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30 CHAPTER 4. METHOD<br />

Hinge Joint<br />

A hinge joint does not have any influence on the position accuracy of the joint frame, because it represents<br />

a rotation and not a translation. Thus it only effects the position accuracy of Child frames. The<br />

angular uncertainty of the model must therefor be applied when calculating the position uncertainty<br />

of the Child frames.<br />

To perform the mapping for a model of a hinge joint to Cartesian space, additionally the distance<br />

d must be known. This value describes the distance from the origin of the Child frame to the origin of<br />

the joint frame. This distance is measured in the plane perpendicular to the axis of rotation. Together<br />

the distance d and the angle s from the model describe a point in polar coordinates. In the following<br />

equations, which describe the mapping steps the value s and σ 2 s are named α and σ 2 α. The velocity in<br />

the model is only necessary for the propagation of the position and thus not used for the mapping.<br />

The mapping of polar coordinates to Cartesian coordinates can be done by simply using trigonometrical<br />

functions. Figure 4.10 visualizes the relationship of polar and Cartesian coordinates, where<br />

Y<br />

1<br />

d<br />

U<br />

α<br />

1 2<br />

X<br />

Figure 4.10: Mapping of polar to Cartesian coordinates.<br />

the point U with polar coordinates d, α is mapped into Cartesian coordinates with x, y. The equations<br />

for calculating the values of x and y simply are<br />

x = d · cos α<br />

y = d · sin α<br />

This relationship can also be seen as a function F which transforms the polar coordinates [ d<br />

into Cartesian coordinates [ x<br />

y ] T . This relationship can be written as<br />

([ d<br />

F<br />

α])<br />

=<br />

[ x<br />

=<br />

y]<br />

[ ] d · cos α<br />

d · sin α<br />

α ] T<br />

The normal distributed uncertainty Σ dα can be mapped from polar to Cartesian space with the<br />

same function F . Since the new uncertainty should also be normal distributed, the mean and variance<br />

must satisfy the equations<br />

with<br />

[ x<br />

y]<br />

[<br />

µx<br />

µ y<br />

]<br />

∼<br />

N<br />

= F<br />

([<br />

µx<br />

µ y<br />

]<br />

, Σ xy<br />

)<br />

([<br />

µd<br />

µ α<br />

])<br />

=<br />

[ ]<br />

µd · cos α<br />

µ d · sin α<br />

The Cartesian covariance matrix Σ xy can be calculated out of the polar covariance matrix Σ dα by

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