Class AccumulatedMagneticFluxDensityTriadNoiseEstimator

java.lang.Object
com.irurueta.navigation.inertial.calibration.noise.AccumulatedTriadNoiseEstimator<com.irurueta.units.MagneticFluxDensityUnit,com.irurueta.units.MagneticFluxDensity,MagneticFluxDensityTriad,AccumulatedMagneticFluxDensityTriadNoiseEstimator,AccumulatedMagneticFluxDensityTriadNoiseEstimatorListener>
com.irurueta.navigation.inertial.calibration.noise.AccumulatedMagneticFluxDensityTriadNoiseEstimator

public class AccumulatedMagneticFluxDensityTriadNoiseEstimator extends AccumulatedTriadNoiseEstimator<com.irurueta.units.MagneticFluxDensityUnit,com.irurueta.units.MagneticFluxDensity,MagneticFluxDensityTriad,AccumulatedMagneticFluxDensityTriadNoiseEstimator,AccumulatedMagneticFluxDensityTriadNoiseEstimatorListener>
Estimates accumulated magnetometer noise variances and PSD's (Power Spectral Densities) along with their average values. This estimator must be used when the body where the magnetometer is attached remains static on the same position and orientation with zero velocity while capturing data. To compute PSD's, this estimator assumes that measurement samples are obtained at a constant provided rate equal to AccumulatedTriadNoiseEstimator.getTimeInterval() seconds. If not available, gyroscope sampling rate average can be estimated using TimeIntervalEstimator. This estimator does NOT require the knowledge of current location and body orientation. Because body location and orientation is not known, estimated average values cannot be used to determine biases. Only norm of noise estimations (variance or standard deviation) can be safely used. This implementation of noise estimator will use the following units: - Teslas (T) for magnetic flux density, average or standard deviation values. - squared Teslas (T^2) for magnetic flux density variances. - (T^2 * s) for magnetometer PSD (Power Spectral Density). - (T * s^0.5) for magnetometer root PSD (Power Spectral Density).