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M squared

M², also known as the beam quality factor or beam propagation factor, is a dimensionless parameter in laser optics that quantifies the quality of a laser beam by comparing its divergence and focusability to those of an ideal diffraction-limited Gaussian beam of the same wavelength.^[1]^[2] For a perfect single-mode TEM₀₀ Gaussian beam, M² equals 1, indicating the theoretical minimum divergence and spot size; values greater than 1 signify deviations due to multimode content, aberrations, or other imperfections that increase beam spread.^[3]^[1] The parameter is formally defined by the International Organization for Standardization (ISO) in standard 11146 as the ratio of the actual beam parameter product—defined as the product of the beam waist radius w₀ and the far-field divergence half-angle θ—to that of an ideal Gaussian beam.^[1]^[2] Mathematically, this is expressed as M² = (π w₀ θ) / λ, where λ is the wavelength of the light.^[3] This formulation allows M² to predict beam behavior throughout propagation, with the beam radius at any position z given by w(z) = w₀ √[1 + (M² z λ / (π w₀²))²], extending the Gaussian beam propagation equation to real beams.^[1]^[3] Measurement of M² follows the ISO 11146 protocol, which requires profiling the beam at multiple positions along its propagation path—typically five locations in the near field, waist, and far field—using techniques such as scanning-slit or knife-edge profilers to determine width, waist location, and divergence.^[2]^[1] Commercial systems automate this process by focusing the beam with a lens and scanning the profile over a range of propagation distances, often yielding results in seconds while ensuring accuracy for beams from continuous-wave to pulsed lasers.^[3]^[2] The significance of M² lies in its direct impact on laser performance in practical applications, as lower values enable tighter focusing for higher power density, reduced divergence for efficient beam delivery over distance, and better coupling into optical fibers or resonators.^[1]^[3] In fields like materials processing, where focused spot size determines cutting or welding precision, or in medical lasers requiring minimal thermal spread, optimizing M² is essential for maximizing effective power and system efficiency.^[3] It also serves as a key specification for laser manufacturers and system integrators to verify compliance with design goals and predict integration challenges.^[3]

Fundamentals

Definition

The beam quality factor M^2, also known as the beam propagation factor, is a dimensionless parameter that quantifies the quality of a laser beam by measuring its deviation from the diffraction-limited performance of an ideal Gaussian beam.^[4] It provides a single, propagation-invariant metric to characterize how effectively a beam can be focused and its overall coherence, with values closer to unity indicating higher quality.^[4] For a fundamental Gaussian mode, which represents the ideal transverse electromagnetic mode with the lowest divergence, M^2 = 1.^[5] In contrast, real laser beams typically have M^2 > 1 due to contributions from higher-order multimodes, phase aberrations, or thermal distortions that degrade the beam's spatial profile and increase divergence.^[5] The M^2 concept originated in the early 1990s, introduced by Anthony E. Siegman as a standardized, invariant measure of beam quality that remains constant through linear optical systems, building on earlier work in laser resonator theory.^[4] A fundamental relation defining M^2 is

M^2 = \frac{\pi w_0 \theta}{\lambda},

where w_0 is the $1/e^2 beam waist radius, \theta is the far-field half-angle divergence, and \lambda is the wavelength in the propagation medium.^[5] This expression scales the product of the beam's minimum width and divergence relative to the diffraction limit for a Gaussian beam.^[5]

Physical Interpretation

The M² factor provides a measure of how closely a laser beam approximates the ideal diffraction-limited behavior of a fundamental Gaussian mode, with values greater than 1 indicating deviations due to higher-order modes or aberrations that degrade performance. Physically, an M² > 1 results in a larger beam size at the focus and increased far-field divergence compared to an ideal Gaussian beam of the same input waist size and power, leading to a corresponding reduction in peak intensity and overall brightness. This degradation arises because the beam parameter product (waist radius times divergence angle) scales linearly with M², effectively spreading the energy over a larger phase-space volume.^[5] For instance, a beam with M² = 2 will produce a focused spot whose area is four times that of an ideal Gaussian beam when propagated through the same focusing optics, quartering the achievable intensity for a given power level. Such effects limit the beam's utility in applications demanding high spatial resolution, as the excess divergence causes faster beam expansion over distance, reducing the effective range for maintaining collimation.^[5] The impact on brightness further underscores these limitations, as M² governs an invariant quantity conserved through lossless paraxial optics. The beam brightness B, representing the maximum radiance, is expressed as
B = \frac{P}{ \frac{M^4 \lambda^2}{4 \pi^2} },
where P is the total optical power and λ is the wavelength; this relation shows that brightness scales inversely with M⁴, imposing a fundamental limit on the intensity that can be concentrated in the focal spot regardless of focusing optics.^[6] Conceptually, the M² factor draws an analogy to light propagation in multimode optical fibers, where higher values correspond to the excitation and mixing of multiple transverse modes, increasing the effective numerical aperture and mimicking the reduced coherence and higher divergence observed in multimode fiber outputs compared to single-mode counterparts.^[7]

Mathematical Formulation

Gaussian Beam Baseline

The Gaussian beam represents the ideal, diffraction-limited case in laser optics, serving as the baseline for the M² beam quality factor, where M² = 1 indicates perfect beam quality.^[8] Its radial intensity profile at any propagation distance z is described by the equation I(r, z) = I_0 \exp\left(- \frac{2 r^2}{w(z)^2}\right), where I_0 is the peak intensity at that z, r is the radial distance from the beam axis, and w(z) is the beam radius at which the intensity falls to $1/e^2 of its peak value.^[8] The beam radius varies with propagation distance z according to w(z) = w_0 \sqrt{1 + \left( \frac{z}{z_R} \right)^2}, with w_0 denoting the minimum beam waist radius at z = 0, and the Rayleigh range z_R = \pi w_0^2 / \lambda defining the distance over which the beam area doubles.^[8] These expressions capture the fundamental paraxial propagation characteristics of the Gaussian beam, ensuring power conservation and minimal diffraction spread.^[8] The far-field divergence half-angle θ for this ideal beam is given by \theta = \lambda / (\pi w_0), where λ is the wavelength, establishing the minimum angular spread achievable for a given waist size and confirming M² = 1.^[5] This divergence arises directly from the wave nature of light and sets the reference for assessing deviations in real beams via the M² factor. A key metric for the Gaussian beam is the beam parameter product (BPP), defined as the product of the waist radius w₀ and the divergence half-angle θ, yielding BPP = λ / π as the fundamental limit for beam brightness and focusability.^[9] This invariant quantity underscores the beam's optimal performance in applications requiring tight focusing. Propagation through free space preserves certain invariants for the Gaussian beam, notably the product w(z) θ remaining constant along z, which reflects the absence of beam degradation.^[8] Similarly, the beam quality factor M² = 1 is invariant under linear optical transformations, providing a stable reference for comparing real laser beams to this ideal profile.

General Beam Propagation

The beam propagation factor M^2 provides a framework for characterizing the quality of arbitrary laser beams beyond the ideal Gaussian case, where M^2 = 1. For a general beam, the key propagation parameters—the waist radius w_0 and far-field divergence angle \theta—are related by the product w_0 \theta = M^2 \lambda / \pi, where \lambda is the wavelength. This relation generalizes the Gaussian beam baseline, scaling the beam parameter product by M^2 to account for deviations from diffraction-limited performance. The propagation of such beams can be modeled using the Gaussian beam equations with the wavelength replaced by an effective wavelength \lambda_{\text{eff}} = M^2 \lambda, or equivalently, with the Rayleigh range scaled as z_{R,\text{eff}} = z_R / M^2, while using the actual waist radius w_0. This approach preserves the beam waist at z=0 and correctly scales the divergence, facilitating predictions in optical system design.^[5] The value of M^2 for an arbitrary beam is derived from intensity-weighted second moments of the transverse position and angular coordinates, providing a rigorous, propagation-invariant measure. Specifically, in the x-direction (with analogous expressions for y), M^2 = \frac{4\pi}{\lambda} \sqrt{\langle x^2 \rangle \langle \theta_x^2 \rangle - \langle x \theta_x \rangle^2}, where the moments are defined as \langle f \rangle = \frac{\int f(x, \theta_x) I(x, \theta_x) \, dx \, d\theta_x}{\int I(x, \theta_x) \, dx \, d\theta_x} over the intensity distribution I. This formulation, rooted in the uncertainty principle analogy for paraxial beams, quantifies the correlation between position and momentum-like angle, with \langle x \theta_x \rangle capturing beam tilt or astigmatism; for uncorrelated, centered beams, it simplifies to M^2 = \frac{4\pi}{\lambda} \sqrt{\langle x^2 \rangle \langle \theta_x^2 \rangle}. These moments are evaluated at the beam waist for \langle x^2 \rangle and in the far field for \langle \theta_x^2 \rangle, standardized in ISO 11146 to ensure consistency across measurements.^[4] An alternative theoretical perspective on M^2 arises from expanding the beam into a complete set of orthogonal eigenmodes, such as Laguerre-Gaussian or Hermite-Gaussian modes, analogous to the Fox-Li method for resonator eigenmodes. In this approach, M^2 represents the ratio of the actual eigenvalue spectrum (or modal content) of the beam to that of an ideal single-mode Gaussian, weighted by the power in each mode. For instance, a beam comprising multiple modes has M^2 = \sum_k p_k (2k + 1), where p_k is the fractional power in the k-th order mode and the factor (2k + 1) reflects the increased divergence of higher-order modes relative to the fundamental. This modal decomposition highlights M^2 as a global measure of modal purity, with values exceeding 1 indicating excitation of higher-order components that degrade focusability.^[4] The parameter M^2 exhibits invariance under paraxial optical transformations, including free-space propagation, thin lenses, and amplifiers, making it a robust figure of merit for beam evolution. During free-space propagation over distance z, the second moments evolve according to the beam matrix formalism, but the determinant \langle x^2 \rangle \langle \theta_x^2 \rangle - \langle x \theta_x \rangle^2 remains constant, preserving M^2. Similarly, for a lens with focal length f, the ABCD ray-transfer matrix transforms the moments while conserving the symplectic invariant tied to M^2. In amplifiers, gain uniformity maintains M^2 if the beam remains paraxial, as demonstrated in multimode fiber amplification where initial M^2 \approx 20 persists post-amplification without introducing new aberrations. These properties ensure M^2 reliably predicts long-term beam behavior in complex systems.^[4]

Measurement Methods

Experimental Techniques

The primary experimental techniques for measuring the M² beam quality factor involve scanning or imaging the laser beam at multiple propagation distances to determine its waist size and divergence, enabling computation of M² through fitting to beam propagation models. These methods typically require a controlled laboratory setup with beam attenuation to prevent detector saturation, precise translation stages for z-positioning, and detectors such as photodiodes or cameras to capture intensity profiles. Measurements are performed in both near-field and far-field regions to capture the hyperbolic beam width evolution, w(z), with data fitted to extract the beam waist w₀ and Rayleigh range z_R. The slit-scanning method uses a narrow slit translated across the beam transverse profile at various z-positions to record transmission curves, from which the beam radius w(z) is derived by analyzing the intensity variation. The slit width is chosen to be much smaller than the beam diameter (typically <10% of w(z)) to minimize diffraction effects, and the scanning is repeated at least 10 planes spanning from near the waist to beyond the Rayleigh range on both sides. Once w(z) data are collected, they are fitted to the hyperbolic form w(z) = w₀ √(1 + (z/z_R)²), yielding w₀ and z_R; M² is then computed as M² = π w₀² / (λ z_R), where λ is the wavelength. This technique, applied to multimode lasers like Nd:YVO₄, has demonstrated M² values around 1.5–2.0 for verifying multi-mode operation.^[10] The knife-edge technique similarly involves translating a razor edge across the beam to measure the transmitted power as a function of edge position, allowing reconstruction of the intensity profile and calculation of the second-moment beam width, which is robust to noise and aligns with established measurement protocols. At each z-plane, the edge scan captures the cumulative intensity distribution, from which the beam radius is determined as the distance between points yielding 15.9% and 84.1% transmission (corresponding to the 1/e² width for Gaussian beams). Multiple scans (at least 10 planes) provide w(z) data for fitting, with the method particularly suited for high-power pulsed lasers due to its simplicity and accuracy in deriving second moments. Error analysis in this approach shows that misalignment of the edge can introduce up to 5% uncertainty in w(z), mitigated by averaging multiple scans.^[11] Direct far-field imaging employs CCD or CMOS cameras to capture the beam's intensity profile at a sufficient distance (typically >10 z_R) or after focusing with a lens, directly measuring the divergence angle θ as the half-angle to the 1/e² intensity points. The camera is positioned to image the far-field pattern, with pixel resolution ensuring at least 10 pixels across the beam diameter; the waist w₀ is inferred from near-field images or propagation back-calculation, while θ is fitted from the Gaussian far-field profile. Combining these with near-field data allows M² computation via the relation involving the product w₀ θ relative to the diffraction limit. This method is efficient for real-time assessment but requires careful calibration to account for lens aberrations. A general step-by-step procedure for these techniques begins with beam truncation using an aperture slightly larger than the 1/e² diameter (1.1–1.5 times) to isolate the fundamental mode and reduce higher-order contributions, followed by focusing the beam with a low-aberration lens to access the waist region. Measurements are conducted at a minimum of 10 z-planes: five in the near field (around the waist) and five in the far field, with z-spacing chosen to adequately cover the near and far fields for optimal fitting sensitivity. Data fitting uses least-squares optimization to extract parameters, with M² derived from the ratio of measured to ideal Gaussian propagation. Common error sources include aperture truncation effects and detector noise or misalignment, addressed through averaging and alignment verification.^[12]

Standardization and Equipment

The ISO 11146 series of standards, first published in 1999 and revised in 2021, provides the international framework for characterizing laser beam propagation, including the M² factor for multimode and astigmatic beams.^[12] These standards outline procedures requiring measurements of beam width at a minimum of 10 planes along the propagation axis—typically five within one Rayleigh length and five beyond—to ensure accurate determination of beam parameters like divergence and waist location.^[13] The methodology emphasizes minimizing systematic errors to achieve an uncertainty of less than ±5% in second-moment calculations, applicable to both continuous-wave and pulsed laser systems.^[14] Commercial M² meters, such as those from Ophir and Thorlabs, implement these ISO-compliant techniques using automated hardware for precise beam profiling. Ophir's BeamSquared systems employ CCD camera arrays to capture beam caustics across UV to near-IR wavelengths, supporting both slit-scanning and imaging modes for CW and pulsed lasers up to 20 meters Rayleigh length. In 2025, Ophir introduced the BeamSquared SP204S-PRO, enhancing precision with 3% astigmatism accuracy.^[15]^[16] Thorlabs' M² measurement kits integrate CMOS beam profilers with motorized translation stages and focusing optics, enabling turnkey evaluation of divergence, waist position, and M² in under 30 seconds for beams from 400 to 2700 nm.^[2] These devices often feature software that automates ISO 11146 data fitting, reducing operator variability. Calibration of M² meters relies on reference Gaussian beams with M² values near 1.01 to verify system accuracy against the ideal TEM₀₀ mode.^[5] For astigmatic beams, standards mandate separate x- and y-axis measurements, yielding M²_x and M²_y to account for directional differences in propagation. Advancements in artificial intelligence have incorporated it for enhanced moment-based calculations, as seen in machine learning models that predict M² from single-shot profiles, improving speed and robustness for fiber and multimode sources.^[17] Additionally, systems now better handle ultrafast pulses through high-frame-rate cameras and pulse-resolved profiling, enabling real-time M² assessment without temporal averaging effects.^[18]

Applications

Laser System Design

In laser resonator design, the M² factor plays a crucial role in optimizing cavity modes to achieve near-diffraction-limited beam quality, as lower values enable tighter focusing and efficient energy extraction. Stable resonators, such as those employing symmetric or dynamically stable configurations, are engineered to support fundamental Gaussian-like modes, typically yielding M² values between 1.1 and 1.5 for high-power systems like Yb:YAG thin-disk lasers. For instance, a simple stable resonator in a 1.1 kW Yb:YAG thin-disk laser has demonstrated an M² < 1.4 by minimizing higher-order mode excitation through precise mirror curvature and gain medium placement. This optimization reduces beam divergence and enhances overall system efficiency, guiding the selection of resonator parameters like mirror reflectivity and cavity length to suppress modal instabilities. In fiber and disk lasers, M² values directly influence mode selection and power scaling strategies. Single-mode fiber lasers achieve excellent beam quality with M² ≈ 1.1, ideal for precision applications, while multimode configurations exhibit higher values ranging from 5 to 20, depending on the number of supported modes and core size. To improve effective beam quality in multimode fiber lasers, techniques such as cladding mode stripping are employed, where devices like etched or epoxy-filled sections attenuate higher-order cladding modes, reducing unwanted power leakage and stabilizing the output M² closer to single-mode performance. Disk lasers, particularly thin-disk designs, leverage their geometry to maintain low M² (e.g., averaged 1.55 in dynamically stable setups) by distributing heat evenly, minimizing thermal distortions that could excite multimodes. Amplification processes often lead to M² degradation due to thermal lensing in the gain medium, where nonuniform heating induces refractive index gradients that distort the wavefront and broaden the beam. In end-pumped solid-state amplifiers, this effect can increase M² by factors of 2-5 at high powers, as observed in Nd:YAG systems where thermal aberrations couple energy into higher modes. Mitigation strategies include beam shaping optics, such as aspheric lenses or phase plates, which precondition the input beam to counteract lensing effects, preserving M² below 2 even at kilowatt levels by flattening the intensity profile and compensating for aberrations. A representative example is diode-pumped solid-state (DPSS) lasers used in high-power cutting applications, where targets of M² < 1.3 ensure deep penetration and minimal kerf width. In sub-nanosecond DPSS systems delivering up to 250 W, this beam quality enables precise material removal in metals, with thermal lensing mitigated through optimized pumping geometries and beam expanders to maintain focus stability over extended operation.

Beam Quality Assessment

In optical systems, the M² factor enables straightforward propagation modeling by scaling the standard Gaussian beam equations, effectively replacing the wavelength λ with M² λ to account for the beam's deviation from ideal diffraction-limited behavior. This adjustment allows prediction of beam parameters such as waist size and divergence at any propagation distance using established Gaussian propagation codes. For instance, the focused spot size w_focus after passing through a lens of focal length f, starting from an input beam waist w_in, is given by w_focus = M² (λ f / (π w_in)), highlighting how higher M² values lead to larger focal spots and reduced intensity concentration.^[4] Assessing system efficiency often involves evaluating power coupling into optical fibers, where the maximum transferable power to a single-mode fiber scales inversely with M⁴ due to conservation of beam brightness and etendue; the effective etendue of the beam increases as (M²)², limiting the fraction of power that matches the fiber's fundamental mode. This scaling underscores M²'s role in optimizing delivery systems, as beams with M² > 1 exhibit reduced coupling efficiency, necessitating compensatory measures like mode matching optics.^[5] Compared to other quality metrics, M² offers advantages in beam assessment due to its propagation invariance, remaining constant regardless of distance or focusing, unlike the Strehl ratio—which quantifies peak intensity degradation from wavefront aberrations and varies with propagation—or encircled energy, which measures energy within a fixed aperture but depends on specific spot sizes. M² is thus preferred for comprehensive system-level predictions, as it integrates both near- and far-field characteristics into a single, conserved parameter suitable for diverse optical configurations.^[4] In industrial applications, such as CO₂ laser welding, M² values typically range from 1.5 to 3 for multimode systems, directly impacting process efficiency; lower M² enables tighter focusing and higher energy density for deeper penetration and faster welding speeds, while values above 2.5 may reduce weld quality due to broader spots and increased heat-affected zones. For example, slab CO₂ lasers with M² ≈ 1.4 achieve enhanced performance in high-power welding tasks compared to higher-M² unstable resonator designs.^[19]

Theoretical Extensions

Embedded Gaussian Model

The embedded Gaussian model provides an approximation for analyzing the propagation of real laser beams that deviate from the ideal Gaussian profile due to higher-order modes or aberrations. In this framework, a real beam is treated as equivalent to a fundamental Gaussian beam but with an effective wavelength \lambda_\mathrm{eff} = M^2 \lambda, where \lambda is the actual wavelength and M^2 is the beam quality factor. This scaling ensures that the beam waist size w_0 and far-field divergence \theta of the real beam match those of the embedded Gaussian, while preserving key invariants like the beam parameter product w_0 \theta = M^2 \lambda / \pi. The model is particularly useful for paraxial beams, where the transverse field distribution can be represented as a superposition of modes "embedded" within a scaled Gaussian envelope, allowing the overall propagation to mimic that of a diffraction-limited beam at the effective wavelength. Mathematically, the model derives from the paraxial wave equation, where the real beam's spot size evolution w(z) follows the Gaussian form but with a modified Rayleigh range z_R = \pi w_0^2 / (M^2 \lambda):

w(z) = w_0 \sqrt{1 + \left( \frac{z M^2 \lambda}{\pi w_0^2} \right)^2}.

This equation arises because higher-order modes contribute to an effective increase in the phase-front curvature and diffraction, effectively embedding them within the fundamental mode's envelope scaled by M. The validity holds under the paraxial approximation, assuming small angles and negligible non-linear effects, as originally formulated for resonator modes and extended to free-space propagation. In applications, the embedded Gaussian model simplifies simulations of beam propagation through optical systems using ABCD matrix methods, where the complex beam parameter q is adjusted by incorporating M^2 to account for non-ideal behavior without computing full modal expansions. Similarly, it facilitates modal decomposition in laser design by treating the beam as a single effective Gaussian, reducing computational complexity for predicting focusability and throughput in systems like amplifiers or focusing optics. For instance, in resonator analysis, it allows quick estimation of mode stability by scaling the Gaussian resonator parameters. The model's accuracy diminishes for highly aberrant or strongly multimode beams with M^2 > 10, where the embedded approximation fails to capture detailed mode interactions or non-paraxial effects, necessitating full eigenmode analysis or advanced metrics like the Strehl ratio for precise characterization.

Limitations and Advanced Metrics

The M² factor is predicated on the paraxial approximation, which assumes small propagation angles relative to the optical axis, enabling the use of simplified Gaussian beam propagation equations scaled by M².^[5] It further assumes rotational symmetry in the beam's intensity profile, treating the beam as circularly symmetric for standard calculations.^[5] While insensitive to specific phase aberrations such as astigmatism—due to its reliance on second-moment widths—M² can be extended to astigmatic beams by computing directionally resolved values, M²_x and M²_y, to quantify asymmetry.^[5] Despite its utility, M² exhibits key limitations, particularly for beams deviating from ideal Gaussian forms. It fails to adequately characterize non-stationary beams, such as those in pulsed lasers where temporal variations in profile occur, as M² averages over the field and overlooks dynamic instabilities.^[3] For beams with hard edges or uniform intensity profiles, like flat-top beams, M² overestimates degradation in quality by assigning values greater than 1, even when such profiles are advantageous for uniform illumination applications, due to its emphasis on far-field divergence over central flatness.^[20] Additionally, M² can yield values less than 1 for superpositions of axially shifted Gaussian beams or incoherent mixtures with differing waists, violating its intended lower bound and highlighting inconsistencies for partially coherent or structured fields.^[21] To address these shortcomings, advanced metrics incorporate higher-order moments or modal content for more nuanced assessment. The kurtosis parameter, a fourth-moment-based measure often linked to an effective M⁴ factor for flat-top beams, quantifies profile flatness or sharpness, with values approaching 1.8 for ideal flat-tops versus 2 for Gaussians; it complements M² by enabling size-independent characterization and accurate M² prediction via relations like the Padé approximation.^[22]^[23]

k = \frac{\int_{-\infty}^{\infty} x^4 I(x) \, dx}{\left( \int_{-\infty}^{\infty} x^2 I(x) \, dx \right)^2}

where I(x) is the intensity and k > 2 indicates peaked profiles while k < 2 signals flatness.^[22] Beam propagation factors extended to higher moments, such as fourth-order variants, generalize M² to capture excess kurtosis in propagation, providing better fidelity for non-Gaussian beams.^[24] TEM mode content analysis via modal decomposition into Hermite-Gaussian bases yields the modal spectrum and computes M² as \sqrt{\sum (m + n + 1) |\rho_{mn}|^2}, where \rho_{mn} are modal coefficients, revealing higher-order mode contributions that degrade quality.^[25] Advanced metrics have also been developed for vector beams, such as the vector quality measure introduced in 2016, which quantifies the degree of vectorial nature from 0 (purely scalar-like) to 1 (purely vectorial) and evaluates non-separable polarization-spatial correlations in cylindrically polarized or vortex beams. This is essential for applications in quantum optics, like entanglement distribution. Extensions include calculations of the M² factor specifically for vector Schell-model beams, as explored in 2019.^[26]^[27]

References

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Beam Quality and Strehl Ratio
### Summary of M² Beam Quality Factor
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Complete M² Measurement Systems - Thorlabs
The M2 factor, also called the beam quality factor or the beam propagation factor, is a measure of the quality of a beam. This parameter is defined as the ...<|control11|><|separator|>
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The M 2 factor (M squared factor), also called beam quality factor or beam propagation factor, is a common measure of the beam quality of a laser beam.Missing: original | Show results with:original
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The« M 2 factor» is a kind of measurement of the “degradation” of the beam quality compared to the fundamental Gaussian beam, taken as reference.<|separator|>
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The beam parameter product is the product of focus beam radius and far-field half-angle beam divergence. It quantifies beam quality.Missing: (4π) | Show results with:(4π)
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The M2 factor describing the quality of the beam can be obtained by scanning a slit through the multi-mode Gaussian beam field.Missing: M² | Show results with:M²
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Aug 6, 2025 · The knife-edge method, is relatively simple to operate, and has high accuracy, which is well-suited for measuring high-peak-power pulsed lasers.
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Beam propagation (M 2 ) measurement made as easy as it gets
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In stock 2–5 day deliveryThis document specifies methods for measuring beam widths (diameter), divergence angles and beam propagation ratios of laser beams.Missing: history | Show results with:history<|separator|>
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Jun 1, 1999 · ISO 11146 is a standard for test methods for laser beam parameters, including beam widths, divergence angle and beam propagation factor.
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BeamSqured solutions for measurement of M² ranging from simple manual processes to fully automated dedicated instruments.
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Deep learning enabled superfast and accurate M 2 evaluation for ...
We introduce deep learning technique to predict the beam propagation factor M2 of the laser beams emitting from few-mode fiber for the first time, ...
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The beam quality of multimode high power Nd:YAG beams is poor compared to CO₂ beams (M² ≤5) of similar powers. Consequently processing speed and penetration ...
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Here we introduce a quantitative beam quality measure for vector beams and demonstrate it on cylindrical vector vortex beams.