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CHAPTER
4
OPTIMIZING THE PULSE DURATION
USING CHIRPSCAN
4.1
Optimization
Once the ChirpScan algorithm is started, the software acquires several spectra and displays all the
acquired spectra in a 2D map (see figure
). A dialog panel then pops up and prompts the user
to proceed to the next step which can either be:
•
keep the current waveform without any modifications (
Keep Ref.WF as is
.)
•
compensate for the measured spectral phase (
Apply these corrections to Ref.WF
).
By selecting one or several check boxes, the user can choose to correct for any combinations of
second, third and fourth orders. The corresponding values of phase coefficients are displayed. The
central wavelength with respect to which these coefficients are defined (Taylor expansion of the
spectral phase) is also displayed as a reminder. The resulting correction is displayed on top of the
2D map and can be compared to the measured phase function (more precisely, to the second order
derivative of the spectral phase). If the corresponding option was selected in the configuration
panel of the ChirpScan algorithm, it is also possible to correct for the residual phase by selecting
”Correct residual phase numerically”.
At this point, the software leaves it to the user to check that the spectrometer did not saturate
at any moment during the scan, i.e. all units are below the maximum count in the 2D scan map.
In case this happens, the user is asked to press
Keep Ref.WF as is
, to adapt the input energy or
adjust the integration time of the spectrometer and run the ChirpScan measurement again.
By clicking on the button labeled
Apply these corrections to Ref.WF
, a new reference
waveform is computed based on the selected phase correction parameters and sent to the Dazzler.
The ChirpScan algorithm can be run again to monitor the effects of the phase corrections and/or
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