Digital Signal Processing Reference
In-Depth Information
B
=
a
x
B
x
+
a
y
B
y
+
a
z
B
z
B
×
A
A
×
B
A
=
a
x
A
x
+
a
y
A
y
+
a
z
A
z
Figure 2-2
Graphical representation of the cross product.
2.2.4 Vector and Scalar Fields
In electromagnetic theory, a
field
is defined as a mathematical function of space
and time. Fields can be classified as either scalar or vector. A
scalar field
has a
specific value (magnitude) at every point in a region of space at each instance in
time. Figure 2-3 shows two examples of a scalar field, temperature in a block of
material and the voltage across a resistive strip. Note that each point
P
(
x
,
y
,
z
),
there exists a corresponding temperature
T
(
x
,
y
,
z
) or voltage
v
(
x
) at any instant
in time. Other examples of scalar fields are pressure and density. A
vector field
has a variable magnitude and direction at any point in time, as illustrated with
Figure 2-4. Note that the velocity and direction of the fluid inside the pipe changes
in the vicinity of the neck-down region, so the magnitude and direction (phase)
of the vectors that describe the motion of the fluid at a given instant in time are a
function of the position in space. Other examples of vector fields are acceleration
and electric and magnetic fields.
2.2.5 Flux
A vector field,
F
(
x
,
y
,
z
,
t
), can be represented graphically by depicting a large
number of individual vectors with a specific magnitude and phase (direction);
however, this is cumbersome. A more useful method for representation of a
vector field is to use the concept of flux.
Flux
is a measure of how many field
vectors pass though a surface in space, as depicted in Figure 2-5a. The net flux
of vector field
F
through surface
S
is shown as
S
F
·
ψ
=
d
s
(2-17)
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