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DEEP DESERT LABS / TOOLS

Optics / 03 / Pulses

Energy, rate,
and the peak.

Relate pulse energy, repetition rate and average power, and find the peak power for a stated pulse shape and duration.

Peak power depends on the shape. Energy divided by duration is only the peak of a flat-top pulse. Choose the shape that describes your pulse. Runs in your browser; nothing is sent or stored.

Pulse train

Temporal shape of the power P(t)
Full width at half maximum of the intensity, not of an autocorrelation trace.
Leave empty for a single pulse.
Known quantity

Result

Peak power P_peak
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Average power
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Shape factor k = P_peak τ / E
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Pulse period 1/f
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Duty factor f τ
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Peak / average
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Train peak including neighbours
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Results to 4 significant figures. Displayed digits are not a measurement uncertainty.

Model and limits

Ppeak=kEτ

peak power; τ is the FWHM of the power P(t)

Pavg=Efrep

average power

P(t)∝exp(−4ln2t2τ2),k=2ln2π≈0.9394

Gaussian pulse

P(t)∝sech2(1.7627tτ),k=ln(1+2)≈0.8814

sech² pulse

k=1

rectangular (flat-top) pulse of length τ

Ptrain=Ppeak(1+2∑m≥1p(mfrepτ))

peak of a train: the neighbours add their tails; p is the unit-peak shape

  • τ is the full width at half maximum of the optical power (intensity) in time. An intensity autocorrelation is wider by 1.414 (Gaussian) or 1.543 (sech²); divide by that factor first.
  • Every pulse in the train is identical and isolated. Satellite pulses, pedestals, ASE or a CW background carry energy without adding to the peak; the result is then an upper bound on the peak power.
  • P_peak is the peak of one isolated pulse. In a train the tails of the neighbours add at each peak: P_train = P_peak (1 + 2 Σ p(m / f τ)), with p the unit-peak shape. The sum is negligible at f τ = 0.1 (below 10⁻¹⁵) and reaches 0.003 % (Gaussian) or 0.7 % (sech²) at f τ = 0.5; it is shown when it exceeds 0.1 %. The page refuses f τ above 0.5 (Gaussian, sech²) or 1 (rectangular), where the train is close to continuous.
  • Peak power is not peak intensity: intensity also needs the beam area and spatial profile.

Sources

  • The shape factors follow from integrating each P(t): E = ∫P dt. For sech², ∫sech²(t/T) dt = 2T and τ = 2 acosh(√2) T.
  • J.-C. Diels and W. Rudolph, Ultrashort Laser Pulse Phenomena, 2nd ed. (Academic Press, 2006): pulse-shape and autocorrelation width factors.
  • Same shape factors as the LaserShark modules physics/amplifier.py and physics/damage.py.