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POWER-AUTOCORRELATION
 

POWER-AUTOCORRELATION 
ENLARGE

A circular auto-correlation of power vs. time produces this plot.  From the autocorrelation we can extract many more details about our signal.  The 1/e width- the time for the lightning signature to reach 36.79% of its peak value- is found.  If this value is less than 10 microseconds, we look further in time for a secondary echo. 

The local maximum after the 1/e time value is considered the secondary echo - even though it may not be an actual echo.  By computing the Signal-to-Noise Ratio (SNR) of this local maximum, we can determine whether or not we will consider it a secondary pulse.  The criteria is for SNR to be greater than or equal to 5 dB. 

SNR is calculated using 10*log(secondary peak/background noise). Background noise is considered the average value of the last 10% of the autocorrelation function).

 
Power versus Time Return Home Compression
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 Detailed Procedure

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CIC - 3  | c3webmeister@c3.lanl.gov | LANL | Copyright © UC 1998 | Disclaimer | 25 June 1998
Shane Crockett <m991368@nadn.navy.mil>  and C M Brislawn <brislawn@jacobs.c3.lanl.gov>