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Amplitude Correction by reference (etalon/standard/model) seismic
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Seismic data distortions happen during the seismic data acquisition. This is due to the source energy dissipation, source & receiver variations, geometrical spreading, near surface effects etc. Due to this, seismic amplitudes vary in degree as the shallow data may have higher amplitudes and the deeper events/data has less amplitude. The variation in amplitudes is quite contrast. Higher frequencies attenuate faster than the lower frequencies due to seismic resolution get impacted and the it is very difficult to interpret the data. To compensate the loss of energy, we often perform amplitude correction methods.
This module performs amplitude correction for input seismic data using another seismic data as etalon (reference/standard).Output seismic traces will have amplitudes similar to etalon. Input seismic data and etalon should have the same number of traces and samples. One input data with amplitude distortions and another seismic data (model/etalon/reference) with correct amplitudes are taken and do the correction by adjusting the user defined time window and trace parameters to minimize the mismatch between input and model gather. This module calculates the amplitude factors by comparing the input with model gather and these amplitude factors are applied on the input data to look similar to the model/reference/etalon gather.
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Notify - It will notify the issue if there are any bad values or NaN. This is halt the workflow execution.
Fix - It will fix the bad values and continue executing the workflow.
Continue - This option will continue the execution of the workflow however if there are any bad values or NaN, it won't fix it.
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There is no information available for this module so the user can ignore it.
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In this example workflow, we are testing Adaptive amplitude correction module on two stack sections. Stack 1 is having amplitude distortions and Stack 2 is amplitudes compensated. Stack 1 acts as Input gather and Stack 2 acts as Etalon/Reference/Model gather. We compute the amplitude factors with the help of Stack 2 and apply these amplitude factors to Stack to compensate the amplitude loss and make both the stacks similar.


Adjust the parameters and launch the Vista items. It displays input, output, input model, difference & amplitude factors.




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There are no action items available for this module so the user can ignore it.
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YouTube video lesson, click here to open [VIDEO IN PROCESS...]
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Yilmaz. O., 1987, Seismic data processing: Society of Exploration Geophysicist
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