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@jannson
Created April 1, 2014 02:51
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陀螺仪重力传感器融合代码
//=====================================================================================================
// IMU.c
// S.O.H. Madgwick
// 25th September 2010
//=====================================================================================================
// Description:
//
// Quaternion implementation of the 'DCM filter' [Mayhony et al].
//
// User must define 'halfT' as the (sample period / 2), and the filter gains 'Kp' and 'Ki'.
//
// Global variables 'q0', 'q1', 'q2', 'q3' are the quaternion elements representing the estimated
// orientation. See my report for an overview of the use of quaternions in this application.
//
// User must call 'IMUupdate()' every sample period and parse calibrated gyroscope ('gx', 'gy', 'gz')
// and accelerometer ('ax', 'ay', 'ay') data. Gyroscope units are radians/second, accelerometer
// units are irrelevant as the vector is normalised.
//
//=====================================================================================================
//----------------------------------------------------------------------------------------------------
// Header files
#include "IMU.h"
#include <math.h>
//----------------------------------------------------------------------------------------------------
// Definitions
#define Kp 2.0f // proportional gain governs rate of convergence to accelerometer/magnetometer
#define Ki 0.005f // integral gain governs rate of convergence of gyroscope biases
#define halfT 0.5f // half the sample period
//---------------------------------------------------------------------------------------------------
// Variable definitions
float q0 = 1, q1 = 0, q2 = 0, q3 = 0; // quaternion elements representing the estimated orientation
float exInt = 0, eyInt = 0, ezInt = 0; // scaled integral error
//====================================================================================================
// Function
//====================================================================================================
void IMUupdate(float gx, float gy, float gz, float ax, float ay, float az) {
float norm;
float vx, vy, vz;
float ex, ey, ez;
// normalise the measurements
norm = sqrt(ax*ax + ay*ay + az*az);
ax = ax / norm;
ay = ay / norm;
az = az / norm;
把加计的三维向量转成单位向量。
// estimated direction of gravity
vx = 2*(q1*q3 - q0*q2);
vy = 2*(q0*q1 + q2*q3);
vz = q0*q0 - q1*q1 - q2*q2 + q3*q3;
这是把四元数换算成《方向余弦矩阵》中的第三列的三个元素。
根据余弦矩阵和欧拉角的定义,地理坐标系的重力向量,转到机体坐标系,正好是这三个元素。
所以这里的vx\y\z,其实就是当前的欧拉角(即四元数)的机体坐标参照系上,换算出来的重力单位向量。
// error is sum of cross product between reference direction of field and direction measured by sensor
ex = (ay*vz - az*vy);
ey = (az*vx - ax*vz);
ez = (ax*vy - ay*vx);
axyz是机体坐标参照系上,加速度计测出来的重力向量,也就是实际测出来的重力向量。
axyz是测量得到的重力向量,vxyz是陀螺积分后的姿态来推算出的重力向量,它们都是机体坐标参照系上的重力向量。
那它们之间的误差向量,就是陀螺积分后的姿态和加计测出来的姿态之间的误差。
向量间的误差,可以用向量叉积(也叫向量外积、叉乘)来表示,exyz就是两个重力向量的叉积。
这个叉积向量仍旧是位于机体坐标系上的,而陀螺积分误差也是在机体坐标系,而且叉积的大小与陀螺积分误差成正比,正好拿来纠正陀螺。(你可以自己拿东西想象一下)由于陀螺是对机体直接积分,所以对陀螺的纠正量会直接体现在对机体坐标系的纠正。
// integral error scaled integral gain
exInt = exInt + ex*Ki;
eyInt = eyInt + ey*Ki;
ezInt = ezInt + ez*Ki;
// adjusted gyroscope measurements
gx = gx + Kp*ex + exInt;
gy = gy + Kp*ey + eyInt;
gz = gz + Kp*ez + ezInt;
用叉积误差来做PI修正陀螺零偏
// integrate quaternion rate and normalise
q0 = q0 + (-q1*gx - q2*gy - q3*gz)*halfT;
q1 = q1 + (q0*gx + q2*gz - q3*gy)*halfT;
q2 = q2 + (q0*gy - q1*gz + q3*gx)*halfT;
q3 = q3 + (q0*gz + q1*gy - q2*gx)*halfT;
四元数微分方程
// normalise quaternion
norm = sqrt(q0*q0 + q1*q1 + q2*q2 + q3*q3);
q0 = q0 / norm;
q1 = q1 / norm;
q2 = q2 / norm;
q3 = q3 / norm;
四元数规范化
}
//====================================================================================================
// END OF CODE
//====================================================================================================
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