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Transcript of 1 Circuit Laws and Theorems-5
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Indian Institute of Technology Guwahati
Department of Electronics & Electrical Engineering
1
EE 101
Electrical Sciences
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Syllabus
Fundamental Laws of Electrical Engineering
Coulombs law
Ohms law
Kirchoffs law
Amperes law
Faradays law of electromagnetic induction
The circuit elements
Ideal independent current and voltage sources
Energy and power
Resistance, inductance and capacitance
Network Theory Series and parallel combination of circuit elements
Network analysis by mesh currents and node pair voltages
Thevenins theorem, Nortons theorem
Network reduction by star delta transformation
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Syllabus
Circuit differential equations
The differential operator General formulation of circuit differential equations
The forced solutions, and natural response
Circuit Dynamics and Forced Responses
First order circuits (R-L,R-Ccircuits)
Sinusoidal Steady State Response of Circuits
Average and effective values of a periodic function
Instantaneous and average power, power factor
Phasor representation of sinusoids
Application of network theorems to complex impedances, and
Balanced three phase circuits
Star and delta connected sources
Star and delta connected loads
Balanced 3-phase system analysis
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Syllabus
Magnetic Theory and circuits
Definition of Magnetic quantities Theory of magnetism The magnetic circuits Hysteresis and eddy current losses in magnetic materials
Electromechanical energy conversion
Basic analysis of electromagnetic torque Analysis of induced voltage Construction features of electric machines
Transformers Theory of operation and phasor diagrams Equivalent circuit and parameters
Three phase induction machines Theory of operation and phasor diagrams Equivalent circuit and parameters
Introduction to synchronous machines and DC machines
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Books
1. Vincent Del Toro, Electrical Engineering Fundamentals, SecondEdition, PHI Learning Private Limited, New Delhi, 2010.
2. Bhag S. Guru, Huseyin R. Hiziroglu, Electric Machinery and
Transformers, 3rdEdition, Oxford University Press, 2001.
3. G B Shrestha, M H Haque, AC Circuits and Machines, PearsonPrentice Hall, 2006
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Lectures 1-5
DC Circuits:Basic Concepts and Fundamental Laws
Network Techniques and Theorems
Circuit Differential Equations
Transient Behavior of RL, RC Circuits
G. B. Shrestha
Visiting Professor
Department of Electronics & Electrical Engineering
Room CET-102, Ph. x3475, Email: [email protected]
Thanks to
Dr. Praveen Kumar, Associate Professor,
for portions of his Lecture Notes on this topic
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Introduction
There are two broad branches of classical electrical engineering Electric circuit theory
Electromechanical energy conversion
Both these branches are based on of experimentally established
fundamental laws. The electric circuit theory mainly consists of :
Coulomb Law(1785), OhmsLaw (1827),
Faradayslaw (1831), and
Kirchhoff's law (1857)
The electromechanical energy conversion can be treated and analyzed byapplying just two of the fundamental laws, namely AmperesLaw (1825)
and Faraday's Law of Induction (1831).
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Fig.1 shows two pointpositivecharges of values Q1and Q
2separated by a
distance of rmeters.
Charles A. Coulomb showed experimentally that a force of repulsion exists
between Q1and Q2 which is given by
Coulombs law for the force on Q2is also frequently written as
1 2
2
1 2
[N] (1)4
where, and are in coulombs
is the separation between the charges in metres
4 is a proportionality constant, and
is the permittivity of the medium
Q QF
r
Q Q
r
Coulombs Law
2
11 22
[N] 2
And, [N/C] is known as electric field intensity of at .4
F Q
QQ Q
r
E
E =
8
r Q2
Figure 1
Q1
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Permittivity
In equation (1) all the quantities can be known through measurements with
the exception of the proportionality factor .
The factor is a property of the medium in which the experiment is
performed and this factor is known as permittivity. The permittivity of a
substance describes how easy/difficult it is to set up an electric field in it.
When the experiment is performed in a vacuum, the value of thepermittivity is: 0=8.85410
-12 [F/m]
Repeating the Coulombsexperiment in oil for the same values of Q1and
Q2 and r, it is found that the resulting force is only about half as much as
for air.
The permittivity of oil is greater than that of air. A convenient way ofexpressing this difference is to introduce a quantity called relative
permittivity defined as: so that0
/ ,r
1 2
2
0
[N]4 r
Q QF
r
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Potential Difference In Fig. 2 the charge Q1is assumed to be located at some fixed point in space. The
charge Q2is assumed initially to be on a horizontal path from Q1and is infinitelyfar away. In this condition the force between Q1and Q2is zero.
If Q2is moved in the direction of,increasingly larger force is requiredto move closer to Q1.
The force exerted on Q2acts along the line Q1Q2 against the movement whilemoving from infinity up to r2, it follows that work is being done on Q2.
The work done on Q2is stored in the form ofpotential energyand is recovered inthe form of kinetic energyimmediately upon release of the force which keeps Q2fixed at a position r2meters from Q1.
The work done on Q2to bring it from infinity to r2can also be expressed in termsof the electric field intensityassociated with charge Q1(eqs. 1 and 2).
In moving Q2from infinity to r2, work must be done against this electric field.
Q1 Q2Figure 2a
r2
Q2Figure 2
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The quantity, work per unit chargeis also known as voltage,is defined as
work done per coulomb of charge while moving Q2from infinity to r2.
To obtain the voltageit is necessary to perform an integration of the electric
field intensity (eq. 2) with respect to the distance.
Mathematically voltage is defined as:
The minus sign is arbitrarily inserted to indicate that work is done on the
charge against the action of the electric field produced by Q1.
Potential Difference
2
22
2
1
22
workVoltage , or
charge
ie, [V] (3)4
r
WV
Q
Q
V Edr r
Q1 Q2Figure 2a
r2
Q2Figure 2
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To determine thepotential differencebetween any two point charges, another
charge Q3is considered and this charge is moved from infinity to r3.
From Fig. 3 it can be seen that r3is smaller than r2, hence more work per unit
charge must be done to place a charge at point 3.
Mathematically voltage or potential of Q3
is calculated as:
Since V3is greater than V2,
there exists a potential difference between these two points.
When a unit charge moves from a point of higher potential (eg, point 3) to one
of lower potential (eg, point 2) it gives away some energy.
Potential Difference
13
3
[V] (4)4
QV
r
r2Q1 Q2
Figure 3Q1
r3
Q3
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On the basis of experiments, Ohm showed that current flow in a circuit
composed of a battery and conductors can be expressed as
where, Iis the current,
Aand are the cross section and the resistivity of the conductor, and
is the rate of change of voltage along the conductor. In case of a uniform conductor, the current can be expressed as
where, V andLare total voltage and the length of the conductor.
Thus, Ohms law states that the current in a wire is proportional to the voltage
across its ends, which can be expressed as:
where, Ris called the resistance of the conductor.
13
Ohms Law
d [A] (5)
d
A vI
l
= [A] (6)/
A V VI
L L A
/ or where, / (7)I V R V IR R L A
d / dv l
Figure 4
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During Ohms time, experimental verification of his law was achieved
exclusively by using direct current sources, namely the voltaic cells.
Further experimentation has shown that Ohmslaw is also valid when the
potential difference across a linear resistor is time varying. In this case
Ohmslaw is expressed as
The lower case letters are used to indicate
the time varying, non constant natures of
the quantities vand i.
Ohms Law
(8)v iR i
v R
Figure 5
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A negative point charge Q1of magnitude 210-12C is placed in
vacuum.
a. Find the value of the electric field at a point 1 m from the
charge.
b. Compute the work done in bringing an electron from a point
very far removed from Q1to a point 0.5 m from the chargec. What force is acting on the electron in part (b)?
Example
Solutiona. 0.018 V/mb. 0.0576 10-19Joules
c. 115.2 10-22N
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Gustav Robert Kirchhoff published the first systematic formulation of the
principles governing the behavior of the electric circuits. His work is
embodied in two fundamental laws:
Kirchoffscurrent law, and
Kirchoffsvoltage law
Kirchhoff's current law states that the sumof the currents entering (or leaving) a node
at any instant is equal to zero. A node is a
junction in a circuit where two or more
circuit elements are joined together (Fig.6).
Mathematically the law is expressed as:
Kirchhoff's Laws
1
0 (9)
where, number of circuit elements connected to a node.
k
jj
I
k
Figure 6
Node 1
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Applying the Kirchoffscurrent law to node 1 in Fig.6 gives
The Kirchhoff's law is the restatement of
theprinciple of conservation of charge.
It may be noted that if the current entering
a node is taken as +ve, then the currentgoing out of the node will beve, and
vice versa.
For two resistances in parallel, KCL can be
used to show that:
Current division in parallel resistances:
Parallel combination of resistances:
Figure. 6: Kirchhoff's current law
Node 1
Kirchoffs Current Law (KCL)
1 2 3 4 5 6 0 (10)I I I I I I
17
2 11 2
1 2 1 2
, (11)R R
I I I IR R R R
1 2
1 2 1 2
1 1 1, or (12)eq
eq
R RR
R R R R R
I
1
I
2
R
1
R
2
I
I
R
eq
Figure. 7: Parallel Resistances
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Kirchoffs Voltage Law (KVL)
Kirchoffsvoltage law states that at
any instant of time, the sum of the
voltages in a closed circuit is zero.
Application of Kirchhoffs voltage law
to the circuit shown inn Figure.7 gives:
It should be noted that the polarity of
various voltages should be properly taken care of.
For two resistances in series, KVL can be used to show that:
Voltage division in series resistances:
Series combination of resistances:
1 2 3 0 (13)V V V E Figure.8: Kirchhoff's voltage law
18
1 21 2
1 2 1 2
, V (14)R R
V V VR R R R
1 2 (15)eqR R R
Figure. 9: Series Resistances
I
V
1
-
R
1
V
2
-
R
2
V
IR
eq
V -
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For an independent voltage source, the magnitude of the voltage is not
affected by either the magnitude or direction of the current.
The characteristics of an independent voltage source is shown in Fig. 8.
A notable point about the ideal voltage source is its zero internal
resistance. This is readily demonstrated by invoking Ohms law in
incremental form:
It may be noted that an ideal voltage source is capable of supplying any amount
of power, which is not true with practical voltage sources.
Ideal Independent Voltage Source
2 1
From Fig. 8,
0
VR
I
V
R I I
I1 I2
Voltage [V]
Current [A]
Figfure. 8: Characteristics of ideal voltage source
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The ideal independent current source is a two terminal element which
supplies its specified current to the circuit it is connected to, independent
of the value and direction of the voltage appearing across its terminals.
The voltage vs. current characteristics of an ideal current source is shown
In Fig. 9.
It may also be noted that an
ideal current source is capable of
supplying any amount of power,
which is not true with practical
current sources.
Ideal Independent Current Source
V1
V2
Voltage [V]
Current [A]
Figure. 9: Characteristics of ideal current source
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In case of ideal dependent or controlled source, the source quantity is
determined by a voltage or current existing at some other location in thesystem or circuit being analyzed.
The dependent sources appear in the equivalent electrical models for
many electronic devices such as transistors, operational amplifiers and
integrated circuits.
The dependent sources are represented as diamonds to distinguish them
from independent sources (Fig. 10).
Ideal Dependent Sources
Figure 10: Controlled or dependent sources
kix gvx
Controlled current sources
kvx+
- rix +-
Controlled voltage sources
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Determine vxin the circuit shown in Fig. 11(a)
Example 1
22
Fig.11a: Circuit for the example 1
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First the given network is properly labeled (Fig.11b)
Using KVL in loop I,
Using KCL at node X
Using KVL in loop II,
Solution
10 4 0xv v v
10
10 10
20 V
And, / 10 2 A
v
i v
104 10
4
5 5 3 A10
4 3 12 V
vi i
v
23
8 5 8 40 Vv
8 1060 0v v
10 4 20 12 8 Vxv v v
Fig.11(b): Labeled circuit
I
IIX
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Star and Delta Networks
Consider the circuit shown, which is not easily
amenable to series parallel circuit reductiontechniques.
A or Star network is a three-terminal three-
branch network with a common point as shown.
The resistance connected between any terminal
i(1, 2 or 3) and the common point in the Ynetwork is denotedRi.
A or Delta network is a three-terminal three-
branch network as shown.
The resistance connected between any two
terminals iandjin the network is denotedRij.
Star and Delta networks are commonly found inmany circuits and are basic configurations in 3-phase circuits.
24
1
1
32
2
1 3
R12 R23
R13
Y or Star
or Delta
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Delta Star Transformation
Every (Delta) network has an equivalent (Star)
network and vice versa.
If the two circuits shown are equivalent, then their
impedances should match under all circumstances.
If terminal 1 is open, then,
If terminal 2 is open,
And, if terminal 3 open,
Adding all three,
Then subtracting each from the total:
25
1
32
2
1 3
R12 R23
R13
231312
23131232
)(
RRR
RRRRR
231312
13231231 )(RRRRRRRR
231312
12231321
)(
RRR
RRRRR
231312
323123211312321
)(
RRR
RRRRRRRRR
,231312
13121
RRR
RRR
,
231312
23212
RRR
RRR
231312
32313
RRR
RRR
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1
32
Star Delta Transformation
Every Y (Star) network has an equivalent (Delta)
network.
Using to Y conversion relations:
We get:
Taking the ratios:
It should be noted that above conversion equations
are equally valid for AC circuits with complex
impedances.
26
2
1 3
R12 R23
R13
)()(
)(
231312
3123122
231312
231312312312133221
RRR
RRR
RRR
RRRRRRRRRRRR
231312
13121
RRR
RRR
,
231312
23212
RRR
RRR
231312
32313
RRR
RRR
,1
323223R
RRRRR ,2
131331R
RRRRR 3
212112 R
RRRRR
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Star Delta Transformation - Example
Example:
Find the current supplied by E, when
E = 10 V,
R1= 3 , R2= 10 , R3= 5 ,
RL
=10 , R4
= 2 , and R5
= 4 .
Ans. 1.25 A
27
Exercise:
Del Toro Problems: 1-10, 3-22, 3-27
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Network Techniques and Theorems
There are several systematic techniques and useful theorems which arebeneficially employed to solve network problems.
Nodal Analysis
Mesh Analysis
Superposition Theorem TheveninsTheorem
Nortons Theorem
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Nodal Analysis
To illustrate the basic mechanics of the technique, consider the three node
circuit shown in Fig.a. In this network there are three nodes.
A three node circuit should have two unknown voltages and two equations;
a 10-node circuit will have nine unknown voltages and nine equations;
an N-node circuit will need (N-1) voltages and (N-1) equations.
In the Fig. b, it is shown that the network has three unique nodes. One node isdesignated as a reference node(Fig.c) and it is the negative terminal of the
nodal voltages.
29
(a) (b)
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In the Fig. b, one node isdesignated as a reference node
(also in Fig. c) and it is the
negative terminal of the nodal
voltages.
Nodal Analysis
--
+ +
V1 V2
1 2
3(c)
30
As a general rule, a node having maximum number of branches is chosen
as the reference node. By doing so the number of equations defining the
network is reduced.
In Fig. c, the voltage of node 1 relative to the reference node is defined asV1and V2is defined as the voltage of node 2 with respect to the reference
node. The voltage between any other pair of nodes may be found in terms
of V1and V2.
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Nodal AnalysisGeneral Procedure
The node analysis is a general method and
can always be applied to any electrical
network. Consider the circuit shown in the
Fig.
Identify the goal of the problem: There are
four nodes in this network. The bottom mostnode is selected as the reference node and all
the other three nodes are labeled as shown in
Fig.
Collect the information: There are threeunknown voltages V1, V2and V3. All current
sources and resistors have designated values
which are marked on the schematic.
31
A 4 node network
Redrawn network
1 2
3
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Nodal AnalysisGeneral Procedure
Devise a plan: This problem is well suited for
nodal analysis and three independent KCLequations may be written.
Construct an appropriate set of equati ons:
There are three unknowns and three equations.
Solve for voltages.
1 31 2
2 32 12
3 3 2 3 1
8 3 at node 13 4
3 at node 23 7
1.4 at node 3
5 7 4
V VV V
V VV VV
V V V V V
32
1 2
3
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The Supernode
Consider the network shown in the fig. If
KCL is applied as in the previous example
then we will run into difficulty at nodes 2
and 3 because the current in the branch 23
cannot be expressed in terms of V23.
To overcome the dilemma, node 2, node 3together with the voltage source is
considered a supernodeand KCL is then
applied.
The above super node is shown as a region
enclosed by the broken lines. A supernode
may be formed covering any region of a
circuit.
33
V1 V2 V3
supernode
1 2
3
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Supernode Example
The super node is shown as a region
enclosed by the broken lines.
The system of equations are:
Then solve for the three unknown voltages.
1 31 2
3 1 32 12
2 3
at node 1
8 33 4
at supernode
3 1.43 4 5
the third equation is22
V VV V
V V VV VV
V V
34
V1 V2 V3
Supernode (nodes 2 & 3
1
2
3
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Mesh Analysis
The node analysis is a general method and can always be applied to anyelectrical network.
Another convenient technique to analyze the networks is mesh analysis.
This technique is not general and can be applied to only planar networks.
If it is possible to draw the diagram of the network on a plane surface in
such a way that no branch passes over or under any other branch, then the
network is said to be aplanar network.
If a network is planar, mesh analysis can be used to accomplish the
analysis. This concept involves the concept of a mesh current.
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Planar and Non Planar Networks
Fig: Planar and non planar networks
a. Planar network
b. Non-planar network
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Consider the two mesh circuit shown in
the Fig. We define a mesh currentas acurrent that flows only around the
perimeter of a mesh.
The left hand mesh has a current i1
flowing in a clockwise direction and a
mesh current of i2is established in theremaining mesh.
The system of equations for the network
in terms of mesh currents are as follows:
Solving the above two equations, the
mesh currents i1 and i2are obtained as
Mesh Analysis
1 1 2
2 1 2
6 3( ) 42, for mesh 13( ) 4 10, for mesh 2
i i ii i i
1 26 A, and 4 Ai i
37
Fig.: Mesh Analysis
i1 i2
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According to superposition theorem, in a linear network containing two or
more sources, the response in any element is equal to the algebraic sum ofthe responses caused by individual sources acting alone while the other
sources are non-operative.
This theorem is useful for analyzing networks that have large number of
independent sources as it makes it possible to consider the effects of eachsource separately.
Superposition theorem is applicable to any linear circuit having time varying
or time invariant elements.
The limitations of superposition theorem are
It is not applicable to the networks consisting of non linear elements like
transistors, diodes, etc., in general (unless linearized).
It is not applicable to the networks consisting of any dependent sources,
in general.
Superposition Theorem
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Superposition Theorem - Example
Compute the current in the 23 Ohm resistor using superposition theorem.
The circuit contains 2 independent sources
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I23a
Superposition Theorem - Solution
With 200V source acting alone
and the 20A current open
circuited:
23
27 (4 23)47 60.5
54
200 3.31 A60.5
273.31 1.65 A
54
eq
total
a
R
I
I
40
With 20A source acting alone and
the 200V source short circuited:
23
27 474 21.15
74
21.1520 9.58 A
21.15 23
eq
b
R
I
I23b
23 23 23Curent through the 23 is: 11.23 Aa bI I I
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Thevenins theorem states that any two-terminal linear network having anumber of sources and resistances can be replaced by a simple equivalent
circuit consisting of a single voltage source in series with a resistance.
The value of the voltage source is equal to the open circuit voltage across
the two terminals of the network.
The resistance is equal to the equivalent resistance measured between the
terminals with all the energy sources replaced by their internal
resistances.
Thevenins Theorem
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The steps involved in determining the Theveninsequivalent circuit are:
Temporarily remove the load resistance where the current is required
Find the open circuit voltage VOCacross the two terminals from where the
load resistance has been removed. This is known the Theveninsvoltage VTH.
Calculate the resistance of the whole network as seen from these two
terminals, after all voltage sources are replaced by short circuit and allcurrent sources are replaced by open circuit leaving internal resistance (if
any). This is called Theveninsresistance, RTH.
Replace the entire network by a single Theveninsvoltage source VTHand
resistance RTH.
Connect the resistance (RL), across which the current value is desired, back
to its terminals from where it was previously removed.
Finally, calculate the current flowing through RLusing the following
expression:
Procedure to Obtain Thevenins Equivalent Circuit
THL
TH L
VI
R R
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Nortons theorem states that any two-terminal linear network with
current sources, voltage sources and resistances can be replaced by anequivalent circuit consisting of a current source in parallel with a
resistance.
The value of the current source is equal to the short circuit current
between the two terminals of the network and the resistance is
equivalent resistance measured between the terminals of the network
with all the energy sources replace by their internal resistance.
Nortons Theorem
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The steps involved in obtaining the Nortons equivalent circuit are:
Temporarily remove the load resistance across the two terminals and
short circuit these terminals.
Calculate the short circuit current IN.
Calculate the resistance of the whole network as seen at these two
terminals, after all voltage sources are replaced by short circuit andcurrent sources are replaced by open circuit leaving internal
resistances (if any). This is Nortons resistance RN.
Replace the entire network by a single Nortons current source whose
short circuit current is INand parallel with Nortons resistance RN.
Connect the load resistance (RL) back to its terminals from where it
was previously removed.
Finally calculate the current flowing through RL.
Procedure to Obtain Nortons Equivalent Circuit
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Obtain the Thevenins and Nortons Equivalent Circuit for the followingnetwork:
Thevenins and Nortons Equivalent Circuits - Example
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With the terminals aand bopen, the two
voltage sources drive a clockwise currentthrough the 3 and 6 resistors
Since no current passes through the upper
right 3 resistor, the Thevenins voltage
can be taken from either active branch:
The equivalent resistance as seen from
terminals aand bis
The Thevenins equivalent circuits is:
Thevenins Equivalent Circuit
20 10 30A
3 6 9I
3020 3 10 V
9THV
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3 63 5
9eqR
Thevenins eq. circuit
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When a short circuit is applied to theterminals, current Iscresults from the two
sources. By superposition theorem, this
current is given by
The Nortons equivalent circuit is:
Nortons Equivalent Circuit
6 20
6 3 3 3 6 / 9
3 10 2 A
3 3 6 3 3 / 6
scI
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Nortons eq. circuit
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Circuit Components R, L, C
When a (time varying) voltage eis applied to a simple resistorR, the
current is given by Ohms law as:
If the voltage is applied to a simple inductor, the relation between eand iis
given by Faradays law as
When voltage eis applied to a simple capacitor the pertinent relationship is
(1)e
iR
or (2)
where, the differential operator /
di ee L e pLi i
dt pL
p d dt
(3)1/
de eC i Cpe i i
dt pC
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Operational Impedance
The use of the differential operator permits the differential equation to be
written as an algebraic expression, wherepLplays a role for inductance that
is the same asRfor resistance.
The inductor is said to posses an operational impedanceofpL.
From the analogy
the capacitor can be said to present to the forcing function ean operationalimpedance of 1/pC
The term operational impedance can be applied to single elements or to
several interconnected elements.
49
Since,e
ipL
Since,1 /
ei
pC
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Consider the network shown in Fig. 1. By KVL, the describing differential
equation for the circuit is:
In terms of the poperator, or the operational impedances, the expression
becomes:
Such representation can be very useful in many situations.
Fig.1: Circuit to illustrate equivalency between p operator
algebraic equation and differential equation
Circuit Differential Equations - Operational Impedance
1(4)
die Ri L idt
dt C
1
1( ) (5)
1
where, ( )
e Ri pLi ipC
e R pL i Z p ipC
Z p R pL pC
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There are situations when it is required to relate an electrical quantity in one
part of the circuit to an appropriate electrical quantity in another part of thecircuit.
In the network of Fig. 1, it may be required to express the ratio of voltage
appearing across the inductor to the source voltage.
If vLis used to denote the voltage developed across
the inductor, the desired result can then be written as
The expression (6) is commonly called
the transfer function. The transfer function relates two quantities that are
identified at different terminal pairs.
The transfer functions may be used to relate ratios of voltages, ratios of
currents, ratios of current to voltage, ratios of voltage to current provided that
the quantities are not identified at the same terminal pairs.
Circuit Equations using Operational Impedances
(6)1 /
Lv pL
e R pL pC
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General Formulation of Circuit Differential Equation
Consider the network shown in Fig. 2, where we like to relate voto e2.
Writing the node equation at node ausing operational impedances:
Then,
This implies that, in the form of differential equation, the voltage vois related
to e2by:
2
0 22
1 2 2 5 2
3 2 4 11 8a
p p pv v e
p p p
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Fig. 2: An RLC network
a2
22
01 2 / 2 1 2 1
(2 )(3 2 )
4 11 8
a a a
a
v v v e
p p
p pv e
p p
2 20 0 2 2
0 22 24 11 8 2 5 2 (7)
d v dv d e dev e
dt dt dt dt
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General Formulation of Circuit Differential Equation
Eq. 7 is often referred to as an equilibrium equation. It relates a linear
combinations of the response function and its derivatives to linear
combinations of the source function and its derivatives.
The operator version of eq. 7 is more generally written as:
Or,
2
0 222 5 2 (8)4 11 8p pv ep p
0 2( ) (9)
where,
( ) operational network function.
v G p e
G p
Fig. 2: An RLC network
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General Formulation of Circuit Differential Equation
For any network, the following generalization holds true
Eq. (10) is generally written as
( ) ( ) ( ) ( ) (11)D p y t N p f t
( ) ( )
( )( ) ( ) ( ) ( ) (10)
( )
( ) response function such as current or voltage in a particular part of the circuit
( )= total networ
response function network function applied source function
N py t G p f t f t
D p
where
y t
G p
k function
( )=numerator polynomial of network function G(p)
( )= denominator polynomial of the network function G(p)
( )= applied voltage source function
N p
D p
f t
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Write the expression for the operational impedance for each branch of the
network shown in Fig.3 and determine the expression for the driving pointimpedance appearing at the terminal a-d.
Example 1
a b c
d
Fig.3: Circuit for the example 1
1 1
2 2
2
1
1
Driving point impedance
Z
ab
bd
bcd
bd bcd ad ab
bd bcd
Z RpC
Z R pL
Z R pLpC
Z ZZ
Z Z
Solution 1
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Solution of Circuit Differential Equation
Consider the response function,
If f(t) is an applied source function, then y(t) is said to be a solution to the
homogeneous linear differential equation.
The completeor fullsolution will consist of two components:
1. The SteadyStateor the Particularor the Forcedsolution.
This component is primarily dependent on the source.
2. The Transientor the Generalor the Naturalsolution
This component is primarily dependent on the network or the system.
The complete solution will be the sum of the two solutions.
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( ) ( ) ( ) ( ) (11)D p y t N p f t
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The Steady State (Forced or Particular) Solution
Consider, the first part of the solution to the network equation
1. The solutiony(t) will exhibit the same nature as the inputf(t). For
example, iff(t)is a sinusoidal function, theny(t)will also be sinusoidal,
althoughy(t)will differ from the source function in amplitude and
phase, in general. If the source function is exponential, the solution willbe exponential. This is why this part of the solution is termed the
particular solution, - the form ofy(t) is particularized to the nature of
the source function.
2. y(t) will continue to exist in the circuit so long as the source function
exists. This is the reason whyf(t)is referred to as theforced solution.
3. y(t) is also referred to as thesteady state solutionbecause this is the
component which remains in the circuit after the transient terms disappear.
( ) ( ) ( ) ( ) (11)D p y t N p f t
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The response to constant sources
The response to a constant source is developed for the network shown in Fig.
4. It is required to find the battery current if(t) due to the source voltage E.
The general procedure to obtain the solution is:
Obtain the equilibrium equation by applyingcircuit theory to the configuration of circuitelements described, in terms of their
Operational impedances.
Put the resulting expression in the formof eq.11. Then examine the right side ofthis equation to determine the exact formneeded by the forced solution to qualify as
a solution to the equilibrium equation. Finally, solve for the unknown quantities.
To find the expression for the current if(t) in the circuit shown in Fig.4, it isrequired to find the impedance Zgd.
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Fig. 4: The network 1
a b c
g
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The response to constant sources
The operation impedance across the terminals g-d is:
The current if(t) is given by
The corresponding differential equation is
2
2
( )
2(3 2 )
4 11 82 1 (12)2 2 4 2
3 2
ab bcd gd bg
ab bcd
Z ZZ p Z
Z Z
pp
p p
p p pp
p
2
24 11 8 2 (14)
f f
f
d i dii E
dt dt
2
2
2 2
2 4 2( )
4 11 8
(4 11 8) ( ) (2 4 2) (13)
f
gd
f
E p pi t
Z p p
p p i t p p E
a b c
g
d
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The response to constant sources
Examination of the equilibrium equation (eq. 13) reveals that because there are
no derivative terms on the right side of the equation, the derivative terms of theresponse function must be identically equal to zero.
Hence, the expected form of the solution for if(t) is
Substituting the solution in eq. (15) into eq. (13) gives the forced or the steadystate solution.
The examination of the network given in Fig. 4 reveals that this result is
entirely expected. The current if(t) finds a closed path only in loopgbcdg. The
left hand part of the loop is open circuit in the steady state due to presence ofthe capacitor.
The voltage across the 2-H inductor is zero in steady state. Hence, the current
is just a d-c current of magnitude E/4.
0( ) (15)fi t I
0 (16)4
EI
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Fig. 5: Series R-L Circuit
The forced solution is the response which has settled down solely to the effects
of the source function. It is also known as thesteady state solution. The forced or the steady state solution always satisfies the defining differential
equation but in general it is not the complete solution over the entire time
domain.
To illustrate the point consider the R-L circuit shown in Fig. 5. In this network
it is desired to find the complete solution for the voltage vappearing across the
resistor for all time tafter the switch is closed.
The equation that relates vto the source voltageEis:
The forced or the steady state solution of eq. 18 is:
1(17)
1 ( / )
(18)
v R
E R pL p L R
L dvv E
R dt
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The Steady State Response of R-L Circuit
(19)fv E
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The Natural Response (Transient Solution)
Solution (19) satisfies eq. 18, however this solution does
not satisfy the circuit behavior in the period immediatelyfollowing the closing of the switch at time t=0+
At time t=0+the current is zero because of the presence of the inductor. Hencev, which is iR, is also zero. Hence, the solution in eq. 19 cannot be a completedescription at t=0+.
Therefore, in the period, t=0+, immediately after the switching of the sourcefunction, it needs to add a complementary functionto the forced solution.
This complementary function will be significant only immediately afterswitching but will disappear as steady state is reached. It is the purpose of thecomplementary function to provide a smooth transition from the initial state of
the response to the final state, in the presence of energy storing elements. The complementary function (natural response) is obtained by solving
equation 18 with no inputs,
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0 (20)L dv
vR dt
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The Natural Response (Transient Solution) of RL Circuit
The solution to the eq. 20 should satisfy that function, i.e, vand its derivative,
dv/dt, must be of the same form to make the left hand side equal to the righthand side.
The plausible solution for eq. 20 is
Substitution of vfrom eq. 21 into eq. 20 gives
Hence, the complementary solution becomes
It is clearly seen that this solution will have a value of K at t=0, but will become 0
when t.
(21)stv Ke
( / ) 1 0 (22)
/ ) (23)
stL R s Ke
s R L
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( / ) (24)R L tv Ke
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The Complete Response of RL Circuit
The complete solution of the original governing differential equation (18) is
The quantityKis found from the initial condition which requires that vto bezero at t=0+
Hence, the complete solution is
The nature of the complimentarySolution is shown in the figure.
It begins with an initial value ofE and exponentially decays to a value ofzero.
0 (24)E K K E
( / )(1 ) (25)R L tv E e
( / ) (25)R L tv E Ke
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The Complete (Transient+ Steady State) Solution
The behavior of the complete solution (eq. 25) is shown in Fig. 6.
Note that the total response now starts with a value of zero and
exponentially rises to the value ofE.
The rate at which this
transition takes place is
entirely dependent uponthe value of (R/L). WhenRis
large (orLis small) the
transition occurs quickly
because the transient term
dies out in little time.
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( / )(1 )R L tv E e
Fig. 6: Complete solution of voltage across the resistor
in RL circuit of Figure 5.
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The Response to Different Kinds of Source
Similar analyses can be conducted for
different types of inputs, say sinusoidal
source as shown in Fig.7.
These cases are not covered in this course.
Similarly, the behavior of various circuit
components can be investigated.
Homework: (RC Circuit)
Investigate the behavior of the voltage across the
resistor in a series RC circuit after switching a dc
source.
Fig.7: Network with sinusoidal source
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Thank you!
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Exercise:
Del Toro Problems: 3-23, 3-32, 3-33, 3-34