Seismic data is used to visualize the Earth's sub surface. This is achieved by measuring travel times of reflections from pressure waves propagating through the ground. Seismic data and interpretations of seismic data will therefore often have z values in travel time, not depth. In order to get a depth value for a travel time value, we need to do a depth conversion. A depth conversion combines the velocity of the pressure wave with the travel time to get a depth value.
Data sets may be depth converted in Geocap using the command "Velocity Model Depth Convert". This command uses a "Velocity Model" as input in order to determine the velocity of a the pressure wave.
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A velocity model is stored as an item in your Projectproject. It represents the seismic velocities in an area , and is used as input to the "Velocity Model Depth Convert" command.
To create a new velocity model
- Locate or create a folder of type Generic.
- Right-click a generic folder with the the folder and click Set Schema. Click Velocity models schemaSelect .
- Right click the folder and click Generate Velocity modelModel
- Set Adjust the parameters you want to use in your modelmodel parameters.
- Click Execute.
A new velocity model i will be created in the folder.
To view or edit an existing velocity model
- Right click the velocity model
- Select "View/Edit"
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- The model editor dialog will appear
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- .
- View or edit the model parameters.
Supported velocity models
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Geocap currently supports these types of velocity models:
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In the Layer Velocity model , you may use seismic horizons as interval velocity boundaries. The horizons may be interpreted lines from 2D seismic (IHorizon or PolyData) or grids (StructuredPoints). You may set the interval velocity of each interval using a table. In the table you also need to set the top horizon of each interval. In addition you need to set the water velocity as input.
When going from top to bottom , the layer velocity model will initially use the water velocity as interval velocity until it meets the top horizon. From the top horizon , it will use the top horizon velocity as interval velocity until it meets the next horizon, and so on. continuing this pairwise matching of successive horizons for the rest of the seismic data.
During depth conversion , the interval velocities are used to calculate an average velocity.
RMS
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Velocity (
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Stacking velocities)
The RMS velocitiy model uses RMS velocity data sets as input. It is possible to select a single data set in the project as input, but you may also select a folder containing multiple RMS velocity data sets as input. In some cases Stacking velocities may be used as RMS velocities.
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In order to generate an average velocity, the velocity model will run Dix formula on the RMS velocity to generate interval velocities. An average velocity is computed from the interval velocities.
Note that the Search search radius should be big large enough so that all points where you need a velocity will have RMS points within the search radius. However if the search radius is set too big, the velocity computation for a point will include too many RMS points, and the calculation may be slow. The recommended radius will depend on the density of the RMS velocity dataset.
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The depth conversion command has options to store the Average average velocity used to do the depth conversion of each point in the result. You may also choose to store the "Instantaneous Velocity". The "Instantaneous Velocity" is computed by looking at the change of average velocity from the velocity model around a point. For seismic lines the the " Instantaneous Velocity" is the interval velocity of a single sample in the seismic. Storing and visualizing these velocities will make you able to quality control the velocity model used for the depth conversion.
If you store velocities when depth converting seismic lines , the velocity values are stored as seismic attributes to the resulting seismic lines. You may visualize the velocities with the regular "Seismic Display" command. Note that storing velocities will make the depth conversion of seismic lines slower.
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