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AP_NavEKF2_MagFusion.cpp
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AP_NavEKF2_MagFusion.cpp
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#include <AP_HAL/AP_HAL.h>
#if HAL_CPU_CLASS >= HAL_CPU_CLASS_150
#include "AP_NavEKF2.h"
#include "AP_NavEKF2_core.h"
#include <AP_AHRS/AP_AHRS.h>
#include <AP_Vehicle/AP_Vehicle.h>
#include <GCS_MAVLink/GCS.h>
#include <stdio.h>
extern const AP_HAL::HAL& hal;
/********************************************************
* RESET FUNCTIONS *
********************************************************/
// Control reset of yaw and magnetic field states
void NavEKF2_core::controlMagYawReset()
{
// Vehicles that can use a zero sideslip assumption (Planes) are a special case
// They can use the GPS velocity to recover from bad initial compass data
// This allows recovery for heading alignment errors due to compass faults
if (assume_zero_sideslip() && !finalInflightYawInit && inFlight ) {
gpsYawResetRequest = true;
return;
} else {
gpsYawResetRequest = false;
}
// Quaternion and delta rotation vector that are re-used for different calculations
Vector3f deltaRotVecTemp;
Quaternion deltaQuatTemp;
bool flightResetAllowed = false;
bool initialResetAllowed = false;
if (!finalInflightYawInit) {
// Use a quaternion division to calculate the delta quaternion between the rotation at the current and last time
deltaQuatTemp = stateStruct.quat / prevQuatMagReset;
prevQuatMagReset = stateStruct.quat;
// convert the quaternion to a rotation vector and find its length
deltaQuatTemp.to_axis_angle(deltaRotVecTemp);
// check if the spin rate is OK - high spin rates can cause angular alignment errors
bool angRateOK = deltaRotVecTemp.length() < 0.1745f;
initialResetAllowed = angRateOK;
flightResetAllowed = angRateOK && !onGround;
}
// Check if conditions for a interim or final yaw/mag reset are met
bool finalResetRequest = false;
bool interimResetRequest = false;
if (flightResetAllowed && !assume_zero_sideslip()) {
// check that we have reached a height where ground magnetic interference effects are insignificant
// and can perform a final reset of the yaw and field states
finalResetRequest = (stateStruct.position.z - posDownAtTakeoff) < -EKF2_MAG_FINAL_RESET_ALT;
// check for increasing height
bool hgtIncreasing = (posDownAtLastMagReset-stateStruct.position.z) > 0.5f;
float yawInnovIncrease = fabsf(innovYaw) - fabsf(yawInnovAtLastMagReset);
// check for increasing yaw innovations
bool yawInnovIncreasing = yawInnovIncrease > 0.25f;
// check that the yaw innovations haven't been caused by a large change in attitude
deltaQuatTemp = quatAtLastMagReset / stateStruct.quat;
deltaQuatTemp.to_axis_angle(deltaRotVecTemp);
bool largeAngleChange = deltaRotVecTemp.length() > yawInnovIncrease;
// if yaw innovations and height have increased and we haven't rotated much
// then we are climbing away from a ground based magnetic anomaly and need to reset
interimResetRequest = hgtIncreasing && yawInnovIncreasing && !largeAngleChange;
}
// an initial reset is required if we have not yet aligned the yaw angle
bool initialResetRequest = initialResetAllowed && !yawAlignComplete;
// a combined yaw angle and magnetic field reset can be initiated by:
magYawResetRequest = magYawResetRequest || // an external request
initialResetRequest || // an initial alignment performed by all vehicle types using magnetometer
interimResetRequest || // an interim alignment required to recover from ground based magnetic anomaly
finalResetRequest; // the final reset when we have acheived enough height to be in stable magnetic field environment
// Perform a reset of magnetic field states and reset yaw to corrected magnetic heading
if (magYawResetRequest || magStateResetRequest || extNavYawResetRequest) {
// if a yaw reset has been requested, apply the updated quaternion to the current state
if (extNavYawResetRequest) {
// get the euler angles from the current state estimate
Vector3f eulerAnglesOld;
stateStruct.quat.to_euler(eulerAnglesOld.x, eulerAnglesOld.y, eulerAnglesOld.z);
// previous value used to calculate a reset delta
Quaternion prevQuat = stateStruct.quat;
// Get the Euler angles from the external vision data
Vector3f eulerAnglesNew;
extNavDataDelayed.quat.to_euler(eulerAnglesNew.x, eulerAnglesNew.y, eulerAnglesNew.z);
// the new quaternion uses the old roll/pitch and new yaw angle
stateStruct.quat.from_euler(eulerAnglesOld.x, eulerAnglesOld.y, eulerAnglesNew.z);
// calculate the change in the quaternion state and apply it to the ouput history buffer
prevQuat = stateStruct.quat/prevQuat;
StoreQuatRotate(prevQuat);
// send initial alignment status to console
if (!yawAlignComplete) {
gcs().send_text(MAV_SEVERITY_INFO, "EKF2 IMU%u ext nav yaw alignment complete",(unsigned)imu_index);
}
// record the reset as complete and also record the in-flight reset as complete to stop further resets when hight is gained
// in-flight reset is unnecessary because we do not need to consider groudn based magnetic anomaly effects
yawAlignComplete = true;
finalInflightYawInit = true;
// clear the yaw reset request flag
extNavYawResetRequest = false;
} else if (magYawResetRequest || magStateResetRequest) {
// get the euler angles from the current state estimate
Vector3f eulerAngles;
stateStruct.quat.to_euler(eulerAngles.x, eulerAngles.y, eulerAngles.z);
// Use the Euler angles and magnetometer measurement to update the magnetic field states
// and get an updated quaternion
Quaternion newQuat = calcQuatAndFieldStates(eulerAngles.x, eulerAngles.y);
if (magYawResetRequest) {
// previous value used to calculate a reset delta
Quaternion prevQuat = stateStruct.quat;
// update the quaternion states using the new yaw angle
stateStruct.quat = newQuat;
// calculate the change in the quaternion state and apply it to the ouput history buffer
prevQuat = stateStruct.quat/prevQuat;
StoreQuatRotate(prevQuat);
// send initial alignment status to console
if (!yawAlignComplete) {
gcs().send_text(MAV_SEVERITY_INFO, "EKF2 IMU%u initial yaw alignment complete",(unsigned)imu_index);
}
// send in-flight yaw alignment status to console
if (finalResetRequest) {
gcs().send_text(MAV_SEVERITY_INFO, "EKF2 IMU%u in-flight yaw alignment complete",(unsigned)imu_index);
} else if (interimResetRequest) {
gcs().send_text(MAV_SEVERITY_WARNING, "EKF2 IMU%u ground mag anomaly, yaw re-aligned",(unsigned)imu_index);
}
// update the yaw reset completed status
recordYawReset();
// clear the yaw reset request flag
magYawResetRequest = false;
// clear the complete flags if an interim reset has been performed to allow subsequent
// and final reset to occur
if (interimResetRequest) {
finalInflightYawInit = false;
finalInflightMagInit = false;
}
}
}
}
}
// this function is used to do a forced re-alignment of the yaw angle to align with the horizontal velocity
// vector from GPS. It is used to align the yaw angle after launch or takeoff.
void NavEKF2_core::realignYawGPS()
{
if ((sq(gpsDataDelayed.vel.x) + sq(gpsDataDelayed.vel.y)) > 25.0f) {
// get quaternion from existing filter states and calculate roll, pitch and yaw angles
Vector3f eulerAngles;
stateStruct.quat.to_euler(eulerAngles.x, eulerAngles.y, eulerAngles.z);
// calculate course yaw angle
float velYaw = atan2f(stateStruct.velocity.y,stateStruct.velocity.x);
// calculate course yaw angle from GPS velocity
float gpsYaw = atan2f(gpsDataDelayed.vel.y,gpsDataDelayed.vel.x);
// Check the yaw angles for consistency
float yawErr = MAX(fabsf(wrap_PI(gpsYaw - velYaw)),fabsf(wrap_PI(gpsYaw - eulerAngles.z)));
// If the angles disagree by more than 45 degrees and GPS innovations are large or no previous yaw alignment, we declare the magnetic yaw as bad
badMagYaw = ((yawErr > 0.7854f) && (velTestRatio > 1.0f) && (PV_AidingMode == AID_ABSOLUTE)) || !yawAlignComplete;
// correct yaw angle using GPS ground course if compass yaw bad
if (badMagYaw) {
// calculate new filter quaternion states from Euler angles
stateStruct.quat.from_euler(eulerAngles.x, eulerAngles.y, gpsYaw);
// reset the velocity and position states as they will be inaccurate due to bad yaw
ResetVelocity();
ResetPosition();
// send yaw alignment information to console
gcs().send_text(MAV_SEVERITY_INFO, "EKF2 IMU%u yaw aligned to GPS velocity",(unsigned)imu_index);
// zero the attitude covariances becasue the corelations will now be invalid
zeroAttCovOnly();
// record the yaw reset event
recordYawReset();
// clear all pending yaw reset requests
gpsYawResetRequest = false;
magYawResetRequest = false;
if (use_compass()) {
// request a mag field reset which may enable us to use the magnetoemter if the previous fault was due to bad initialisation
magStateResetRequest = true;
// clear the all sensors failed status so that the magnetometers sensors get a second chance now that we are flying
allMagSensorsFailed = false;
}
}
}
}
/********************************************************
* FUSE MEASURED_DATA *
********************************************************/
// select fusion of magnetometer data
void NavEKF2_core::SelectMagFusion()
{
// start performance timer
hal.util->perf_begin(_perf_FuseMagnetometer);
// clear the flag that lets other processes know that the expensive magnetometer fusion operation has been perfomred on that time step
// used for load levelling
magFusePerformed = false;
// check for and read new magnetometer measurements
readMagData();
// If we are using the compass and the magnetometer has been unhealthy for too long we declare a timeout
if (magHealth) {
magTimeout = false;
lastHealthyMagTime_ms = imuSampleTime_ms;
} else if ((imuSampleTime_ms - lastHealthyMagTime_ms) > frontend->magFailTimeLimit_ms && use_compass()) {
magTimeout = true;
}
// check for availability of magnetometer data to fuse
magDataToFuse = storedMag.recall(magDataDelayed,imuDataDelayed.time_ms);
// Control reset of yaw and magnetic field states if we are using compass data
if (magDataToFuse && use_compass()) {
controlMagYawReset();
}
// determine if conditions are right to start a new fusion cycle
// wait until the EKF time horizon catches up with the measurement
bool dataReady = (magDataToFuse && statesInitialised && use_compass() && yawAlignComplete);
if (dataReady) {
// use the simple method of declination to maintain heading if we cannot use the magnetic field states
if(inhibitMagStates || magStateResetRequest || !magStateInitComplete) {
fuseEulerYaw();
// zero the test ratio output from the inactive 3-axis magnetometer fusion
magTestRatio.zero();
} else {
// if we are not doing aiding with earth relative observations (eg GPS) then the declination is
// maintained by fusing declination as a synthesised observation
if (PV_AidingMode != AID_ABSOLUTE) {
FuseDeclination(0.34f);
}
// fuse the three magnetometer componenents sequentially
for (mag_state.obsIndex = 0; mag_state.obsIndex <= 2; mag_state.obsIndex++) {
hal.util->perf_begin(_perf_test[0]);
FuseMagnetometer();
hal.util->perf_end(_perf_test[0]);
// don't continue fusion if unhealthy
if (!magHealth) {
break;
}
}
// zero the test ratio output from the inactive simple magnetometer yaw fusion
yawTestRatio = 0.0f;
}
}
// If we have no magnetometer and are on the ground, fuse in a synthetic heading measurement to prevent the
// filter covariances from becoming badly conditioned
if (!use_compass()) {
if (onGround && (imuSampleTime_ms - lastYawTime_ms > 1000)) {
fuseEulerYaw();
magTestRatio.zero();
yawTestRatio = 0.0f;
}
}
// If the final yaw reset has been performed and the state variances are sufficiently low
// record that the earth field has been learned.
if (!magFieldLearned && finalInflightMagInit) {
magFieldLearned = (P[16][16] < sq(0.01f)) && (P[17][17] < sq(0.01f)) && (P[18][18] < sq(0.01f));
}
// record the last learned field variances
if (magFieldLearned && !inhibitMagStates) {
earthMagFieldVar.x = P[16][16];
earthMagFieldVar.y = P[17][17];
earthMagFieldVar.z = P[18][18];
bodyMagFieldVar.x = P[19][19];
bodyMagFieldVar.y = P[20][20];
bodyMagFieldVar.z = P[21][21];
}
// stop performance timer
hal.util->perf_end(_perf_FuseMagnetometer);
}
/*
* Fuse magnetometer measurements using explicit algebraic equations generated with Matlab symbolic toolbox.
* The script file used to generate these and other equations in this filter can be found here:
* https://github.com/priseborough/InertialNav/blob/master/derivations/RotationVectorAttitudeParameterisation/GenerateNavFilterEquations.m
*/
void NavEKF2_core::FuseMagnetometer()
{
hal.util->perf_begin(_perf_test[1]);
// declarations
ftype &q0 = mag_state.q0;
ftype &q1 = mag_state.q1;
ftype &q2 = mag_state.q2;
ftype &q3 = mag_state.q3;
ftype &magN = mag_state.magN;
ftype &magE = mag_state.magE;
ftype &magD = mag_state.magD;
ftype &magXbias = mag_state.magXbias;
ftype &magYbias = mag_state.magYbias;
ftype &magZbias = mag_state.magZbias;
uint8_t &obsIndex = mag_state.obsIndex;
Matrix3f &DCM = mag_state.DCM;
Vector3f &MagPred = mag_state.MagPred;
ftype &R_MAG = mag_state.R_MAG;
ftype *SH_MAG = &mag_state.SH_MAG[0];
Vector24 H_MAG;
Vector6 SK_MX;
Vector6 SK_MY;
Vector6 SK_MZ;
hal.util->perf_end(_perf_test[1]);
// perform sequential fusion of magnetometer measurements.
// this assumes that the errors in the different components are
// uncorrelated which is not true, however in the absence of covariance
// data fit is the only assumption we can make
// so we might as well take advantage of the computational efficiencies
// associated with sequential fusion
// calculate observation jacobians and Kalman gains
if (obsIndex == 0)
{
hal.util->perf_begin(_perf_test[2]);
// copy required states to local variable names
q0 = stateStruct.quat[0];
q1 = stateStruct.quat[1];
q2 = stateStruct.quat[2];
q3 = stateStruct.quat[3];
magN = stateStruct.earth_magfield[0];
magE = stateStruct.earth_magfield[1];
magD = stateStruct.earth_magfield[2];
magXbias = stateStruct.body_magfield[0];
magYbias = stateStruct.body_magfield[1];
magZbias = stateStruct.body_magfield[2];
// rotate predicted earth components into body axes and calculate
// predicted measurements
DCM[0][0] = q0*q0 + q1*q1 - q2*q2 - q3*q3;
DCM[0][1] = 2.0f*(q1*q2 + q0*q3);
DCM[0][2] = 2.0f*(q1*q3-q0*q2);
DCM[1][0] = 2.0f*(q1*q2 - q0*q3);
DCM[1][1] = q0*q0 - q1*q1 + q2*q2 - q3*q3;
DCM[1][2] = 2.0f*(q2*q3 + q0*q1);
DCM[2][0] = 2.0f*(q1*q3 + q0*q2);
DCM[2][1] = 2.0f*(q2*q3 - q0*q1);
DCM[2][2] = q0*q0 - q1*q1 - q2*q2 + q3*q3;
MagPred[0] = DCM[0][0]*magN + DCM[0][1]*magE + DCM[0][2]*magD + magXbias;
MagPred[1] = DCM[1][0]*magN + DCM[1][1]*magE + DCM[1][2]*magD + magYbias;
MagPred[2] = DCM[2][0]*magN + DCM[2][1]*magE + DCM[2][2]*magD + magZbias;
// calculate the measurement innovation for each axis
for (uint8_t i = 0; i<=2; i++) {
innovMag[i] = MagPred[i] - magDataDelayed.mag[i];
}
// scale magnetometer observation error with total angular rate to allow for timing errors
R_MAG = sq(constrain_float(frontend->_magNoise, 0.01f, 0.5f)) + sq(frontend->magVarRateScale*delAngCorrected.length() / imuDataDelayed.delAngDT);
// calculate common expressions used to calculate observation jacobians an innovation variance for each component
SH_MAG[0] = sq(q0) - sq(q1) + sq(q2) - sq(q3);
SH_MAG[1] = sq(q0) + sq(q1) - sq(q2) - sq(q3);
SH_MAG[2] = sq(q0) - sq(q1) - sq(q2) + sq(q3);
SH_MAG[3] = 2.0f*q0*q1 + 2.0f*q2*q3;
SH_MAG[4] = 2.0f*q0*q3 + 2.0f*q1*q2;
SH_MAG[5] = 2.0f*q0*q2 + 2.0f*q1*q3;
SH_MAG[6] = magE*(2.0f*q0*q1 - 2.0f*q2*q3);
SH_MAG[7] = 2.0f*q1*q3 - 2.0f*q0*q2;
SH_MAG[8] = 2.0f*q0*q3;
// Calculate the innovation variance for each axis
// X axis
varInnovMag[0] = (P[19][19] + R_MAG - P[1][19]*(magD*SH_MAG[2] - SH_MAG[6] + magN*SH_MAG[5]) + P[16][19]*SH_MAG[1] + P[17][19]*SH_MAG[4] + P[18][19]*SH_MAG[7] + P[2][19]*(magE*SH_MAG[0] + magD*SH_MAG[3] - magN*(SH_MAG[8] - 2.0f*q1*q2)) - (magD*SH_MAG[2] - SH_MAG[6] + magN*SH_MAG[5])*(P[19][1] - P[1][1]*(magD*SH_MAG[2] - SH_MAG[6] + magN*SH_MAG[5]) + P[16][1]*SH_MAG[1] + P[17][1]*SH_MAG[4] + P[18][1]*SH_MAG[7] + P[2][1]*(magE*SH_MAG[0] + magD*SH_MAG[3] - magN*(SH_MAG[8] - 2.0f*q1*q2))) + SH_MAG[1]*(P[19][16] - P[1][16]*(magD*SH_MAG[2] - SH_MAG[6] + magN*SH_MAG[5]) + P[16][16]*SH_MAG[1] + P[17][16]*SH_MAG[4] + P[18][16]*SH_MAG[7] + P[2][16]*(magE*SH_MAG[0] + magD*SH_MAG[3] - magN*(SH_MAG[8] - 2.0f*q1*q2))) + SH_MAG[4]*(P[19][17] - P[1][17]*(magD*SH_MAG[2] - SH_MAG[6] + magN*SH_MAG[5]) + P[16][17]*SH_MAG[1] + P[17][17]*SH_MAG[4] + P[18][17]*SH_MAG[7] + P[2][17]*(magE*SH_MAG[0] + magD*SH_MAG[3] - magN*(SH_MAG[8] - 2.0f*q1*q2))) + SH_MAG[7]*(P[19][18] - P[1][18]*(magD*SH_MAG[2] - SH_MAG[6] + magN*SH_MAG[5]) + P[16][18]*SH_MAG[1] + P[17][18]*SH_MAG[4] + P[18][18]*SH_MAG[7] + P[2][18]*(magE*SH_MAG[0] + magD*SH_MAG[3] - magN*(SH_MAG[8] - 2.0f*q1*q2))) + (magE*SH_MAG[0] + magD*SH_MAG[3] - magN*(SH_MAG[8] - 2.0f*q1*q2))*(P[19][2] - P[1][2]*(magD*SH_MAG[2] - SH_MAG[6] + magN*SH_MAG[5]) + P[16][2]*SH_MAG[1] + P[17][2]*SH_MAG[4] + P[18][2]*SH_MAG[7] + P[2][2]*(magE*SH_MAG[0] + magD*SH_MAG[3] - magN*(SH_MAG[8] - 2.0f*q1*q2))));
if (varInnovMag[0] >= R_MAG) {
faultStatus.bad_xmag = false;
} else {
// the calculation is badly conditioned, so we cannot perform fusion on this step
// we reset the covariance matrix and try again next measurement
CovarianceInit();
obsIndex = 1;
faultStatus.bad_xmag = true;
hal.util->perf_end(_perf_test[2]);
return;
}
// Y axis
varInnovMag[1] = (P[20][20] + R_MAG + P[0][20]*(magD*SH_MAG[2] - SH_MAG[6] + magN*SH_MAG[5]) + P[17][20]*SH_MAG[0] + P[18][20]*SH_MAG[3] - (SH_MAG[8] - 2.0f*q1*q2)*(P[20][16] + P[0][16]*(magD*SH_MAG[2] - SH_MAG[6] + magN*SH_MAG[5]) + P[17][16]*SH_MAG[0] + P[18][16]*SH_MAG[3] - P[2][16]*(magE*SH_MAG[4] + magD*SH_MAG[7] + magN*SH_MAG[1]) - P[16][16]*(SH_MAG[8] - 2.0f*q1*q2)) - P[2][20]*(magE*SH_MAG[4] + magD*SH_MAG[7] + magN*SH_MAG[1]) + (magD*SH_MAG[2] - SH_MAG[6] + magN*SH_MAG[5])*(P[20][0] + P[0][0]*(magD*SH_MAG[2] - SH_MAG[6] + magN*SH_MAG[5]) + P[17][0]*SH_MAG[0] + P[18][0]*SH_MAG[3] - P[2][0]*(magE*SH_MAG[4] + magD*SH_MAG[7] + magN*SH_MAG[1]) - P[16][0]*(SH_MAG[8] - 2.0f*q1*q2)) + SH_MAG[0]*(P[20][17] + P[0][17]*(magD*SH_MAG[2] - SH_MAG[6] + magN*SH_MAG[5]) + P[17][17]*SH_MAG[0] + P[18][17]*SH_MAG[3] - P[2][17]*(magE*SH_MAG[4] + magD*SH_MAG[7] + magN*SH_MAG[1]) - P[16][17]*(SH_MAG[8] - 2.0f*q1*q2)) + SH_MAG[3]*(P[20][18] + P[0][18]*(magD*SH_MAG[2] - SH_MAG[6] + magN*SH_MAG[5]) + P[17][18]*SH_MAG[0] + P[18][18]*SH_MAG[3] - P[2][18]*(magE*SH_MAG[4] + magD*SH_MAG[7] + magN*SH_MAG[1]) - P[16][18]*(SH_MAG[8] - 2.0f*q1*q2)) - P[16][20]*(SH_MAG[8] - 2.0f*q1*q2) - (magE*SH_MAG[4] + magD*SH_MAG[7] + magN*SH_MAG[1])*(P[20][2] + P[0][2]*(magD*SH_MAG[2] - SH_MAG[6] + magN*SH_MAG[5]) + P[17][2]*SH_MAG[0] + P[18][2]*SH_MAG[3] - P[2][2]*(magE*SH_MAG[4] + magD*SH_MAG[7] + magN*SH_MAG[1]) - P[16][2]*(SH_MAG[8] - 2.0f*q1*q2)));
if (varInnovMag[1] >= R_MAG) {
faultStatus.bad_ymag = false;
} else {
// the calculation is badly conditioned, so we cannot perform fusion on this step
// we reset the covariance matrix and try again next measurement
CovarianceInit();
obsIndex = 2;
faultStatus.bad_ymag = true;
hal.util->perf_end(_perf_test[2]);
return;
}
// Z axis
varInnovMag[2] = (P[21][21] + R_MAG + P[16][21]*SH_MAG[5] + P[18][21]*SH_MAG[2] - (2.0f*q0*q1 - 2.0f*q2*q3)*(P[21][17] + P[16][17]*SH_MAG[5] + P[18][17]*SH_MAG[2] - P[0][17]*(magE*SH_MAG[0] + magD*SH_MAG[3] - magN*(SH_MAG[8] - 2.0f*q1*q2)) + P[1][17]*(magE*SH_MAG[4] + magD*SH_MAG[7] + magN*SH_MAG[1]) - P[17][17]*(2.0f*q0*q1 - 2.0f*q2*q3)) - P[0][21]*(magE*SH_MAG[0] + magD*SH_MAG[3] - magN*(SH_MAG[8] - 2.0f*q1*q2)) + P[1][21]*(magE*SH_MAG[4] + magD*SH_MAG[7] + magN*SH_MAG[1]) + SH_MAG[5]*(P[21][16] + P[16][16]*SH_MAG[5] + P[18][16]*SH_MAG[2] - P[0][16]*(magE*SH_MAG[0] + magD*SH_MAG[3] - magN*(SH_MAG[8] - 2.0f*q1*q2)) + P[1][16]*(magE*SH_MAG[4] + magD*SH_MAG[7] + magN*SH_MAG[1]) - P[17][16]*(2.0f*q0*q1 - 2.0f*q2*q3)) + SH_MAG[2]*(P[21][18] + P[16][18]*SH_MAG[5] + P[18][18]*SH_MAG[2] - P[0][18]*(magE*SH_MAG[0] + magD*SH_MAG[3] - magN*(SH_MAG[8] - 2.0f*q1*q2)) + P[1][18]*(magE*SH_MAG[4] + magD*SH_MAG[7] + magN*SH_MAG[1]) - P[17][18]*(2.0f*q0*q1 - 2.0f*q2*q3)) - (magE*SH_MAG[0] + magD*SH_MAG[3] - magN*(SH_MAG[8] - 2.0f*q1*q2))*(P[21][0] + P[16][0]*SH_MAG[5] + P[18][0]*SH_MAG[2] - P[0][0]*(magE*SH_MAG[0] + magD*SH_MAG[3] - magN*(SH_MAG[8] - 2.0f*q1*q2)) + P[1][0]*(magE*SH_MAG[4] + magD*SH_MAG[7] + magN*SH_MAG[1]) - P[17][0]*(2.0f*q0*q1 - 2.0f*q2*q3)) - P[17][21]*(2.0f*q0*q1 - 2.0f*q2*q3) + (magE*SH_MAG[4] + magD*SH_MAG[7] + magN*SH_MAG[1])*(P[21][1] + P[16][1]*SH_MAG[5] + P[18][1]*SH_MAG[2] - P[0][1]*(magE*SH_MAG[0] + magD*SH_MAG[3] - magN*(SH_MAG[8] - 2.0f*q1*q2)) + P[1][1]*(magE*SH_MAG[4] + magD*SH_MAG[7] + magN*SH_MAG[1]) - P[17][1]*(2.0f*q0*q1 - 2.0f*q2*q3)));
if (varInnovMag[2] >= R_MAG) {
faultStatus.bad_zmag = false;
} else {
// the calculation is badly conditioned, so we cannot perform fusion on this step
// we reset the covariance matrix and try again next measurement
CovarianceInit();
obsIndex = 3;
faultStatus.bad_zmag = true;
hal.util->perf_end(_perf_test[2]);
return;
}
// calculate the innovation test ratios
for (uint8_t i = 0; i<=2; i++) {
magTestRatio[i] = sq(innovMag[i]) / (sq(MAX(0.01f * (float)frontend->_magInnovGate, 1.0f)) * varInnovMag[i]);
}
// check the last values from all components and set magnetometer health accordingly
magHealth = (magTestRatio[0] < 1.0f && magTestRatio[1] < 1.0f && magTestRatio[2] < 1.0f);
// if the magnetometer is unhealthy, do not proceed further
if (!magHealth) {
hal.util->perf_end(_perf_test[2]);
return;
}
for (uint8_t i = 0; i<=stateIndexLim; i++) H_MAG[i] = 0.0f;
H_MAG[1] = SH_MAG[6] - magD*SH_MAG[2] - magN*SH_MAG[5];
H_MAG[2] = magE*SH_MAG[0] + magD*SH_MAG[3] - magN*(SH_MAG[8] - 2.0f*q1*q2);
H_MAG[16] = SH_MAG[1];
H_MAG[17] = SH_MAG[4];
H_MAG[18] = SH_MAG[7];
H_MAG[19] = 1.0f;
// calculate Kalman gain
SK_MX[0] = 1.0f / varInnovMag[0];
SK_MX[1] = magE*SH_MAG[0] + magD*SH_MAG[3] - magN*(SH_MAG[8] - 2.0f*q1*q2);
SK_MX[2] = magD*SH_MAG[2] - SH_MAG[6] + magN*SH_MAG[5];
SK_MX[3] = SH_MAG[7];
Kfusion[0] = SK_MX[0]*(P[0][19] + P[0][16]*SH_MAG[1] + P[0][17]*SH_MAG[4] - P[0][1]*SK_MX[2] + P[0][2]*SK_MX[1] + P[0][18]*SK_MX[3]);
Kfusion[1] = SK_MX[0]*(P[1][19] + P[1][16]*SH_MAG[1] + P[1][17]*SH_MAG[4] - P[1][1]*SK_MX[2] + P[1][2]*SK_MX[1] + P[1][18]*SK_MX[3]);
Kfusion[2] = SK_MX[0]*(P[2][19] + P[2][16]*SH_MAG[1] + P[2][17]*SH_MAG[4] - P[2][1]*SK_MX[2] + P[2][2]*SK_MX[1] + P[2][18]*SK_MX[3]);
Kfusion[3] = SK_MX[0]*(P[3][19] + P[3][16]*SH_MAG[1] + P[3][17]*SH_MAG[4] - P[3][1]*SK_MX[2] + P[3][2]*SK_MX[1] + P[3][18]*SK_MX[3]);
Kfusion[4] = SK_MX[0]*(P[4][19] + P[4][16]*SH_MAG[1] + P[4][17]*SH_MAG[4] - P[4][1]*SK_MX[2] + P[4][2]*SK_MX[1] + P[4][18]*SK_MX[3]);
Kfusion[5] = SK_MX[0]*(P[5][19] + P[5][16]*SH_MAG[1] + P[5][17]*SH_MAG[4] - P[5][1]*SK_MX[2] + P[5][2]*SK_MX[1] + P[5][18]*SK_MX[3]);
Kfusion[6] = SK_MX[0]*(P[6][19] + P[6][16]*SH_MAG[1] + P[6][17]*SH_MAG[4] - P[6][1]*SK_MX[2] + P[6][2]*SK_MX[1] + P[6][18]*SK_MX[3]);
Kfusion[7] = SK_MX[0]*(P[7][19] + P[7][16]*SH_MAG[1] + P[7][17]*SH_MAG[4] - P[7][1]*SK_MX[2] + P[7][2]*SK_MX[1] + P[7][18]*SK_MX[3]);
Kfusion[8] = SK_MX[0]*(P[8][19] + P[8][16]*SH_MAG[1] + P[8][17]*SH_MAG[4] - P[8][1]*SK_MX[2] + P[8][2]*SK_MX[1] + P[8][18]*SK_MX[3]);
Kfusion[9] = SK_MX[0]*(P[9][19] + P[9][16]*SH_MAG[1] + P[9][17]*SH_MAG[4] - P[9][1]*SK_MX[2] + P[9][2]*SK_MX[1] + P[9][18]*SK_MX[3]);
Kfusion[10] = SK_MX[0]*(P[10][19] + P[10][16]*SH_MAG[1] + P[10][17]*SH_MAG[4] - P[10][1]*SK_MX[2] + P[10][2]*SK_MX[1] + P[10][18]*SK_MX[3]);
Kfusion[11] = SK_MX[0]*(P[11][19] + P[11][16]*SH_MAG[1] + P[11][17]*SH_MAG[4] - P[11][1]*SK_MX[2] + P[11][2]*SK_MX[1] + P[11][18]*SK_MX[3]);
Kfusion[12] = SK_MX[0]*(P[12][19] + P[12][16]*SH_MAG[1] + P[12][17]*SH_MAG[4] - P[12][1]*SK_MX[2] + P[12][2]*SK_MX[1] + P[12][18]*SK_MX[3]);
Kfusion[13] = SK_MX[0]*(P[13][19] + P[13][16]*SH_MAG[1] + P[13][17]*SH_MAG[4] - P[13][1]*SK_MX[2] + P[13][2]*SK_MX[1] + P[13][18]*SK_MX[3]);
Kfusion[14] = SK_MX[0]*(P[14][19] + P[14][16]*SH_MAG[1] + P[14][17]*SH_MAG[4] - P[14][1]*SK_MX[2] + P[14][2]*SK_MX[1] + P[14][18]*SK_MX[3]);
Kfusion[15] = SK_MX[0]*(P[15][19] + P[15][16]*SH_MAG[1] + P[15][17]*SH_MAG[4] - P[15][1]*SK_MX[2] + P[15][2]*SK_MX[1] + P[15][18]*SK_MX[3]);
// end perf block
// zero Kalman gains to inhibit wind state estimation
if (!inhibitWindStates) {
Kfusion[22] = SK_MX[0]*(P[22][19] + P[22][16]*SH_MAG[1] + P[22][17]*SH_MAG[4] - P[22][1]*SK_MX[2] + P[22][2]*SK_MX[1] + P[22][18]*SK_MX[3]);
Kfusion[23] = SK_MX[0]*(P[23][19] + P[23][16]*SH_MAG[1] + P[23][17]*SH_MAG[4] - P[23][1]*SK_MX[2] + P[23][2]*SK_MX[1] + P[23][18]*SK_MX[3]);
} else {
Kfusion[22] = 0.0f;
Kfusion[23] = 0.0f;
}
// zero Kalman gains to inhibit magnetic field state estimation
if (!inhibitMagStates) {
Kfusion[16] = SK_MX[0]*(P[16][19] + P[16][16]*SH_MAG[1] + P[16][17]*SH_MAG[4] - P[16][1]*SK_MX[2] + P[16][2]*SK_MX[1] + P[16][18]*SK_MX[3]);
Kfusion[17] = SK_MX[0]*(P[17][19] + P[17][16]*SH_MAG[1] + P[17][17]*SH_MAG[4] - P[17][1]*SK_MX[2] + P[17][2]*SK_MX[1] + P[17][18]*SK_MX[3]);
Kfusion[18] = SK_MX[0]*(P[18][19] + P[18][16]*SH_MAG[1] + P[18][17]*SH_MAG[4] - P[18][1]*SK_MX[2] + P[18][2]*SK_MX[1] + P[18][18]*SK_MX[3]);
Kfusion[19] = SK_MX[0]*(P[19][19] + P[19][16]*SH_MAG[1] + P[19][17]*SH_MAG[4] - P[19][1]*SK_MX[2] + P[19][2]*SK_MX[1] + P[19][18]*SK_MX[3]);
Kfusion[20] = SK_MX[0]*(P[20][19] + P[20][16]*SH_MAG[1] + P[20][17]*SH_MAG[4] - P[20][1]*SK_MX[2] + P[20][2]*SK_MX[1] + P[20][18]*SK_MX[3]);
Kfusion[21] = SK_MX[0]*(P[21][19] + P[21][16]*SH_MAG[1] + P[21][17]*SH_MAG[4] - P[21][1]*SK_MX[2] + P[21][2]*SK_MX[1] + P[21][18]*SK_MX[3]);
} else {
for (uint8_t i=16; i<=21; i++) {
Kfusion[i] = 0.0f;
}
}
// reset the observation index to 0 (we start by fusing the X measurement)
obsIndex = 0;
// set flags to indicate to other processes that fusion has been performed and is required on the next frame
// this can be used by other fusion processes to avoid fusing on the same frame as this expensive step
magFusePerformed = true;
magFuseRequired = true;
hal.util->perf_end(_perf_test[2]);
}
else if (obsIndex == 1) // we are now fusing the Y measurement
{
hal.util->perf_begin(_perf_test[3]);
// calculate observation jacobians
for (uint8_t i = 0; i<=stateIndexLim; i++) H_MAG[i] = 0.0f;
H_MAG[0] = magD*SH_MAG[2] - SH_MAG[6] + magN*SH_MAG[5];
H_MAG[2] = - magE*SH_MAG[4] - magD*SH_MAG[7] - magN*SH_MAG[1];
H_MAG[16] = 2.0f*q1*q2 - SH_MAG[8];
H_MAG[17] = SH_MAG[0];
H_MAG[18] = SH_MAG[3];
H_MAG[20] = 1.0f;
// calculate Kalman gain
SK_MY[0] = 1.0f / varInnovMag[1];
SK_MY[1] = magE*SH_MAG[4] + magD*SH_MAG[7] + magN*SH_MAG[1];
SK_MY[2] = magD*SH_MAG[2] - SH_MAG[6] + magN*SH_MAG[5];
SK_MY[3] = SH_MAG[8] - 2.0f*q1*q2;
Kfusion[0] = SK_MY[0]*(P[0][20] + P[0][17]*SH_MAG[0] + P[0][18]*SH_MAG[3] + P[0][0]*SK_MY[2] - P[0][2]*SK_MY[1] - P[0][16]*SK_MY[3]);
Kfusion[1] = SK_MY[0]*(P[1][20] + P[1][17]*SH_MAG[0] + P[1][18]*SH_MAG[3] + P[1][0]*SK_MY[2] - P[1][2]*SK_MY[1] - P[1][16]*SK_MY[3]);
Kfusion[2] = SK_MY[0]*(P[2][20] + P[2][17]*SH_MAG[0] + P[2][18]*SH_MAG[3] + P[2][0]*SK_MY[2] - P[2][2]*SK_MY[1] - P[2][16]*SK_MY[3]);
Kfusion[3] = SK_MY[0]*(P[3][20] + P[3][17]*SH_MAG[0] + P[3][18]*SH_MAG[3] + P[3][0]*SK_MY[2] - P[3][2]*SK_MY[1] - P[3][16]*SK_MY[3]);
Kfusion[4] = SK_MY[0]*(P[4][20] + P[4][17]*SH_MAG[0] + P[4][18]*SH_MAG[3] + P[4][0]*SK_MY[2] - P[4][2]*SK_MY[1] - P[4][16]*SK_MY[3]);
Kfusion[5] = SK_MY[0]*(P[5][20] + P[5][17]*SH_MAG[0] + P[5][18]*SH_MAG[3] + P[5][0]*SK_MY[2] - P[5][2]*SK_MY[1] - P[5][16]*SK_MY[3]);
Kfusion[6] = SK_MY[0]*(P[6][20] + P[6][17]*SH_MAG[0] + P[6][18]*SH_MAG[3] + P[6][0]*SK_MY[2] - P[6][2]*SK_MY[1] - P[6][16]*SK_MY[3]);
Kfusion[7] = SK_MY[0]*(P[7][20] + P[7][17]*SH_MAG[0] + P[7][18]*SH_MAG[3] + P[7][0]*SK_MY[2] - P[7][2]*SK_MY[1] - P[7][16]*SK_MY[3]);
Kfusion[8] = SK_MY[0]*(P[8][20] + P[8][17]*SH_MAG[0] + P[8][18]*SH_MAG[3] + P[8][0]*SK_MY[2] - P[8][2]*SK_MY[1] - P[8][16]*SK_MY[3]);
Kfusion[9] = SK_MY[0]*(P[9][20] + P[9][17]*SH_MAG[0] + P[9][18]*SH_MAG[3] + P[9][0]*SK_MY[2] - P[9][2]*SK_MY[1] - P[9][16]*SK_MY[3]);
Kfusion[10] = SK_MY[0]*(P[10][20] + P[10][17]*SH_MAG[0] + P[10][18]*SH_MAG[3] + P[10][0]*SK_MY[2] - P[10][2]*SK_MY[1] - P[10][16]*SK_MY[3]);
Kfusion[11] = SK_MY[0]*(P[11][20] + P[11][17]*SH_MAG[0] + P[11][18]*SH_MAG[3] + P[11][0]*SK_MY[2] - P[11][2]*SK_MY[1] - P[11][16]*SK_MY[3]);
Kfusion[12] = SK_MY[0]*(P[12][20] + P[12][17]*SH_MAG[0] + P[12][18]*SH_MAG[3] + P[12][0]*SK_MY[2] - P[12][2]*SK_MY[1] - P[12][16]*SK_MY[3]);
Kfusion[13] = SK_MY[0]*(P[13][20] + P[13][17]*SH_MAG[0] + P[13][18]*SH_MAG[3] + P[13][0]*SK_MY[2] - P[13][2]*SK_MY[1] - P[13][16]*SK_MY[3]);
Kfusion[14] = SK_MY[0]*(P[14][20] + P[14][17]*SH_MAG[0] + P[14][18]*SH_MAG[3] + P[14][0]*SK_MY[2] - P[14][2]*SK_MY[1] - P[14][16]*SK_MY[3]);
Kfusion[15] = SK_MY[0]*(P[15][20] + P[15][17]*SH_MAG[0] + P[15][18]*SH_MAG[3] + P[15][0]*SK_MY[2] - P[15][2]*SK_MY[1] - P[15][16]*SK_MY[3]);
// zero Kalman gains to inhibit wind state estimation
if (!inhibitWindStates) {
Kfusion[22] = SK_MY[0]*(P[22][20] + P[22][17]*SH_MAG[0] + P[22][18]*SH_MAG[3] + P[22][0]*SK_MY[2] - P[22][2]*SK_MY[1] - P[22][16]*SK_MY[3]);
Kfusion[23] = SK_MY[0]*(P[23][20] + P[23][17]*SH_MAG[0] + P[23][18]*SH_MAG[3] + P[23][0]*SK_MY[2] - P[23][2]*SK_MY[1] - P[23][16]*SK_MY[3]);
} else {
Kfusion[22] = 0.0f;
Kfusion[23] = 0.0f;
}
// zero Kalman gains to inhibit magnetic field state estimation
if (!inhibitMagStates) {
Kfusion[16] = SK_MY[0]*(P[16][20] + P[16][17]*SH_MAG[0] + P[16][18]*SH_MAG[3] + P[16][0]*SK_MY[2] - P[16][2]*SK_MY[1] - P[16][16]*SK_MY[3]);
Kfusion[17] = SK_MY[0]*(P[17][20] + P[17][17]*SH_MAG[0] + P[17][18]*SH_MAG[3] + P[17][0]*SK_MY[2] - P[17][2]*SK_MY[1] - P[17][16]*SK_MY[3]);
Kfusion[18] = SK_MY[0]*(P[18][20] + P[18][17]*SH_MAG[0] + P[18][18]*SH_MAG[3] + P[18][0]*SK_MY[2] - P[18][2]*SK_MY[1] - P[18][16]*SK_MY[3]);
Kfusion[19] = SK_MY[0]*(P[19][20] + P[19][17]*SH_MAG[0] + P[19][18]*SH_MAG[3] + P[19][0]*SK_MY[2] - P[19][2]*SK_MY[1] - P[19][16]*SK_MY[3]);
Kfusion[20] = SK_MY[0]*(P[20][20] + P[20][17]*SH_MAG[0] + P[20][18]*SH_MAG[3] + P[20][0]*SK_MY[2] - P[20][2]*SK_MY[1] - P[20][16]*SK_MY[3]);
Kfusion[21] = SK_MY[0]*(P[21][20] + P[21][17]*SH_MAG[0] + P[21][18]*SH_MAG[3] + P[21][0]*SK_MY[2] - P[21][2]*SK_MY[1] - P[21][16]*SK_MY[3]);
} else {
for (uint8_t i=16; i<=21; i++) {
Kfusion[i] = 0.0f;
}
}
// set flags to indicate to other processes that fusion has been performede and is required on the next frame
// this can be used by other fusion processes to avoid fusing on the same frame as this expensive step
magFusePerformed = true;
magFuseRequired = true;
hal.util->perf_end(_perf_test[3]);
}
else if (obsIndex == 2) // we are now fusing the Z measurement
{
hal.util->perf_begin(_perf_test[4]);
// calculate observation jacobians
for (uint8_t i = 0; i<=stateIndexLim; i++) H_MAG[i] = 0.0f;
H_MAG[0] = magN*(SH_MAG[8] - 2.0f*q1*q2) - magD*SH_MAG[3] - magE*SH_MAG[0];
H_MAG[1] = magE*SH_MAG[4] + magD*SH_MAG[7] + magN*SH_MAG[1];
H_MAG[16] = SH_MAG[5];
H_MAG[17] = 2.0f*q2*q3 - 2.0f*q0*q1;
H_MAG[18] = SH_MAG[2];
H_MAG[21] = 1.0f;
// calculate Kalman gain
SK_MZ[0] = 1.0f / varInnovMag[2];
SK_MZ[1] = magE*SH_MAG[0] + magD*SH_MAG[3] - magN*(SH_MAG[8] - 2.0f*q1*q2);
SK_MZ[2] = magE*SH_MAG[4] + magD*SH_MAG[7] + magN*SH_MAG[1];
SK_MZ[3] = 2.0f*q0*q1 - 2.0f*q2*q3;
Kfusion[0] = SK_MZ[0]*(P[0][21] + P[0][18]*SH_MAG[2] + P[0][16]*SH_MAG[5] - P[0][0]*SK_MZ[1] + P[0][1]*SK_MZ[2] - P[0][17]*SK_MZ[3]);
Kfusion[1] = SK_MZ[0]*(P[1][21] + P[1][18]*SH_MAG[2] + P[1][16]*SH_MAG[5] - P[1][0]*SK_MZ[1] + P[1][1]*SK_MZ[2] - P[1][17]*SK_MZ[3]);
Kfusion[2] = SK_MZ[0]*(P[2][21] + P[2][18]*SH_MAG[2] + P[2][16]*SH_MAG[5] - P[2][0]*SK_MZ[1] + P[2][1]*SK_MZ[2] - P[2][17]*SK_MZ[3]);
Kfusion[3] = SK_MZ[0]*(P[3][21] + P[3][18]*SH_MAG[2] + P[3][16]*SH_MAG[5] - P[3][0]*SK_MZ[1] + P[3][1]*SK_MZ[2] - P[3][17]*SK_MZ[3]);
Kfusion[4] = SK_MZ[0]*(P[4][21] + P[4][18]*SH_MAG[2] + P[4][16]*SH_MAG[5] - P[4][0]*SK_MZ[1] + P[4][1]*SK_MZ[2] - P[4][17]*SK_MZ[3]);
Kfusion[5] = SK_MZ[0]*(P[5][21] + P[5][18]*SH_MAG[2] + P[5][16]*SH_MAG[5] - P[5][0]*SK_MZ[1] + P[5][1]*SK_MZ[2] - P[5][17]*SK_MZ[3]);
Kfusion[6] = SK_MZ[0]*(P[6][21] + P[6][18]*SH_MAG[2] + P[6][16]*SH_MAG[5] - P[6][0]*SK_MZ[1] + P[6][1]*SK_MZ[2] - P[6][17]*SK_MZ[3]);
Kfusion[7] = SK_MZ[0]*(P[7][21] + P[7][18]*SH_MAG[2] + P[7][16]*SH_MAG[5] - P[7][0]*SK_MZ[1] + P[7][1]*SK_MZ[2] - P[7][17]*SK_MZ[3]);
Kfusion[8] = SK_MZ[0]*(P[8][21] + P[8][18]*SH_MAG[2] + P[8][16]*SH_MAG[5] - P[8][0]*SK_MZ[1] + P[8][1]*SK_MZ[2] - P[8][17]*SK_MZ[3]);
Kfusion[9] = SK_MZ[0]*(P[9][21] + P[9][18]*SH_MAG[2] + P[9][16]*SH_MAG[5] - P[9][0]*SK_MZ[1] + P[9][1]*SK_MZ[2] - P[9][17]*SK_MZ[3]);
Kfusion[10] = SK_MZ[0]*(P[10][21] + P[10][18]*SH_MAG[2] + P[10][16]*SH_MAG[5] - P[10][0]*SK_MZ[1] + P[10][1]*SK_MZ[2] - P[10][17]*SK_MZ[3]);
Kfusion[11] = SK_MZ[0]*(P[11][21] + P[11][18]*SH_MAG[2] + P[11][16]*SH_MAG[5] - P[11][0]*SK_MZ[1] + P[11][1]*SK_MZ[2] - P[11][17]*SK_MZ[3]);
Kfusion[12] = SK_MZ[0]*(P[12][21] + P[12][18]*SH_MAG[2] + P[12][16]*SH_MAG[5] - P[12][0]*SK_MZ[1] + P[12][1]*SK_MZ[2] - P[12][17]*SK_MZ[3]);
Kfusion[13] = SK_MZ[0]*(P[13][21] + P[13][18]*SH_MAG[2] + P[13][16]*SH_MAG[5] - P[13][0]*SK_MZ[1] + P[13][1]*SK_MZ[2] - P[13][17]*SK_MZ[3]);
Kfusion[14] = SK_MZ[0]*(P[14][21] + P[14][18]*SH_MAG[2] + P[14][16]*SH_MAG[5] - P[14][0]*SK_MZ[1] + P[14][1]*SK_MZ[2] - P[14][17]*SK_MZ[3]);
Kfusion[15] = SK_MZ[0]*(P[15][21] + P[15][18]*SH_MAG[2] + P[15][16]*SH_MAG[5] - P[15][0]*SK_MZ[1] + P[15][1]*SK_MZ[2] - P[15][17]*SK_MZ[3]);
// zero Kalman gains to inhibit wind state estimation
if (!inhibitWindStates) {
Kfusion[22] = SK_MZ[0]*(P[22][21] + P[22][18]*SH_MAG[2] + P[22][16]*SH_MAG[5] - P[22][0]*SK_MZ[1] + P[22][1]*SK_MZ[2] - P[22][17]*SK_MZ[3]);
Kfusion[23] = SK_MZ[0]*(P[23][21] + P[23][18]*SH_MAG[2] + P[23][16]*SH_MAG[5] - P[23][0]*SK_MZ[1] + P[23][1]*SK_MZ[2] - P[23][17]*SK_MZ[3]);
} else {
Kfusion[22] = 0.0f;
Kfusion[23] = 0.0f;
}
// zero Kalman gains to inhibit magnetic field state estimation
if (!inhibitMagStates) {
Kfusion[16] = SK_MZ[0]*(P[16][21] + P[16][18]*SH_MAG[2] + P[16][16]*SH_MAG[5] - P[16][0]*SK_MZ[1] + P[16][1]*SK_MZ[2] - P[16][17]*SK_MZ[3]);
Kfusion[17] = SK_MZ[0]*(P[17][21] + P[17][18]*SH_MAG[2] + P[17][16]*SH_MAG[5] - P[17][0]*SK_MZ[1] + P[17][1]*SK_MZ[2] - P[17][17]*SK_MZ[3]);
Kfusion[18] = SK_MZ[0]*(P[18][21] + P[18][18]*SH_MAG[2] + P[18][16]*SH_MAG[5] - P[18][0]*SK_MZ[1] + P[18][1]*SK_MZ[2] - P[18][17]*SK_MZ[3]);
Kfusion[19] = SK_MZ[0]*(P[19][21] + P[19][18]*SH_MAG[2] + P[19][16]*SH_MAG[5] - P[19][0]*SK_MZ[1] + P[19][1]*SK_MZ[2] - P[19][17]*SK_MZ[3]);
Kfusion[20] = SK_MZ[0]*(P[20][21] + P[20][18]*SH_MAG[2] + P[20][16]*SH_MAG[5] - P[20][0]*SK_MZ[1] + P[20][1]*SK_MZ[2] - P[20][17]*SK_MZ[3]);
Kfusion[21] = SK_MZ[0]*(P[21][21] + P[21][18]*SH_MAG[2] + P[21][16]*SH_MAG[5] - P[21][0]*SK_MZ[1] + P[21][1]*SK_MZ[2] - P[21][17]*SK_MZ[3]);
} else {
for (uint8_t i=16; i<=21; i++) {
Kfusion[i] = 0.0f;
}
}
// set flags to indicate to other processes that fusion has been performede and is required on the next frame
// this can be used by other fusion processes to avoid fusing on the same frame as this expensive step
magFusePerformed = true;
magFuseRequired = false;
hal.util->perf_end(_perf_test[4]);
}
hal.util->perf_begin(_perf_test[5]);
// correct the covariance P = (I - K*H)*P
// take advantage of the empty columns in KH to reduce the
// number of operations
for (unsigned i = 0; i<=stateIndexLim; i++) {
for (unsigned j = 0; j<=2; j++) {
KH[i][j] = Kfusion[i] * H_MAG[j];
}
for (unsigned j = 3; j<=15; j++) {
KH[i][j] = 0.0f;
}
for (unsigned j = 16; j<=21; j++) {
KH[i][j] = Kfusion[i] * H_MAG[j];
}
for (unsigned j = 22; j<=23; j++) {
KH[i][j] = 0.0f;
}
}
for (unsigned j = 0; j<=stateIndexLim; j++) {
for (unsigned i = 0; i<=stateIndexLim; i++) {
ftype res = 0;
res += KH[i][0] * P[0][j];
res += KH[i][1] * P[1][j];
res += KH[i][2] * P[2][j];
res += KH[i][16] * P[16][j];
res += KH[i][17] * P[17][j];
res += KH[i][18] * P[18][j];
res += KH[i][19] * P[19][j];
res += KH[i][20] * P[20][j];
res += KH[i][21] * P[21][j];
KHP[i][j] = res;
}
}
// Check that we are not going to drive any variances negative and skip the update if so
bool healthyFusion = true;
for (uint8_t i= 0; i<=stateIndexLim; i++) {
if (KHP[i][i] > P[i][i]) {
healthyFusion = false;
}
}
if (healthyFusion) {
// update the covariance matrix
for (uint8_t i= 0; i<=stateIndexLim; i++) {
for (uint8_t j= 0; j<=stateIndexLim; j++) {
P[i][j] = P[i][j] - KHP[i][j];
}
}
// force the covariance matrix to be symmetrical and limit the variances to prevent ill-condiioning.
ForceSymmetry();
ConstrainVariances();
// update the states
// zero the attitude error state - by definition it is assumed to be zero before each observaton fusion
stateStruct.angErr.zero();
// correct the state vector
for (uint8_t j= 0; j<=stateIndexLim; j++) {
statesArray[j] = statesArray[j] - Kfusion[j] * innovMag[obsIndex];
}
// the first 3 states represent the angular misalignment vector. This is
// is used to correct the estimated quaternion on the current time step
stateStruct.quat.rotate(stateStruct.angErr);
} else {
// record bad axis
if (obsIndex == 0) {
faultStatus.bad_xmag = true;
} else if (obsIndex == 1) {
faultStatus.bad_ymag = true;
} else if (obsIndex == 2) {
faultStatus.bad_zmag = true;
}
CovarianceInit();
hal.util->perf_end(_perf_test[5]);
return;
}
hal.util->perf_end(_perf_test[5]);
}
/*
* Fuse magnetic heading measurement using explicit algebraic equations generated with Matlab symbolic toolbox.
* The script file used to generate these and other equations in this filter can be found here:
* https://github.com/priseborough/InertialNav/blob/master/derivations/RotationVectorAttitudeParameterisation/GenerateNavFilterEquations.m
* This fusion method only modifies the orientation, does not require use of the magnetic field states and is computationally cheaper.
* It is suitable for use when the external magnetic field environment is disturbed (eg close to metal structures, on ground).
* It is not as robust to magnetometer failures.
* It is not suitable for operation where the horizontal magnetic field strength is weak (within 30 degrees latitude of the the magnetic poles)
*/
void NavEKF2_core::fuseEulerYaw()
{
float q0 = stateStruct.quat[0];
float q1 = stateStruct.quat[1];
float q2 = stateStruct.quat[2];
float q3 = stateStruct.quat[3];
// compass measurement error variance (rad^2)
const float R_YAW = sq(frontend->_yawNoise);
// calculate observation jacobian, predicted yaw and zero yaw body to earth rotation matrix
// determine if a 321 or 312 Euler sequence is best
float predicted_yaw;
float measured_yaw;
float H_YAW[3];
Matrix3f Tbn_zeroYaw;
if (fabsf(prevTnb[0][2]) < fabsf(prevTnb[1][2])) {
// calculate observation jacobian when we are observing the first rotation in a 321 sequence
float t2 = q0*q0;
float t3 = q1*q1;
float t4 = q2*q2;
float t5 = q3*q3;
float t6 = t2+t3-t4-t5;
float t7 = q0*q3*2.0f;
float t8 = q1*q2*2.0f;
float t9 = t7+t8;
float t10 = sq(t6);
if (t10 > 1e-6f) {
t10 = 1.0f / t10;
} else {
return;
}
float t11 = t9*t9;
float t12 = t10*t11;
float t13 = t12+1.0f;
float t14;
if (fabsf(t13) > 1e-3f) {
t14 = 1.0f/t13;
} else {
return;
}
float t15 = 1.0f/t6;
H_YAW[0] = 0.0f;
H_YAW[1] = t14*(t15*(q0*q1*2.0f-q2*q3*2.0f)+t9*t10*(q0*q2*2.0f+q1*q3*2.0f));
H_YAW[2] = t14*(t15*(t2-t3+t4-t5)+t9*t10*(t7-t8));
// calculate predicted and measured yaw angle
Vector3f euler321;
stateStruct.quat.to_euler(euler321.x, euler321.y, euler321.z);
predicted_yaw = euler321.z;
if (use_compass() && yawAlignComplete && magStateInitComplete) {
// Use measured mag components rotated into earth frame to measure yaw
Tbn_zeroYaw.from_euler(euler321.x, euler321.y, 0.0f);
Vector3f magMeasNED = Tbn_zeroYaw*magDataDelayed.mag;
measured_yaw = wrap_PI(-atan2f(magMeasNED.y, magMeasNED.x) + _ahrs->get_compass()->get_declination());
} else if (extNavUsedForYaw) {
// Get the yaw angle from the external vision data
extNavDataDelayed.quat.to_euler(euler321.x, euler321.y, euler321.z);
measured_yaw = euler321.z;
} else {
// no data so use predicted to prevent unconstrained variance growth
measured_yaw = predicted_yaw;
}
} else {
// calculate observaton jacobian when we are observing a rotation in a 312 sequence
float t2 = q0*q0;
float t3 = q1*q1;
float t4 = q2*q2;
float t5 = q3*q3;
float t6 = t2-t3+t4-t5;
float t7 = q0*q3*2.0f;
float t10 = q1*q2*2.0f;
float t8 = t7-t10;
float t9 = sq(t6);
if (t9 > 1e-6f) {
t9 = 1.0f/t9;
} else {
return;
}
float t11 = t8*t8;
float t12 = t9*t11;
float t13 = t12+1.0f;
float t14;
if (fabsf(t13) > 1e-3f) {
t14 = 1.0f/t13;
} else {
return;
}
float t15 = 1.0f/t6;
H_YAW[0] = -t14*(t15*(q0*q2*2.0+q1*q3*2.0)-t8*t9*(q0*q1*2.0-q2*q3*2.0));
H_YAW[1] = 0.0f;
H_YAW[2] = t14*(t15*(t2+t3-t4-t5)+t8*t9*(t7+t10));
// calculate predicted and measured yaw angle
Vector3f euler312 = stateStruct.quat.to_vector312();
predicted_yaw = euler312.z;
if (use_compass() && yawAlignComplete && magStateInitComplete) {
// Use measured mag components rotated into earth frame to measure yaw
Tbn_zeroYaw.from_euler312(euler312.x, euler312.y, 0.0f);
Vector3f magMeasNED = Tbn_zeroYaw*magDataDelayed.mag;
measured_yaw = wrap_PI(-atan2f(magMeasNED.y, magMeasNED.x) + _ahrs->get_compass()->get_declination());
} else if (extNavUsedForYaw) {
// Get the yaw angle from the external vision data
euler312 = extNavDataDelayed.quat.to_vector312();
measured_yaw = euler312.z;
} else {
// no data so use predicted to prevent unconstrained variance growth
measured_yaw = predicted_yaw;
}
}
// Calculate the innovation
float innovation = wrap_PI(predicted_yaw - measured_yaw);
// Copy raw value to output variable used for data logging
innovYaw = innovation;
// Calculate innovation variance and Kalman gains, taking advantage of the fact that only the first 3 elements in H are non zero
float PH[3];
float varInnov = R_YAW;
for (uint8_t rowIndex=0; rowIndex<=2; rowIndex++) {
PH[rowIndex] = 0.0f;
for (uint8_t colIndex=0; colIndex<=2; colIndex++) {
PH[rowIndex] += P[rowIndex][colIndex]*H_YAW[colIndex];
}
varInnov += H_YAW[rowIndex]*PH[rowIndex];
}
float varInnovInv;
if (varInnov >= R_YAW) {
varInnovInv = 1.0f / varInnov;
// output numerical health status
faultStatus.bad_yaw = false;
} else {
// the calculation is badly conditioned, so we cannot perform fusion on this step
// we reset the covariance matrix and try again next measurement
CovarianceInit();
// output numerical health status
faultStatus.bad_yaw = true;
return;
}
// calculate Kalman gain
for (uint8_t rowIndex=0; rowIndex<=stateIndexLim; rowIndex++) {
Kfusion[rowIndex] = 0.0f;
for (uint8_t colIndex=0; colIndex<=2; colIndex++) {
Kfusion[rowIndex] += P[rowIndex][colIndex]*H_YAW[colIndex];
}
Kfusion[rowIndex] *= varInnovInv;
}
// calculate the innovation test ratio
yawTestRatio = sq(innovation) / (sq(MAX(0.01f * (float)frontend->_yawInnovGate, 1.0f)) * varInnov);
// Declare the magnetometer unhealthy if the innovation test fails
if (yawTestRatio > 1.0f) {
magHealth = false;
// On the ground a large innovation could be due to large initial gyro bias or magnetic interference from nearby objects
// If we are flying, then it is more likely due to a magnetometer fault and we should not fuse the data
if (inFlight) {
return;
}
} else {
magHealth = true;
}
// limit the innovation so that initial corrections are not too large
if (innovation > 0.5f) {
innovation = 0.5f;
} else if (innovation < -0.5f) {
innovation = -0.5f;
}
// correct the covariance using P = P - K*H*P taking advantage of the fact that only the first 3 elements in H are non zero
// calculate K*H*P
for (uint8_t row = 0; row <= stateIndexLim; row++) {
for (uint8_t column = 0; column <= 2; column++) {
KH[row][column] = Kfusion[row] * H_YAW[column];
}
}
for (uint8_t row = 0; row <= stateIndexLim; row++) {
for (uint8_t column = 0; column <= stateIndexLim; column++) {
float tmp = KH[row][0] * P[0][column];
tmp += KH[row][1] * P[1][column];
tmp += KH[row][2] * P[2][column];
KHP[row][column] = tmp;
}
}
// Check that we are not going to drive any variances negative and skip the update if so
bool healthyFusion = true;
for (uint8_t i= 0; i<=stateIndexLim; i++) {
if (KHP[i][i] > P[i][i]) {
healthyFusion = false;
}
}
if (healthyFusion) {
// update the covariance matrix
for (uint8_t i= 0; i<=stateIndexLim; i++) {
for (uint8_t j= 0; j<=stateIndexLim; j++) {
P[i][j] = P[i][j] - KHP[i][j];
}
}
// force the covariance matrix to be symmetrical and limit the variances to prevent ill-condiioning.
ForceSymmetry();
ConstrainVariances();
// zero the attitude error state - by definition it is assumed to be zero before each observaton fusion
stateStruct.angErr.zero();
// correct the state vector
for (uint8_t i=0; i<=stateIndexLim; i++) {
statesArray[i] -= Kfusion[i] * innovation;
}
// the first 3 states represent the angular misalignment vector. This is
// is used to correct the estimated quaternion on the current time step
stateStruct.quat.rotate(stateStruct.angErr);
// record fusion event
faultStatus.bad_yaw = false;
lastYawTime_ms = imuSampleTime_ms;
} else {
// record fusion numerical health status
faultStatus.bad_yaw = true;
}
}
/*
* Fuse declination angle using explicit algebraic equations generated with Matlab symbolic toolbox.
* The script file used to generate these and other equations in this filter can be found here:
* https://github.com/priseborough/InertialNav/blob/master/derivations/RotationVectorAttitudeParameterisation/GenerateNavFilterEquations.m
* This is used to prevent the declination of the EKF earth field states from drifting during operation without GPS
* or some other absolute position or velocity reference
*/
void NavEKF2_core::FuseDeclination(float declErr)
{