NewExplore the PTI Laser Toolkit Fifteen interactive tools — beam geometry, fiber, wavelength, pulse timing and conversions. Open toolkit Close

Power Technology, Inc.

Laser Toolkit

Fifteen engineering calculators for laser specification and integration, including beam geometry, fiber coupling, wavelength, pulse timing, and unit conversions.

Wavelength

Wavelength Viewer

Visualize approximate perceived color and photopic response, with spectral region, frequency, photon energy, wavenumber, and detection guidance.

Green Visible
Photopic response V(λ)
89% of peak
Region
Visible
Frequency
563.5THz
Photon energy
2.331eV
Wavenumber
18,797cm⁻¹
View PTI green laser products →

Catalog wavelength: 532 nm

Drag the scale, tap a tick, or type a value

Beam & optics

Beam spread & irradiance

Calculate beam diameter and average or peak irradiance at a specified distance.

Beam diameter
Spot area
Average irradiance
Peak irradiance

Far-field approximation: diameter grows linearly as d₀ + θz. For an ideal Gaussian spatial profile, on-axis peak irradiance is twice the area-average value.

Beam & optics

Divergence from measurements

Calculate beam divergence from diameters measured at the aperture and a second axial position.

Full divergence
In degrees
Half-angle

Measure both diameters to the same convention — 1/e² or FWHM, but not one of each.

Beam & optics

Fan angle for line lasers

The minimum fan angle needed to cover a target width at a given distance.

Minimum fan angle
Width at 1 m

Line lasers are specified by fan angle. Select the next available angle at or above the calculated minimum; excess coverage can be masked.

Wavelength

Wavelength ↔ frequency

Convert between wavelength, optical frequency, and photon energy.

Photon energy
Period

Edit either field and the other follows. Uses c = 299,792,458 m/s in vacuum.

Wavelength

Wavenumber ↔ wavelength

Convert between reciprocal centimetres and wavelength in nanometres.

Relationship
λnm = 10⁷ ÷ ν̃

For a Raman shift, subtract the shift in cm⁻¹ from the excitation wavenumber, then convert the result back to nanometres.

Pulse & power

Duty factor

Calculate the fraction of each pulse period during which the source emits.

Duty factor
Pulse period
Off time

Duty factor rises with either a longer pulse or a faster repetition rate, and falls as the period lengthens.

Pulse & power

Pulse energy & average power

Calculate pulse energy, average power, and duty factor from peak power, pulse width, and repetition rate.

Temporal shape
Energy per pulse
Average power
Duty factor

Pulse width is treated as full duration for rectangular pulses and intensity FWHM for Gaussian pulses.

Assumptions & formulas
Rectangular: E = Ppeakτ Gaussian (FWHM): E ≈ 1.06447Ppeakτ Paverage = E × repetition rate

Peak power must describe the actual temporal peak. A measured pulse waveform should be integrated when its shape is not well represented by either option.

Conversions

Optical length units

Convert among length units commonly used in optics and spectroscopy.

Relationship
1 Å = 0.1 nm

Edit any field and the other two follow. Older spectroscopy literature quotes lines in Ångströms — 6328 Å is the HeNe red line.

Conversions

Temperature

Convert operating and storage temperatures among Celsius, Fahrenheit, and kelvin.

Relationship
°F = °C × 9/5 + 32

Laser-diode wavelength generally varies with junction temperature; values specified at 25 °C should not be assumed across the full operating range.

Beam & optics New

Gaussian propagation & focus

Model a Gaussian-like beam in free space or estimate the spot formed by a lens. Each section works independently.

Free-space propagation

Beam diameter X × Y
Rayleigh range X / Y
Full divergence X / Y

Lens focus — uses wavelength and M² above

Focused diameter X × Y
Confocal range X / Y
Approx. lens NA X / Y

Clear aperture is optional. Enter it to check for possible beam clipping.

Assumptions & formulas

Inputs are full 1/e² intensity diameters of a Gaussian-like beam. X and Y are solved independently. This calculator provides engineering estimates; it is not an ISO-compliant M² measurement.

zR = πw₀²/(M²λ); w(z) = w₀√[1+(z/zR)²] θ(full) = 2M²λ/(πw₀) wfocus ≈ M²λf/(πwlens); confocal range = 2πwfocus²/(M²λ)

ISO 11146 uses second-moment beam widths and separate treatment for general astigmatic beams. Use an M² value obtained from a validated measurement; entering 1 assumes an ideal Gaussian. ISO 11146-1 overview.

Discuss a custom beam requirement →

Beam & optics New

Fiber NA & acceptance angle

Calculate the acceptance cone of a step-index fiber and optionally check its normalized frequency.

Numerical aperture
Acceptance half / full angle
Approximate f-number
V-number

The V-number output requires both core diameter and wavelength.

Assumptions & formulas

Step-index, meridional-ray approximation. Material indices must be entered at the operating wavelength.

NA = √(n₁²−n₂²); θa = asin(NA/n₀) f/# ≈ 1/(2NA); V = (2πa/λ)NA

For a conventional step-index fiber, V < 2.405 is the usual single-mode cutoff criterion; actual coupling also depends on mode-field diameter, alignment and beam quality.

Explore PTI fiber-output lasers →

Conversions New

Optical loss & power budget

Combine component losses to estimate delivered power. Detector responsivity is optional.

Delivered power
Total transmission
Total loss
Detector current

Enter responsivity at the operating wavelength to estimate ideal photocurrent.

Assumptions & formulas
Ttotal = T₁T₂…; Pout = PinTtotal Loss(dB) = −10 log₁₀(T); P(dBm) = 10 log₁₀[P(mW)] Detector current I = responsivity(A/W) × Pout(W)

Losses are treated as independent scalar power losses. Polarization, back-reflection, detector saturation, coupling alignment and wavelength dependence are not modeled.

Browse PTI laser products →

Pulse & power New

Pulse fluence & peak irradiance

Calculate from either pulse energy or peak power while accounting for temporal and spatial pulse shape.

Known quantity
Temporal shape
Spatial profile
Peak fluence
Area-average fluence
Pulse energy
Peak power
Peak irradiance
Average power

For Gaussian spatial mode, diameters are full 1/e² intensity widths.

Assumptions & formulas

Rectangular temporal pulse: E = Ppeakτ. Gaussian temporal pulse with intensity FWHM τ: E = Ppeakτ√π/[2√(ln2)] ≈ 1.06447Ppeakτ.

A = πDxDy/4; Favg = E/A Gaussian spatial peak = 2 × area average; top-hat peak = area average Paverage = E × repetition rate

Real pulses and diode beams can depart from these ideal profiles. NIST notes that accurate peak-power work depends on resolving the actual waveform and detector impulse response. NIST SP 250-64.

Explore PTI pulsed diode lasers →

Beam & optics New

Refraction & window displacement

Solve a single interface, then optionally estimate lateral shift through a parallel window.

Refracted angle
Brewster angle
Critical angle
Lateral displacement
Path inside window

Angles are measured from the surface normal. Indices should correspond to the operating wavelength.

Assumptions & formulas
n₁sinθ₁ = n₂sinθ₂; θB = atan(n₂/n₁) θc = asin(n₂/n₁), only when n₁ > n₂ Lateral shift δ = t sin(θ₁−θ₂)/cosθ₂

The window calculation assumes plane, parallel surfaces and isotropic, nonabsorbing media. Coatings, wedge, dispersion and polarization-dependent Fresnel losses are not included.

Discuss your optical integration →

No matching tools. Suggested searches: divergence, duty factor, joules, or angstrom.

Results support preliminary engineering estimates and comparisons; they do not determine laser-safety classification. For hazard distances, eyewear selection, and exposure limits, apply the relevant IEC 60825 and ANSI Z136 requirements and consult a qualified laser-safety professional.

Divergence Calculation

Distance [m]:

Laser:
Power [mW]:
Divergence [mrad]:
Diameter at aperture [mm]:
Beam diameter after m: mm
Area of laser point after m: mm2
Laser intensity of uniform beam after m: mW/mm2

Find a laser beam's divergence

Specifications:
Distance from Laser Aperture -> Projection surface [m]:
Beam Waist Diameter at Laser Aperture [mm]:
Laser spot diameter at the projection surface [mm]:
The Full Divergence of the laser system is:
0.00 mrad

Calculating nanometers from wavenumber

To convert from wavenumber (cm-1) to nanometers, use the following equation: 1/cm-1 x 107 = nanometers. Or to convert from nanometers to wavenumber, you simply reverse the equation so that wavenumber (cm-1) = 107 / wavelength in nanometers. Or use the tool below.

Converting angstroms to nanometers

To convert from angstroms to nanometers, use the following equation:

1 angstrom = 0.1 nanometer. Or use the tool below.

Converting fahrenheit to celsius

To convert from fahrenheit to celsius, use the following equation:

32° Fahrenheit = 0° Celsius. Or use the tool below.

Converting watts to joules

Power is measured in Watts, named after James Watt (1736-1819). Joules (named after James Prescott Joule, 1818-1889) are units of energy. Use the following equation to convert from Watts to Joules.

1 Watt = 1 Joule per second of power

Fan Angle Calculator


To achieve your desired projection, select a minimum fan angle of: 67 degrees

Meters




Centimeters




Feet




Inches



37m
49m
Meters         Centimeters         Feet         Inches      

Converting wavelength to frequency



Wavelength (nm):


Frequency (Hz):


Result:

You can use the following equation to convert wavelength to frequency:

v (Hz) = 2.998 x 1017 / wavelength (nm).

Calculating duty factor

Duty factor (also known as duty cycle) is the ratio of pulse duration to pulse period. Duty factor (Df) is calculated as follows.

Df = pulse duration (sec) / pulse repetition period (sec)

Multiply the result by 100 to get your answer as a percentage.

Please note that as pulse repetition frequency increases, duty factor increases. As pulse repetition period increases, duty factor decreases. As pulse duration increases, duty factor increases.

Contact Us

For custom quotes and more information about our laser technology services, please call, chat or submit our online form below.