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USBL System Calibration
The purpose of this type of USBL System Calibration is to confirm that no biases are caused by the system's bearing information and that the speed of sound (scale factor) used in position calculations is correct. It is usually considered acceptable to use calibration results to remove any minor residual errors such as a bearing error of less than 1 or 2 degrees and speed of sound error within 1% or so. If large errors are found then the instillation of the USBL and its support equipment should be reviewed and necessary corrections made. The IPS System Calibration feature calculates and displays the overall azimuth (bearing) error in the system and gives the scaling factor to correct the raw slant range values. These results can be used to correct minor bearing errors or to determine if the USBL support equipment has been set up correctly. In addition to applying the calibration results to real time data to adjust minor discrepancies, the calibration results may also be saved for use at a later time or printed. The Calibration will work for both BATS, Trackpoint and LXT units and previously saved data may be loaded back into the software and used for calibration.
The image above displays the results of asystem calibration. The cyan dots in the view grid demonstrate how the data points used in the calibration would be plotted if the system calibration corrections were applied. The green data points represent the original data used for the calibration. Note the center of the cyan data points are grouped more closely to the mean position. In this case the beacon was stationary and the errors shown by the green dots are caused by incorrect equipment offsets. The IPS determined the installation biases (yaw, pitch and roll) of the equipment and converted the raw data to correct geodetic positions. Please see the IPS Help File USBL Calibration section for more information.ur own text and edit me. It's easy.
If the calibration was meaningful the Before and After frequency plots should show that the position of the beacon goes from broadly distributed positions to a very tight cluster as seen in the figures on the right. In the image on the left before the calibration the yellow points are scattered. In the image on the right the points come together and form a spike
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