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The magnitude condition is a constraint that is satisfied by the locus of points in the s-plane on which closed-loop poles of a system reside. In combination with the angle condition , these two mathematical expressions fully determine the root locus .
Let the characteristic equation of a system be
1
+
G
(
s
)
=
0
{\displaystyle 1+{\textbf {G}}(s)=0}
, where
G
(
s
)
=
P
(
s
)
Q
(
s
)
{\displaystyle {\textbf {G}}(s)={\frac {{\textbf {P}}(s)}{{\textbf {Q}}(s)}}}
. Rewriting the equation in polar form is useful.
e
j
2
π
+
G
(
s
)
=
0
{\displaystyle e^{j2\pi }+{\textbf {G}}(s)=0}
G
(
s
)
=
−
1
=
e
j
(
π
+
2
k
π
)
{\displaystyle {\textbf {G}}(s)=-1=e^{j(\pi +2k\pi )}}
where
(
k
=
0
,
1
,
2
,
.
.
.
)
{\displaystyle (k=0,1,2,...)}
are the only solutions to this equation. Rewriting
G
(
s
)
{\displaystyle {\textbf {G}}(s)}
in factored form ,
G
(
s
)
=
P
(
s
)
Q
(
s
)
=
K
(
s
−
a
1
)
(
s
−
a
2
)
⋯
(
s
−
a
n
)
(
s
−
b
1
)
(
s
−
b
2
)
⋯
(
s
−
b
m
)
,
{\displaystyle {\textbf {G}}(s)={\frac {{\textbf {P}}(s)}{{\textbf {Q}}(s)}}=K{\frac {(s-a_{1})(s-a_{2})\cdots (s-a_{n})}{(s-b_{1})(s-b_{2})\cdots (s-b_{m})}},}
and representing each factor
(
s
−
a
p
)
{\displaystyle (s-a_{p})}
and
(
s
−
b
q
)
{\displaystyle (s-b_{q})}
by their vector equivalents,
A
p
e
j
θ
p
{\displaystyle A_{p}e^{j\theta _{p}}}
and
B
q
e
j
ϕ
q
{\displaystyle B_{q}e^{j\phi _{q}}}
, respectively,
G
(
s
)
{\displaystyle {\textbf {G}}(s)}
may be rewritten.
G
(
s
)
=
K
A
1
A
2
⋯
A
n
e
j
(
θ
1
+
θ
2
+
⋯
+
θ
n
)
B
1
B
2
⋯
B
m
e
j
(
ϕ
1
+
ϕ
2
+
⋯
+
ϕ
m
)
{\displaystyle {\textbf {G}}(s)=K{\frac {A_{1}A_{2}\cdots A_{n}e^{j(\theta _{1}+\theta _{2}+\cdots +\theta _{n})}}{B_{1}B_{2}\cdots B_{m}e^{j(\phi _{1}+\phi _{2}+\cdots +\phi _{m})}}}}
Simplifying the characteristic equation,
e
j
(
π
+
2
k
π
)
=
K
A
1
A
2
⋯
A
n
e
j
(
θ
1
+
θ
2
+
⋯
+
θ
n
)
B
1
B
2
⋯
B
m
e
j
(
ϕ
1
+
ϕ
2
+
⋯
+
ϕ
m
)
=
K
A
1
A
2
⋯
A
n
B
1
B
2
⋯
B
m
e
j
(
θ
1
+
θ
2
+
⋯
+
θ
n
−
(
ϕ
1
+
ϕ
2
+
⋯
+
ϕ
m
)
)
,
{\displaystyle {\begin{aligned}e^{j(\pi +2k\pi )}&=K{\frac {A_{1}A_{2}\cdots A_{n}e^{j(\theta _{1}+\theta _{2}+\cdots +\theta _{n})}}{B_{1}B_{2}\cdots B_{m}e^{j(\phi _{1}+\phi _{2}+\cdots +\phi _{m})}}}\\&=K{\frac {A_{1}A_{2}\cdots A_{n}}{B_{1}B_{2}\cdots B_{m}}}e^{j(\theta _{1}+\theta _{2}+\cdots +\theta _{n}-(\phi _{1}+\phi _{2}+\cdots +\phi _{m}))},\end{aligned}}}
from which we derive the magnitude condition:
1
=
K
A
1
A
2
⋯
A
n
B
1
B
2
⋯
B
m
.
{\displaystyle 1=K{\frac {A_{1}A_{2}\cdots A_{n}}{B_{1}B_{2}\cdots B_{m}}}.}
The angle condition is derived similarly.