for accurate measurement.
No. Every real optical beam with a finite width or waist will diverge as it propagates due to diffraction—the wave nature of light. Perfectly non-divergent beams are not physically possible.
The M² factor quantifies the departure of a real beam from an ideal Gaussian beam. A higher M² means more divergence for a given waist size, limiting how tightly the beam can be focused or collimated.
Manage beam divergence for superior performance in laser applications, communications, and industrial processes with advanced optics and measurement tools.
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