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161 lines
6.4 KiB
161 lines
6.4 KiB
% IMPORTANT - This script requires the Matlab symbolic toolbox |
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% Author: Paul Riseborough |
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% Last Modified: 16 Feb 2015 |
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% Derivation of a navigation EKF using a local NED earth Tangent Frame for |
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% the initial alignment and gyro bias estimation from a moving platform |
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% Based on use of a rotation vector for attitude estimation as described |
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% here: |
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% |
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% Mark E. Pittelkau. "Rotation Vector in Attitude Estimation", |
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% Journal of Guidance, Control, and Dynamics, Vol. 26, No. 6 (2003), |
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% pp. 855-860. |
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% |
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% The benefits for use of rotation error vector over use of a four parameter |
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% quaternion representation of the estiamted orientation are: |
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% a) Reduced computational load |
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% b) Improved stability |
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% c) The ability to recover faster from large orientation errors. This |
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% makes this filter particularly suitable where the initial alignment is |
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% uncertain |
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% State vector: |
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% error rotation vector |
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% Velocity - North, East, Down (m/s) |
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% Delta Angle bias - X,Y,Z (rad) |
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% Observations: |
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% NED velocity - N,E,D (m/s) |
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% body fixed magnetic field vector - X,Y,Z |
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% Time varying parameters: |
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% XYZ delta angle measurements in body axes - rad |
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% XYZ delta velocity measurements in body axes - m/sec |
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% magnetic declination |
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clear all; |
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%% define symbolic variables and constants |
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syms dax day daz real % IMU delta angle measurements in body axes - rad |
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syms dvx dvy dvz real % IMU delta velocity measurements in body axes - m/sec |
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syms q0 q1 q2 q3 real % quaternions defining attitude of body axes relative to local NED |
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syms vn ve vd real % NED velocity - m/sec |
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syms dax_b day_b daz_b real % delta angle bias - rad |
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syms dvx_b dvy_b dvz_b real % delta velocity bias - m/sec |
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syms dt real % IMU time step - sec |
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syms gravity real % gravity - m/sec^2 |
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syms daxNoise dayNoise dazNoise dvxNoise dvyNoise dvzNoise real; % IMU delta angle and delta velocity measurement noise |
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syms vwn vwe real; % NE wind velocity - m/sec |
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syms magX magY magZ real; % XYZ body fixed magnetic field measurements - milligauss |
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syms magN magE magD real; % NED earth fixed magnetic field components - milligauss |
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syms R_VN R_VE R_VD real % variances for NED velocity measurements - (m/sec)^2 |
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syms R_MAG real % variance for magnetic flux measurements - milligauss^2 |
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syms rotErr1 rotErr2 rotErr3 real; % error rotation vector |
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%% define the process equations |
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% define the measured Delta angle and delta velocity vectors |
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dAngMeas = [dax; day; daz]; |
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dVelMeas = [dvx; dvy; dvz]; |
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% define the delta angle bias errors |
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dAngBias = [dax_b; day_b; daz_b]; |
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% define the quaternion rotation vector for the state estimate |
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estQuat = [q0;q1;q2;q3]; |
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% define the attitude error rotation vector, where error = truth - estimate |
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errRotVec = [rotErr1;rotErr2;rotErr3]; |
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% define the attitude error quaternion using a first order linearisation |
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errQuat = [1;0.5*errRotVec]; |
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% Define the truth quaternion as the estimate + error |
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truthQuat = QuatMult(estQuat, errQuat); |
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% derive the truth body to nav direction cosine matrix |
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Tbn = Quat2Tbn(truthQuat); |
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% define the truth delta angle |
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% ignore coning acompensation as these effects are negligible in terms of |
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% covariance growth for our application and grade of sensor |
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dAngTruth = dAngMeas - dAngBias - [daxNoise;dayNoise;dazNoise]; |
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% Define the truth delta velocity |
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dVelTruth = dVelMeas - [dvxNoise;dvyNoise;dvzNoise]; |
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% define the attitude update equations |
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% use a first order expansion of rotation to calculate the quaternion increment |
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% acceptable for propagation of covariances |
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deltaQuat = [1; |
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0.5*dAngTruth(1); |
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0.5*dAngTruth(2); |
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0.5*dAngTruth(3); |
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]; |
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truthQuatNew = QuatMult(truthQuat,deltaQuat); |
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% calculate the updated attitude error quaternion with respect to the previous estimate |
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errQuatNew = QuatDivide(truthQuatNew,estQuat); |
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% change to a rotaton vector - this is the error rotation vector updated state |
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errRotNew = 2 * [errQuatNew(2);errQuatNew(3);errQuatNew(4)]; |
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% define the velocity update equations |
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% ignore coriolis terms for linearisation purposes |
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vNew = [vn;ve;vd] + [0;0;gravity]*dt + Tbn*dVelTruth; |
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% define the IMU bias error update equations |
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dabNew = [dax_b; day_b; daz_b]; |
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% Define the state vector & number of states |
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stateVector = [errRotVec;vn;ve;vd;dAngBias]; |
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nStates=numel(stateVector); |
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%% derive the covariance prediction equation |
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% This reduces the number of floating point operations by a factor of 6 or |
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% more compared to using the standard matrix operations in code |
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% Define the control (disturbance) vector. Error growth in the inertial |
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% solution is assumed to be driven by 'noise' in the delta angles and |
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% velocities, after bias effects have been removed. This is OK because we |
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% have sensor bias accounted for in the state equations. |
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distVector = [daxNoise;dayNoise;dazNoise;dvxNoise;dvyNoise;dvzNoise]; |
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% derive the control(disturbance) influence matrix |
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G = jacobian([errRotNew;vNew;dabNew], distVector); |
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G = subs(G, {'rotErr1', 'rotErr2', 'rotErr3'}, {0,0,0}); |
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% derive the state error matrix |
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distMatrix = diag(distVector); |
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Q = G*distMatrix*transpose(G); |
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f = matlabFunction(Q,'file','calcQ.m'); |
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% derive the state transition matrix |
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vNew = subs(vNew,{'daxNoise','dayNoise','dazNoise','dvxNoise','dvyNoise','dvzNoise'}, {0,0,0,0,0,0}); |
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errRotNew = subs(errRotNew,{'daxNoise','dayNoise','dazNoise','dvxNoise','dvyNoise','dvzNoise'}, {0,0,0,0,0,0}); |
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F = jacobian([errRotNew;vNew;dabNew], stateVector); |
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F = subs(F, {'rotErr1', 'rotErr2', 'rotErr3'}, {0,0,0}); |
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f = matlabFunction(F,'file','calcF.m'); |
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% define a symbolic covariance matrix using strings to represent |
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% '_l_' to represent '( ' |
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% '_c_' to represent , |
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% '_r_' to represent ')' |
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% these can be substituted later to create executable code |
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% for rowIndex = 1:nStates |
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% for colIndex = 1:nStates |
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% eval(['syms OP_l_',num2str(rowIndex),'_c_',num2str(colIndex), '_r_ real']); |
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% eval(['P(',num2str(rowIndex),',',num2str(colIndex), ') = OP_l_',num2str(rowIndex),'_c_',num2str(colIndex),'_r_;']); |
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% end |
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% end |
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% Derive the predicted covariance matrix using the standard equation |
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% nextP = F*P*transpose(F) + Q; |
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% f = matlabFunction(nextP,'file','calcP.m'); |
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%% derive equations for fusion of magnetic deviation measurement |
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% rotate body measured field into earth axes |
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magMeasNED = Tbn*[magX;magY;magZ]; |
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% the predicted measurement is the angle wrt true north of the horizontal |
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% component of the measured field |
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angMeas = tan(magMeasNED(2)/magMeasNED(1)); |
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H_MAG = jacobian(angMeas,stateVector); % measurement Jacobian |
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H_MAG = subs(H_MAG, {'rotErr1', 'rotErr2', 'rotErr3'}, {0,0,0}); |
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f = matlabFunction(H_MAG,'file','calcH_MAG.m');
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