Temporal energy centroid of an optical pulse

ID: temporal-energy-centroid-of-an-optical-pulse

The temporal energy centroid of an optical pulse is its energy-weighted mean time. For nonnegative radiant power with finite positive energy and finite absolute first moment,
The normalization uses radiant energy as integrated radiant flux.[ref] The centroid is a moment of the energy-normalized pulse profile; it need not coincide with the largest power value, a threshold crossing or the middle of the FWHM interval.
For an original two-component example, let ninety percent of the energy belong to a symmetric narrow component centred at zero and ten percent to a symmetric component centred at . Linearity of the integral gives . Weak delayed energy can move the centroid even when the dominant peak remains near zero. Multiplying the whole power trace by a positive constant leaves unchanged; translating it by shifts its centroid by .
A detector response can shift the measured centroid too. Suppose a normalized impulse response and normalized optical profile have finite absolute first moments. For their convolution , direct integration with gives
Thus a causal exponential detector response of time constant shifts the recorded centroid by in this model. NIST's pulsed-radiometer characterization explicitly measures detector impulse responses and uses convolution to assess reproduced waveforms.[ref] The centroid identity is the independent moment calculation above.
Baseline drift can cause a separate shift. Suppose a true pulse has and , but a positive residual baseline of remains across the analysis window from to . Its added energy is , centred at . The resulting centroid is
A waveform measurement should therefore record the time window, baseline estimate and detector timing response with its reported centroid. A negative background-subtracted trace also needs care: it is not automatically a nonnegative energy distribution.

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