Eigenvector slew

Eigenvector slew

In aerospace engineering, especially those areas dealing with spacecraft, the eigenvector slew is a method to calculate a steering correction (called a slew) by rotating the spacecraft around one fixed axis. This correponds in general to the fastest and most efficient way to reach the desired target orientation as there is only one acceleration phase and one braking phase for the angular rate. If this fixed axis is not a principal axis a time varying torque must be applied to force the spacecraft to rotate as desired, though. Also the gyroscopic effect of momentum wheels must be compensated for.

That such a rotation exists corresponds precisely to a main result of the mathematical theory of rotation operators, the (only) eigenvector of the rotation operator corresponding to the desired re-orientation is this axis.

Given the current orientation of the craft, and the desired orientation of the craft in cartesian coordinates, the required axis of rotation and corresponding rotation angle to achieve the new orientation is determined by computing the eigenvector of the rotation operator.

Problem

Let

:hat{x} , hat{y} , hat{z}

be a body fixed reference system for a 3 axis stabilized spacecraft. The initial attitudeis given by

:hat{x}=hat{a}:hat{y}=hat{b}:hat{z}=hat{c}.

One wants to find an axis relative the spacecraft body

:hat{r}=r_x cdot hat{x} +r_y cdot hat{y} +r_z cdot hat{z}

and a rotation angle alpha such that after the rotation with the angle alpha one has that

:hat{x}=hat{d}:hat{y}=hat{e}:hat{z}=hat{f}

where

:hat{d} , hat{e} , hat{f}

are the new target directions.

In vector form this means that

:hat{d}=r_a cdot hat{r} + cos alpha cdot ( hat{a} - r_a cdot hat{r})+ sin alpha cdot hat{r} imes hat{a}:hat{e}=r_b cdot hat{r} + cos alpha cdot ( hat{b} - r_b cdot hat{r})+ sin alpha cdot hat{r} imes hat{b}:hat{f}=r_c cdot hat{r} + cos alpha cdot ( hat{c} - r_c cdot hat{r})+ sin alpha cdot hat{r} imes hat{c}.

Solution

In terms of linear algebra this means that one wants to find an eigenvector with the eigenvalue = 1 for the linear mapping defined by

:hat{a} longrightarrow hat{d}:hat{b} longrightarrow hat{e}:hat{c} longrightarrow hat{f}

which relative to the

:hat{a} , hat{b} , hat{c}

coordinate system has the matrix

:egin{bmatrix}langle hat{d}| hat{a} angle & langlehat{e}| hat{a} angle & langlehat{f}| hat{a} angle \langlehat{d}| hat{b} angle & langlehat{e}| hat{b} angle & langlehat{f}| hat{b} angle \langlehat{d}| hat{c} angle & langlehat{e}| hat{c} angle & langlehat{f}| hat{c} angleend{bmatrix}

Because this is the matrix of the rotation operator relative the base vector system hat{a} , hat{b} , hat{c} the eigenvalue can be determined with the algorithm described in "Rotation operator (vector space)".

With the notations used here this is:

:cos alpha=frac{langlehat{d}| hat{a} angle+langlehat{e}| hat{b} angle+langlehat{f}| hat{c} angle-1}{2}:r_a=langlehat{f}| hat{b} angle-langlehat{e}| hat{c} angle:r_b=langlehat{d}| hat{c} angle-langlehat{f}| hat{a} angle:r_c=langlehat{e}| hat{a} angle-langlehat{d}| hat{b} angle:|ar{r}|=sqrtr_a}^2+{r_b}^2+{r_c}^2}:sin alpha=frac{2}

The rotation angle alpha is

:alpha=operatorname{arg}(cos alpha,sin alpha)

where "operatorname{arg}(x , y)" is the polar argument of the vector ( x , y ) corresponding to the function function ATAN2(y,x) (or in double precision DATAN2(y,x)) available in for example the programming language FORTRAN.

The resulting alpha will be in the interval 0 le alpha le pi.

If 0 < alpha < pi then |ar{r}| > 0 and the uniquely defined rotation (unit) vector is:

:hat{r}=frac{ar{r

Note that :langlehat{d}| hat{a} angle +langlehat{e}| hat{b} angle+langlehat{f}| hat{c} angle

is the trace of the matrix defined by the orthogonal linear mapping and that the components of the "eigenvector" are fixed and constant during the rotation, i.e. :hat{r}=r_x cdot hat{x}(t) +r_y cdot hat{y}(t) +r_z cdot hat{z}(t)=r_x cdot hat{a} +r_y cdot hat{b} +r_z cdot hat{c}=r_x cdot hat{d} +r_y cdot hat{e} +r_z cdot hat{f}where hat{x} , hat{y} , hat{z} are moving with time t during the slew.

See also

* Rotation operator (vector space)
* Slew (spacecraft)


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