Cartesian Components of a Vector
Consider a Cartesian coordinate system consisting of
an origin, , and three mutually perpendicular coordinate axes, , , and
. See Figure A.4. Such a system is said to be right-handed if, when looking along the direction, a clockwise
rotation about is required to take into . Otherwise, it is said to be left-handed. In physics, it is conventional to always use right-handed coordinate systems.
Figure A.4:
A right-handed Cartesian coordinate system.
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It is convenient to define unit vectors, , , and , parallel to , , and , respectively.
Incidentally, a unit vector is a vector whose magnitude is unity. The position vector, , of some general point whose Cartesian coordinates
are (, , ) is then given by
|
(1.11) |
In other words, we can get from to by moving a distance parallel to , then a distance
parallel to , and then a distance parallel to . Similarly, if is an arbitrary vector then
|
(1.12) |
where , , and are termed the Cartesian components of . It is conventional to write
.
It follows that
,
, and
. Of course,
.
According to the three-dimensional generalization of the Pythagorean theorem, the distance
is
given by
|
(1.13) |
By analogy, the magnitude of a general vector takes the form
|
(1.14) |
If
and
then it is
easily demonstrated that
|
(1.15) |
Furthermore, if is a scalar then it is apparent that
|
(1.16) |