CH.8 Time Varying Field

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CHAPTER (8)
TIME VARYING ELECTRIC
AND
MAGNETIC FIELDS
47
AAST
Prof. Darwish
Faraday’s law:
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Due to the first experiment of Faraday, we can say that a
time-varying magnetic field produces an electromotive
force (emf) which may establish a current in a suitable
closed circuit. Faraday’s law is stated as
๐๐๐’Ž (๐’•)
๐’†๐’Ž๐’‡ = −
๐๐’•
๐๐ (๐’•)
[๐‘ฝ]
(๐Ÿ)
A non zero value of ๏ฟฝ ๐’Ž ๏ฟฝ may result from any of the
๐๐’•
following situations:
• A time-changing flux linking a stationary closed path.
• Relative motion between a steady flux and a closed
path.
• A combination of the two previous situations.
Note:
1- The minus sign is an indication that the emf is in
such a direction as to produce a current whose
flux, if added to the original flux, would reduce the
magnitude of the emf.
This statement that the induced voltage acts to
produce an opposing flux is known as Lenz’s law.
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2- For N – turns filamentary conductor closed path
๐๐๐’Ž (๐’•)
๐’†๐’Ž๐’‡ = − ๐‘ต
๐๐’•
(๐Ÿ)
48
AAST
Prof. Darwish
The emf is considered as the voltage about a specific
closed path, and it is defined as
๐๐๐’Ž
๏ฟฝ๏ฟฝ๏ฟฝ๏ฟฝโƒ—
๏ฟฝ
๏ฟฝโƒ—
๐’†. ๐’Ž. ๐’‡ = ๏ฟฝ ๐‘ฌ . ๐’…๐’ = −
(๐Ÿ‘)
๐๐’•
In electro-statics, equation (3) must lead to zero potential
difference about a closed path. In time varying fields, the line
integral leads to an emf or a potential difference.
Equation (3) can be written as
๏ฟฝ๏ฟฝ๏ฟฝ๏ฟฝโƒ— = −
๏ฟฝ๏ฟฝโƒ— . ๐’…๐’
๐’†. ๐’Ž. ๐’‡ = ๏ฟฝ ๐‘ฌ
๐๐๐’Ž
๐
๏ฟฝ๏ฟฝ๏ฟฝ๏ฟฝโƒ— (๐Ÿ’)
๏ฟฝ๏ฟฝโƒ— . ๐’…๐’”
= −
๏ฟฝ๐‘ฉ
๐๐’•
๐๐’•
In general, Faraday’s law manifests itself in either or
both a stationary circuit linked by a time varying
magnetic flux, such as a transformer, or the magnetic flux
may be static, but the circuit is moving relative to the flux
in such a way as to produce a time varying flux enclosed
by the circuit. A rotating machine generates an emf by
the latter mechanism.
๐Ÿ๐’”๐’• ๐‘ด๐’‚๐’™๐’˜๐’†๐’๐’′ ๐’” ๐’†๐’’๐’–๐’‚๐’•๐’Š๐’๐’
Applying Stock’s theorem on equation (4)
๏ฟฝ๏ฟฝ๏ฟฝ๏ฟฝโƒ— = ๏ฟฝ ๐›๐’™๐‘ฌ
๏ฟฝ๏ฟฝ๏ฟฝ๏ฟฝโƒ— = −
๏ฟฝ๏ฟฝโƒ— . ๐’…๐’
๏ฟฝ๏ฟฝโƒ— . ๐’…๐’”
๐’†. ๐’Ž. ๐’‡ = ๏ฟฝ ๐‘ฌ
๐
๏ฟฝ๏ฟฝ๏ฟฝ๏ฟฝโƒ—
๏ฟฝ๏ฟฝโƒ— . ๐’…๐’”
๏ฟฝ๐‘ฉ
๐๐’•
So, ๐Ÿ๐’”๐’• ๐‘ด๐’‚๐’™๐’˜๐’†๐’๐’′ ๐’” ๐’†๐’’๐’–๐’‚๐’•๐’Š๐’๐’ ๐’Š๐’ ๐’…๐’Š๐’‡๐’‡๐’†๐’“๐’†๐’๐’•๐’Š๐’‚๐’ ๐’‡๐’๐’“๐’Ž ๐’Š๐’”
๏ฟฝ๏ฟฝโƒ—
๐๐‘ฉ
๏ฟฝ๏ฟฝโƒ— = −
๐›๐’™๐‘ฌ
(๐Ÿ“)
๐๐’•
49
AAST
Prof. Darwish
And, ๐Ÿ๐’”๐’• ๐‘ด๐’‚๐’™๐’˜๐’†๐’๐’′ ๐’” ๐’†๐’’๐’–๐’‚๐’•๐’Š๐’๐’ ๐’Š๐’ ๐’Š๐’๐’•๐’†๐’ˆ๐’“๐’‚๐’ ๐’‡๐’๐’“๐’Ž ๐’Š๐’”
๏ฟฝ๏ฟฝโƒ— . ๏ฟฝ๏ฟฝ๏ฟฝ๏ฟฝโƒ—
๏ฟฝ๏ฟฝโƒ— . ๏ฟฝ๏ฟฝ๏ฟฝ๏ฟฝโƒ—
๏ฟฝ๐‘ฌ
๐’…๐’ = ๏ฟฝ ๐›๐’™๐‘ฌ
๐’…๐’” = −
๐
๏ฟฝ๏ฟฝโƒ— . ๏ฟฝ๏ฟฝ๏ฟฝ๏ฟฝโƒ—
๏ฟฝ๐‘ฉ
๐’…๐’”
๐๐’•
Displacement current density ๐‘ฑโƒ—๐’…
(๐Ÿ”)
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It is shown from ๐Ÿ๐’”๐’• ๐‘ด๐’‚๐’™๐’˜๐’†๐’๐’′ ๐’”๐’†๐’’๐’–๐’‚๐’•๐’Š๐’๐’ in differential
form (5)
๏ฟฝ๏ฟฝโƒ— = −
๐›๐’™๐‘ฌ
๏ฟฝ๏ฟฝโƒ—
๐๐‘ฉ
๐๐’•
that a time varying magnetic field produces an electric
๏ฟฝ๏ฟฝโƒ—. From the definition of the curl, the electric field
field ๐‘ฌ
๏ฟฝ๏ฟฝโƒ— has the special property of circulation; its line integral
๐‘ฌ
about a general closed path is not zero.
Now we will consider the time varying electric field.
From Curl law as it applies to steady magnetic fields,
where
๏ฟฝ๏ฟฝโƒ— = ๐‘ฑโƒ—๐’„
๐› ๐’™ ๏ฟฝ๐‘ฏ
(๐Ÿ•)
๐“๐š๐ค๐ข๐ง๐  ๐ญ๐ก๐ž ๐๐ข๐ฏ๐ž๐ซ๐ ๐ž๐ง๐œ๐ž ๐จ๐Ÿ ๐›๐จ๐ญ๐ก ๐ฌ๐ข๐๐ž๐ฌ ๐จ๐Ÿ ๐ž๐ช๐ฎ๐š๐ญ๐ข๐จ๐ง (๐Ÿ•),
๏ฟฝ๏ฟฝโƒ— = ๐› . ๐‘ฑโƒ—๐’„
๐› . ๐› ๐’™ ๏ฟฝ๐‘ฏ
(๐Ÿ–)
Mathematically, the left hand side of equation (8)
๏ฟฝ๏ฟฝ๏ฟฝโƒ— = ๐ŸŽ), while the right hand side of
equals zero (๐›. ๐› ๐’™ ๐‘ฏ
equation (8), from continuity equation (conservation
of charge) equals to
๐๐†๐’—
โƒ—
๐› . ๐‘ฑ๐’„ = −
(๐Ÿ—)
๐๐’•
AAST
Prof. Darwish
50
So, equation (8) becomes
๏ฟฝ๏ฟฝ๏ฟฝโƒ— = ๐› . ๐‘ฑโƒ—๐’„ = −
๐› .๐› ๐’™ ๐‘ฏ
๐๐†๐’—
๐๐’•
(๐Ÿ๐ŸŽ)
Since in equation (10), the L.H.S = 0, but the R.H.S ≠ 0, so
there is a missing term that appear in time varying field as that
๏ฟฝ๏ฟฝโƒ—
๐๐‘ฉ
appear in first Maxwell’s equation๏ฟฝ− ๏ฟฝ, in order to fulfill that
๐๐’•
R.H.S = L.H.S. This missing term that must be added to the
๐๐†
L.H.S is ๏ฟฝ+ ๐’— ๏ฟฝ. So
๐๐’•
๏ฟฝ๏ฟฝโƒ— = −
๐› . ๐› ๐’™ ๏ฟฝ๐‘ฏ
๐๐†๐’—
๐๐†๐’—
+
๐๐’•
๐๐’•
(๐Ÿ๐Ÿ)
๏ฟฝ๏ฟฝโƒ— = ๐†๐’— , equation (11)
Using the divergence law, ๐› . ๐ƒ
becomes
๏ฟฝ๏ฟฝโƒ— = −
๐› . ๐› ๐’™ ๏ฟฝ๐‘ฏ
So,
๐๐†๐’—
๐
๏ฟฝ๏ฟฝโƒ— ๏ฟฝ
+
๏ฟฝ๐› . ๐ƒ
๐๐’•
๐๐’•
๏ฟฝโƒ—
๐ ๏ฟฝ๐ƒ
๐๐†๐’—
๏ฟฝ๏ฟฝ๏ฟฝโƒ— −
๐› . ๏ฟฝ๐› ๐’™ ๐‘ฏ
๏ฟฝ= −
= ๐› . ๐‘ฑโƒ—๐’„
๐๐’•
๐๐’•
๏ฟฝโƒ—
๐ ๏ฟฝ๐ƒ
๏ฟฝ๏ฟฝ๏ฟฝโƒ— = ๐‘ฑโƒ—๐’„ +
๐›๐’™๐‘ฏ
๐๐’•
๏ฟฝ๏ฟฝโƒ— = ๐‘ฑโƒ—๐’„ + ๐‘ฑโƒ—๐’…
๐› ๐’™ ๏ฟฝ๐‘ฏ
Jc , Jd = 0
Jd , Jc = 0
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๐‘ฑโƒ—๐’„ ๐’Š๐’” ๐’•๐’‰๐’† ๐’„๐’๐’…๐’–๐’„๐’•๐’Š๐’๐’ ๐’„๐’–๐’“๐’“๐’†๐’๐’• ๐’…๐’†๐’๐’”๐’Š๐’•๐’š
๐‘ฑโƒ—๐’… ๐’Š๐’” ๐’•๐’‰๐’† ๐’…๐’Š๐’”๐’‘๐’๐’‚๐’„๐’†๐’Ž๐’†๐’๐’• ๐’„๐’–๐’“๐’“๐’†๐’๐’• ๐’…๐’†๐’๐’”๐’Š๐’•๐’š
AAST
Prof. Darwish
A
51
So, ๐Ÿ๐’๐’… ๐‘ด๐’‚๐’™๐’˜๐’†๐’๐’′ ๐’” ๐’†๐’’๐’–๐’‚๐’•๐’Š๐’๐’ ๐’Š๐’ ๐’…๐’Š๐’‡๐’‡๐’†๐’“๐’†๐’๐’•๐’Š๐’‚๐’ ๐’‡๐’๐’“๐’Ž ๐’Š๐’”
๏ฟฝ๏ฟฝ๏ฟฝโƒ— = ๐‘ฑโƒ—๐’„ + ๐‘ฑโƒ—๐’…
๐›๐’™๐‘ฏ
(๐Ÿ๐Ÿ)
And, ๐Ÿ๐’๐’… ๐‘ด๐’‚๐’™๐’˜๐’†๐’๐’′ ๐’” ๐’†๐’’๐’–๐’‚๐’•๐’Š๐’๐’ ๐’Š๐’ ๐’Š๐’๐’•๐’†๐’ˆ๐’“๐’‚๐’ ๐’‡๐’๐’“๐’Ž ๐’Š๐’”
๏ฟฝโƒ—
๐ ๏ฟฝ๐ƒ
๏ฟฝ๏ฟฝโƒ— . ๏ฟฝ๏ฟฝ๏ฟฝ๏ฟฝโƒ—
๏ฟฝ๏ฟฝโƒ— . ๏ฟฝ๏ฟฝ๏ฟฝ๏ฟฝโƒ—
๏ฟฝ ๏ฟฝ๐‘ฏ
๐’…๐’ = ๏ฟฝ ๐› ๐’™ ๏ฟฝ๐‘ฏ
๐’…๐’” = ๏ฟฝ
. ๏ฟฝ๏ฟฝ๏ฟฝ๏ฟฝโƒ—
๐’…๐’” + ๏ฟฝ ๐‘ฑโƒ—๐’„ . ๏ฟฝ๏ฟฝ๏ฟฝ๏ฟฝโƒ—
๐’…๐’” (๐Ÿ๐Ÿ‘)
๐๐’•
3rd Maxwell's equation:
PU
UP
rd
0
3
Maxwell's equation in Integral form
⋅
=
→
B
d
S
∫
Applying the divergence theorem
๏ฟฝโƒ— . ๏ฟฝ๏ฟฝ๏ฟฝ๏ฟฝโƒ—
๏ฟฝโƒ— ๐’…๐’— = ๐ŸŽ
๏ฟฝ ๏ฟฝ๐‘ฉ
๐’…๐’” = ๏ฟฝ ๐› . ๏ฟฝ๐‘ฉ
So, ๐Ÿ‘๐’“๐’… ๐‘ด๐’‚๐’™๐’˜๐’†๐’๐’′ ๐’” ๐’†๐’’๐’–๐’‚๐’•๐’Š๐’๐’ ๐’Š๐’ ๐’…๐’Š๐’‡๐’‡๐’†๐’“๐’†๐’๐’•๐’Š๐’‚๐’ ๐’‡๐’๐’“๐’Ž ๐’Š๐’”
๏ฟฝโƒ— = ๐ŸŽ
๐› . ๏ฟฝ๐‘ฉ
(๐Ÿ๐Ÿ’)
And, ๐Ÿ‘๐’“๐’… ๐‘ด๐’‚๐’™๐’˜๐’†๐’๐’′ ๐’” ๐’†๐’’๐’–๐’‚๐’•๐’Š๐’๐’ ๐’Š๐’ ๐’Š๐’๐’•๐’†๐’ˆ๐’“๐’‚๐’ ๐’‡๐’๐’“๐’Ž ๐’Š๐’”
๏ฟฝโƒ— . ๏ฟฝ๏ฟฝ๏ฟฝ๏ฟฝโƒ—
๏ฟฝโƒ— ๐’…๐’— = ๐ŸŽ
๏ฟฝ ๏ฟฝ๐‘ฉ
๐’…๐’” = ๏ฟฝ ๐› . ๏ฟฝ๐‘ฉ
(๐Ÿ๐Ÿ“)
52
AAST
Prof. Darwish
4th Maxwell’s equation:
PU
UP
Applying the divergence theorem on the electric flux
๏ฟฝ๏ฟฝโƒ—, we have
density ๐‘ซ
๏ฟฝโƒ— . ๏ฟฝ๏ฟฝ๏ฟฝ๏ฟฝโƒ—
๏ฟฝโƒ— ๐’…๐’— = ๏ฟฝ ๐†๐’— ๐’…๐’—
๏ฟฝ ๏ฟฝ๐‘ซ
๐’…๐’” = ๐‘ธ๐’†๐’ = ๏ฟฝ ๐› . ๏ฟฝ๐‘ซ
So, ๐Ÿ’๐’•๐’‰ ๐‘ด๐’‚๐’™๐’˜๐’†๐’๐’′ ๐’” ๐’†๐’’๐’–๐’‚๐’•๐’Š๐’๐’ ๐’Š๐’ ๐’…๐’Š๐’‡๐’‡๐’†๐’“๐’†๐’๐’•๐’Š๐’‚๐’ ๐’‡๐’๐’“๐’Ž ๐’Š๐’”
๏ฟฝ๏ฟฝโƒ— = ๐†๐’—
๐› .๐‘ซ
(๐Ÿ๐Ÿ”)
And, ๐Ÿ’๐’•๐’‰ ๐‘ด๐’‚๐’™๐’˜๐’†๐’๐’′ ๐’” ๐’†๐’’๐’–๐’‚๐’•๐’Š๐’๐’ ๐’Š๐’ ๐’Š๐’๐’•๐’†๐’ˆ๐’“๐’‚๐’ ๐’‡๐’๐’“๐’Ž ๐’Š๐’”
๏ฟฝโƒ— . ๏ฟฝ๏ฟฝ๏ฟฝ๏ฟฝโƒ—
๏ฟฝโƒ— ๐’…๐’— = ๏ฟฝ ๐†๐’— ๐’…๐’—
๏ฟฝ ๏ฟฝ๐‘ซ
๐’…๐’” = ๐‘ธ๐’†๐’ = ๏ฟฝ ๐› . ๏ฟฝ๐‘ซ
Summary:
(๐Ÿ๐Ÿ•)
U
Maxwell's equation
Differential form
๏ฟฝโƒ— = −
๐›๐’™๐‘ฌ
๏ฟฝ๏ฟฝโƒ—
๐๐‘ฉ
๐๐’•
Integral form
๏ฟฝ๏ฟฝโƒ— . ๏ฟฝ๏ฟฝ๏ฟฝ๏ฟฝโƒ—
๏ฟฝ ๏ฟฝ๐‘ฌโƒ— . ๏ฟฝ๏ฟฝ๏ฟฝ๏ฟฝโƒ—
๐’…๐’ = ๏ฟฝ ๐›๐’™๐‘ฌ
๐’…๐’” = −
๏ฟฝ๏ฟฝโƒ— . ๏ฟฝ๏ฟฝ๏ฟฝ๏ฟฝโƒ—
๏ฟฝ๏ฟฝโƒ— . ๏ฟฝ๏ฟฝ๏ฟฝ๏ฟฝโƒ—
๏ฟฝ ๏ฟฝ๐‘ฏ
๐’…๐’ = ๏ฟฝ ๐› ๐’™ ๏ฟฝ๐‘ฏ
๐’…๐’” = ๏ฟฝ
๏ฟฝ๏ฟฝโƒ— = ๐‘ฑโƒ—๐’„ + ๐‘ฑโƒ—๐’…
๐› ๐’™ ๏ฟฝ๐‘ฏ
๏ฟฝ๏ฟฝโƒ— = ๐†๐’—
๐› .๐‘ซ
๐
๏ฟฝโƒ— . ๏ฟฝ๏ฟฝ๏ฟฝ๏ฟฝโƒ—
๏ฟฝ ๏ฟฝ๐‘ฉ
๐’…๐’”
๐๐’•
๏ฟฝโƒ—
๐๐ƒ
. ๏ฟฝ๏ฟฝ๏ฟฝ๏ฟฝโƒ—
๐’…๐’” + ๏ฟฝ ๐‘ฑโƒ—๐’„ . ๏ฟฝ๏ฟฝ๏ฟฝ๏ฟฝโƒ—
๐’…๐’”
๐๐’•
๏ฟฝ๏ฟฝ๏ฟฝ๏ฟฝโƒ— = ๐‘ธ๐’†๐’ = ๏ฟฝ ๐› . ๐‘ซ
๏ฟฝ๏ฟฝโƒ— . ๐’…๐’”
๏ฟฝ๏ฟฝโƒ— ๐’…๐’— = ๏ฟฝ ๐†๐’— ๐’…๐’—
๏ฟฝ๐‘ซ
๏ฟฝ๏ฟฝโƒ— = ๐ŸŽ
๐› .๐‘ฉ
๏ฟฝโƒ— . ๏ฟฝ๏ฟฝ๏ฟฝ๏ฟฝโƒ—
๏ฟฝโƒ— ๐’…๐’— = ๐ŸŽ
๏ฟฝ ๏ฟฝ๐‘ฉ
๐’…๐’” = ๏ฟฝ ๐› . ๏ฟฝ๐‘ฉ
53
AAST
Prof. Darwish
Jd =
ε ∂E
∂D
= 0
∂t
∂t
∇ ⋅ Jc +
∂ρ v
= 0
∂t
Id = J
d
⋅A
54
AAST
Prof. Darwish
Example:
U
A coaxial cable of ε r = 4, the inner conductor radius = 1mm
and the outer conductor radius = 5mm. Find the
displacement current between the two conductors per meter
if the voltage difference equal 100 cos (12π.106t) volt.
R
R
P
P
Solution:
U
1- Using circuit concept
U
For a coaxial cable :
2πε
2π ∗ 8.85 ∗ 10 −12 * 4
=
C=
๏ฃซb๏ฃถ
๏ฃซ5๏ฃถ
ln๏ฃฌ ๏ฃท
ln๏ฃฌ ๏ฃท
๏ฃญa๏ฃธ
๏ฃญ1๏ฃธ
Ιd = C
1
5
dV
dt
dV
= 100 sin(12π ∗ 10 6 t ) ∗ 12π ∗ 10 6
dt
2π ∗ 8.85 ∗ 10−12 * 4
100 sin(12π ∗ 106 t ) ∗ 12π ∗ 106 A/m
Ιd =
๏ฃซ5๏ฃถ
ln๏ฃฌ ๏ฃท
๏ฃญ1๏ฃธ
2- Using electro-magnetic field concept
U
The displacement current density
๏ฟฝ๏ฟฝโƒ—
๐๐‘ซ
from ๐‘ฑโƒ—๐’… = , after determining
๐๐’•
Gauss’s law as follows:
๏ฟฝ๏ฟฝ๏ฟฝ๏ฟฝโƒ— = ๐‘ธ๐’†๐’
๏ฟฝโƒ— . ๐’…๐’”
1) โˆฎ ๏ฟฝ๐‘ซ
2) ๐’„๐’‰๐’๐’Š๐’„๐’† ๐’๐’‡ ๐‘ฎ๐’‚๐’–๐’”๐’”๐’Š๐’‚๐’ ๐’”๐’–๐’“๐’‡๐’‚๐’„๐’†
3) ๐‘ธ๐’†๐’ = ๐†๐’ ๐’
๏ฟฝ๏ฟฝ๏ฟฝ๏ฟฝโƒ— = ๐Ÿ๐…๐’“๐’„ ๐’ ๐‘ซ
๏ฟฝโƒ— . ๐’…๐’”
4) โˆฎ ๏ฟฝ๐‘ซ
5) ๐Ÿ๐…๐’“๐’„ ๐’ ๐‘ซ = ๐†๐’ ๐’
๐†
๏ฟฝโƒ— = ๐’‚
๏ฟฝ๐’“๐’„ ๐’ ๐‘ช๏ฟฝ ๐Ÿ
6) ๏ฟฝ๐‘ซ
๐Ÿ๐…๐’“
๐’Ž
AAST
๏ฟฝโƒ— = ๐’‚
๏ฟฝ ๐’“๐’„
7) ๏ฟฝ๐‘ฌ
๐’„
๐†๐’
๐Ÿ๐…๐œบ๐’ ๐œบ๐’“ ๐’“๐’„
๐‘ต๏ฟฝ
๐‘ช
Prof. Darwish
๐‘ฑโƒ—๐’… can be determined
๏ฟฝ๐‘ซ
๏ฟฝโƒ— by applying the
55
In order to determine ๐†๐’ in terms of the potential
difference V, the potential V is determined as
๐’‚
๐‘ฝ๐’‚๐’ƒ =
๏ฟฝ๏ฟฝ๏ฟฝ๏ฟฝโƒ—
๏ฟฝ๏ฟฝโƒ— . ๐’…๐’
๐‘ฝ๐’‚๐’ƒ = − ๏ฟฝ ๐‘ฌ
๐’ƒ
๐Ÿ
๐†๐’
๏ฟฝ ๐’“๐’„
− ∫๐Ÿ“ ๐’‚
๐Ÿ๐…๐œบ๐’ ๐œบ๐’“ ๐’“๐’„
๏ฟฝ๐’“๐’„ ๐’…๐’“๐’„
.๐’‚
๐†๐’
๐Ÿ๐ŸŽ๐ŸŽ ๐œ๐จ๐ฌ (๐Ÿ๐Ÿ๐…. ๐Ÿ๐ŸŽ ๐’•) =
๐’๐’ (๐Ÿ“)
๐Ÿ๐…๐œบ๐’ ๐œบ๐’“
๐Ÿ”
๐Ÿ๐ŸŽ๐ŸŽ ๐…๐œบ๐’ ๐œบ๐’“ ๐œ๐จ๐ฌ (๐Ÿ๐Ÿ๐…. ๐Ÿ๐ŸŽ๐Ÿ” ๐’•)
๐†๐’ =
๐’๐’ (๐Ÿ“)
So,
๏ฟฝ๏ฟฝโƒ— = ๐’‚
๏ฟฝ ๐’“๐’„
๐‘ซ
๐†๐’
๐Ÿ๐ŸŽ๐ŸŽ ๐…๐œบ๐’ ๐œบ๐’“ ๐’„๐’๐’” (๐Ÿ๐Ÿ๐…. ๐Ÿ๐ŸŽ๐Ÿ” ๐’•)
๏ฟฝ ๐’“๐’„
= ๐’‚
๐Ÿ๐…๐’“๐’„
๐Ÿ๐…๐’“๐’„ ๐’๐’ (๐Ÿ“)
๏ฟฝ๏ฟฝโƒ—
๐Ÿ๐ŸŽ๐ŸŽ ๐…๐œบ๐’ ๐œบ๐’“ ๏ฟฝ๐Ÿ๐Ÿ๐…. ๐Ÿ๐ŸŽ๐Ÿ” ๏ฟฝ๐’”๐’Š๐’ (๐Ÿ๐Ÿ๐…. ๐Ÿ๐ŸŽ๐Ÿ” ๐’•)
๐๐‘ซ
๏ฟฝ ๐’“๐’„
=−๐’‚
๐‘ฑโƒ—๐’… =
๐Ÿ๐…๐’“๐’„ ๐’๐’ (๐Ÿ“)
๐๐’•
๐’…๐’”
๐‘ฐ๐’… = ๏ฟฝ ๐‘ฑโƒ—๐’… . ๏ฟฝ๏ฟฝ๏ฟฝ๏ฟฝโƒ—
๐Ÿ๐…
๐‘ฐ๐’… = ๏ฟฝ
๐ŸŽ
๐’
๏ฟฝ ๐’“๐’„
๏ฟฝ −๐’‚
๐ŸŽ
๐Ÿ๐ŸŽ๐ŸŽ ๐…๐œบ๐’ ๐œบ๐’“ (๐Ÿ๐Ÿ๐…. ๐Ÿ๐ŸŽ๐Ÿ” )๐’”๐’Š๐’ (๐Ÿ๐Ÿ๐…. ๐Ÿ๐ŸŽ๐Ÿ” ๐’•)
๏ฟฝ ๐’“๐’„ ๐’“๐’„ ๐’…๐‹๐’…๐’›
.๐’‚
๐Ÿ๐…๐’“๐’„ ๐’๐’ (๐Ÿ“)
๐Ÿ๐ŸŽ๐ŸŽ ๐…๐œบ๐’ ๐œบ๐’“ (๐Ÿ๐Ÿ๐…. ๐Ÿ๐ŸŽ๐Ÿ” )๐’”๐’Š๐’ (๐Ÿ๐Ÿ๐…. ๐Ÿ๐ŸŽ๐Ÿ” ๐’•)
๐’
๐‘ฐ๐’… =
๐’๐’ (๐Ÿ“)
๐Ÿ๐ŸŽ๐ŸŽ ๐…๐œบ๐’ ๐œบ๐’“ (๐Ÿ๐Ÿ๐…. ๐Ÿ๐ŸŽ๐Ÿ” )๐’”๐’Š๐’ (๐Ÿ๐Ÿ๐…. ๐Ÿ๐ŸŽ๐Ÿ” ๐’•)
๐‘ฐ๐’…
=
๐‘จ/๐’Ž
๐’
๐’๐’ (๐Ÿ“)
56
AAST
Prof. Darwish
Inductance:
U
When dealing with time – varying current and thus time
– varying magnetic fields, the inductance of the inductor
as a circuit concept becomes quite important and is
defined as
I
I
N
๐‘ณ =
๐šฒ
๐‘ฐ
[๐‘ฏ]
φm
Where:
๐šฒ (lambda) is the total flux linkage of the inductors and I
is the current flowing in the inductor.
A flux linkage of one exists when 1 Wb of flux links one
turn of the inductor.
So, if all the flux link all the turns, the total flux linkage
is equal to
[๐–๐› ๐ญ๐ฎ๐ซ๐ง๐ฌ]
๐šฒ = ๐ ๐›™๐ฆ
Where, ๐›™๐ฆ is the total flux produced by the inductor
L is the self inductance
If the coil has N turns:
๐šฒ
๐ ๐›™๐ฆ
๐‘ณ = =
๐‘ฐ
๐‘ฐ
57
AAST
Prof. Darwish
Example:
U
Find the self inductance of the solenoid shown in figure.
Solution:
U
๐šฒ
๐ ๐›™๐ฆ
=
๐‘ฐ
๐‘ฐ
๏ฟฝ๏ฟฝ๏ฟฝ๏ฟฝโƒ— = ๐ ๐€ = ๐ ๏ฟฝ๐›‘๐š๐Ÿ ๏ฟฝ
๏ฟฝ๏ฟฝโƒ— . ๐๐ฌ
๐›™๐ฆ = โˆฌ ๐
๐‘ณ =
๏ฟฝ๏ฟฝโƒ— = ๐›๐จ ๐›๐ซ ๐‡
๏ฟฝ๏ฟฝโƒ—
๐
๏ฟฝ๏ฟฝโƒ— can be determined by
The magnetic field intensity ๐‡
applying Ampere’s circuital law as follows:
๏ฟฝ๏ฟฝ๏ฟฝโƒ— = ๐‘ฐ๐’†๐’
๏ฟฝ๏ฟฝโƒ— . ๐๐ฅ
(1) โˆฎ ๐‡
(2) ๐‘ช๐’‰๐’๐’Š๐’„๐’† ๐’๐’‡ ๐‘จ๐’Ž๐’‘๐’†๐’“๐’Š๐’‚๐’ ๐’๐’๐’๐’‘
(3) ๐‘ฐ๐’†๐’ = ๐‘ต ๐‘ฐ
๏ฟฝ๏ฟฝ๏ฟฝโƒ— = ๐‘ฏ ๐’
๏ฟฝ๏ฟฝโƒ— . ๐๐ฅ
(4) โˆฎ ๐‡
๏ฟฝ๏ฟฝโƒ— = ๐‘ต ๐‘ฐ ๐š๏ฟฝ๐ณ
(5) ๐‡
๐’
So,
๏ฟฝ๐
๏ฟฝโƒ— = ๐›๐จ ๐›๐ซ ๐‡
๏ฟฝ๏ฟฝโƒ— = ๐›๐จ ๐›๐ซ ๐‘ต ๐‘ฐ ๐š๏ฟฝ๐ณ
๐’
๐‘ต๐‘ฐ
๐›™๐ฆ = ๐ ๏ฟฝ๐›‘๐š ๏ฟฝ = ๐›๐จ ๐›๐ซ
๏ฟฝ๐›‘๐š๐Ÿ ๏ฟฝ
๐’
๐Ÿ
๐‘ณ =
๐šฒ
๐‘ฐ
=
๐ ๐›™๐ฆ
๐‘ฐ
= ๐› ๐จ ๐›๐ซ
๐‘ต๐Ÿ
๐’
๏ฟฝ๐›‘๐š๐Ÿ ๏ฟฝ
[๐‡]
58
AAST
Prof. Darwish
Example:
U
Find the self inductance of the torrid shown.
Solution:
๐šฒ
๐ ๐›™๐ฆ
๐‘ณ = =
๐‘ฐ
๐‘ฐ
๏ฟฝ๏ฟฝโƒ— can be
The magnetic field intensity ๐‡
determined by applying Ampere’s
circuital law as follows:
๏ฟฝ๏ฟฝ๏ฟฝโƒ— = ๐‘ฐ๐’†๐’
๏ฟฝ๏ฟฝโƒ— . ๐๐ฅ
(1) โˆฎ ๐‡
(2) ๐‘ช๐’‰๐’๐’Š๐’„๐’† ๐’๐’‡ ๐‘จ๐’Ž๐’‘๐’†๐’“๐’Š๐’‚๐’ ๐’๐’๐’๐’‘
(3) ๐‘ฐ๐’†๐’ = ๐‘ต ๐‘ฐ
๏ฟฝ๏ฟฝ๏ฟฝโƒ— = ๐‘ฏ ๐Ÿ๐…๐’“๐’„
๏ฟฝ๏ฟฝโƒ— . ๐๐ฅ
(4) โˆฎ ๐‡
๏ฟฝ๏ฟฝโƒ— = ๐‘ต ๐‘ฐ ๐š๏ฟฝ๐›—
(5) ๐‡
U
So,
๐Ÿ๐…๐’“๐’„
๏ฟฝ๐
๏ฟฝโƒ— = ๐›๐จ ๐›๐ซ ๐‡
๏ฟฝ๏ฟฝโƒ— = ๐›๐จ ๐›๐ซ
๐‘ต๐‘ฐ
๐Ÿ๐…๐’“๐’„
๐š๏ฟฝ๐›—
Average path radius ๐’“๐’„|๐’‚๐’—๐’†๐’“๐’‚๐’ˆ๐’† = ๐’ƒ =
๏ฟฝ๏ฟฝโƒ—๐’‚๐’— = ๐›™ = ๐š
๏ฟฝ๐›—
๐‘ฉ
๐ฆ
๐’‚+๐’„
๐Ÿ
๐›™๐ฆ = ๐๐š๐ฏ ๐€
๐œ−๐š ๐Ÿ
๐€ = ๐›‘๏ฟฝ
๏ฟฝ
๐Ÿ
๐‘ต๐‘ฐ
๐œ−๐š ๐Ÿ
๐›™๐ฆ = ๐›๐จ ๐›๐ซ
๐›‘๏ฟฝ
๏ฟฝ
๐Ÿ๐…๐’ƒ
๐Ÿ
๐‘ต ๐‘ฐ(๐œ − ๐š)๐Ÿ
๐›™๐ฆ = ๐›๐จ ๐›๐ซ
๐Ÿ’(๐œ + ๐š)
AAST
๐‘ต๐Ÿ (๐œ − ๐š)๐Ÿ
๐šฒ
๐ ๐›™๐ฆ
๐‘ณ = =
= ๐› ๐จ ๐›๐ซ
๐‘ฏ๐’†๐’๐’†๐’“๐’š
(
)
๐‘ฐ
๐Ÿ’ ๐œ+๐š
๐‘ฐ
Prof. Darwish
59
Example:
U
Find the self inductance per unit length of a T.L. (coaxial
cable).
Solution:
U
๐šฒ
๐ ๐›™๐ฆ
๐‘ณ = =
๐‘ฐ
๐‘ฐ
๐‘ต=๐Ÿ
I
I
a
b
L
๏ฟฝ๏ฟฝโƒ— can be determined by
The magnetic field intensity ๐‡
applying Ampere’s circuital law as follows:
๏ฟฝ๏ฟฝ๏ฟฝโƒ— = ๐‘ฐ๐’†๐’
๏ฟฝ๏ฟฝโƒ— . ๐๐ฅ
(1) โˆฎ ๐‡
(2) ๐‘ช๐’‰๐’๐’Š๐’„๐’† ๐’๐’‡ ๐‘จ๐’Ž๐’‘๐’†๐’“๐’Š๐’‚๐’ ๐’๐’๐’๐’‘
(3) ๐‘ฐ๐’†๐’ = ๐‘ฐ
๏ฟฝ๏ฟฝ๏ฟฝโƒ— = ๐‘ฏ ๐Ÿ๐…๐’“๐’„
๏ฟฝ๏ฟฝโƒ— . ๐๐ฅ
(4) โˆฎ ๐‡
๏ฟฝ๏ฟฝโƒ— = ๐‘ฐ ๐š๏ฟฝ๐›—
(5) ๐‡
๐Ÿ๐…๐’“๐’„
So,
๏ฟฝ๐
๏ฟฝโƒ— = ๐›๐จ ๐›๐ซ ๐‡
๏ฟฝ๏ฟฝโƒ— = ๐›๐จ ๐›๐ซ
๐‘ฐ
๐š๏ฟฝ๐›—
๐Ÿ๐…๐’“๐’„
๏ฟฝ๏ฟฝ๏ฟฝ๏ฟฝโƒ— = ∫๐ฅ ∫๐› ๐›๐จ ๐›๐ซ ๐‘ฐ ๐š๏ฟฝ๐›— . ๐š๏ฟฝ๐›— ๐๐’“๐’„ ๐’…๐’›
๏ฟฝ๏ฟฝโƒ— . ๐๐ฌ
๐›™๐ฆ = โˆฌ ๐
๐ŸŽ ๐š
๐Ÿ๐…๐’“
๐›™๐ฆ =
AAST
๐‘ณ =
๐šฒ
๐‘ฐ
๐›๐จ ๐›๐ซ ๐‘ฐ๐’
=
๐Ÿ๐…
๐›™๐ฆ
๐‘ฐ
๐ฅ๐ง(๐’“๐’„ )๐›๐š =
=
๐›๐จ ๐›๐ซ ๐’
๐Ÿ๐…
Prof. Darwish
๐›๐จ ๐›๐ซ ๐‘ฐ๐’
๐Ÿ๐…
๐›
๐ฅ๐ง ๏ฟฝ ๏ฟฝ
๐’‚
๐’„
๐›
๐ฅ๐ง ๏ฟฝ ๏ฟฝ
๐’‚
[๐‡]
60
Example:
๐‹
๐›๐จ ๐› ๐ซ
๐›
=
๐ฅ๐ง ๏ฟฝ ๏ฟฝ
๐’
๐Ÿ๐…
๐’‚
[๐‡/๐ฆ]
U
Find the inductance per meter for two parallel wires.
Solution:
U
I
d
a
I
๐šฒ
๐ ๐›™๐ฆ
๐‘ณ = =
๐‘ฐ
๐‘ฐ
๐‘ต=๐Ÿ
๏ฟฝ๏ฟฝโƒ— can be determined by
The magnetic field intensity ๐‡
applying Ampere’s circuital law as follows:
๏ฟฝ๏ฟฝ๏ฟฝโƒ— = ๐‘ฐ๐’†๐’
๏ฟฝ๏ฟฝโƒ— . ๐๐ฅ
(1) โˆฎ ๐‡
(2) ๐‘ช๐’‰๐’๐’Š๐’„๐’† ๐’๐’‡ ๐‘จ๐’Ž๐’‘๐’†๐’“๐’Š๐’‚๐’ ๐’๐’๐’๐’‘
(3) ๐‘ฐ๐’†๐’ = ๐‘ฐ
๏ฟฝ๏ฟฝ๏ฟฝโƒ— = ๐‘ฏ ๐Ÿ๐…๐’“๐’„
๏ฟฝ๏ฟฝโƒ— . ๐๐ฅ
(4) โˆฎ ๐‡
๏ฟฝ๏ฟฝโƒ— = ๐‘ฐ ๐š๏ฟฝ๐›—
(5) ๐‡
So,
๐Ÿ๐…๐’“๐’„
๏ฟฝ๐
๏ฟฝโƒ— = ๐›๐จ ๐›๐ซ ๐‡
๏ฟฝ๏ฟฝโƒ— = ๐›๐จ ๐›๐ซ
AAST
๐‘ฐ
๐Ÿ๐…๐’“๐’„
๐š๏ฟฝ๐›—
๏ฟฝ๏ฟฝ๏ฟฝ๏ฟฝโƒ— = ∫๐ฅ ∫๐−๐Ÿ๐š ๐›๐จ ๐›๐ซ ๐‘ฐ ๐š๏ฟฝ๐›— . ๐š๏ฟฝ๐›— ๐๐’“๐’„ ๐’…๐’›
๏ฟฝ๏ฟฝโƒ— . ๐๐ฌ
๐›™๐ฆ = โˆฌ ๐
๐ŸŽ ๐š
๐Ÿ๐…๐’“
Prof. Darwish
๐’„
61
๐›™๐ฆ =
๐›๐จ ๐›๐ซ ๐‘ฐ๐’
๐Ÿ๐…
๐ฅ๐ง(๐’“๐’„ )๐−๐Ÿ๐š
=
๐š
๐›๐จ ๐›๐ซ ๐‘ฐ๐’
๐Ÿ๐…
๐ฅ๐ง ๏ฟฝ
๐−๐Ÿ๐š
๐’‚
๐šฒ
๐›™๐ฆ
๐›๐จ ๐›๐ซ ๐’
๐ − ๐Ÿ๐š
๐‘ณ = =
=
๐ฅ๐ง ๏ฟฝ
๏ฟฝ
๐Ÿ๐…
๐‘ฐ
๐‘ฐ
๐’‚
๏ฟฝ
[๐‡]
Mutual inductance:
U
Mutual inductance exists between two magnetic circuits that
share a common flux linkage. So, the mutual inductance is due
to the influence of one circuit on another and vice versa.
๐‘ด๐Ÿ๐Ÿ =
๐‘ต๐Ÿ ๐›™๐ฆ๐Ÿ๐Ÿ
๐šฒ๐Ÿ๐Ÿ
=
๐‘ฐ๐Ÿ
๐‘ฐ๐Ÿ
Where, ๐šฒ๐Ÿ๐Ÿ is the linkage of circuit 2 produced by ๐‘ฐ๐Ÿ in circuit 1.
For a linear magnetic medium, it can be shown that ๐‘ด๐Ÿ๐Ÿ = ๐‘ด๐Ÿ๐Ÿ .
๐‘ด๐Ÿ๐Ÿ =
๐šฒ๐Ÿ๐Ÿ
๐‘ฐ๐Ÿ
=
๐‘ต๐Ÿ ๐›™๐ฆ๐Ÿ๐Ÿ
๐‘ฐ๐Ÿ
62
AAST
Prof. Darwish
Example:
U
Find M 12 .
R
R
Solution:
U
ψ 12
μ μ Ν I (c − a )
= 0 r 1 1
4(c + a )
N 2ψ 12
Μ 12 =
2
I1
μ μ Ν N I (c − a )
μ μ Ν N (c − a )
∴ M 12 = 0 r 1 2 1
= 0 r 1 2
4 I1 (c + a )
4(c + a )
2
2
63
AAST
Prof. Darwish
Magnetic Circuits:
U
Example:
U
≡
NI = Rψ m
R = Reluctance
= The impedance of magnetic material for flow of magnetic flux
R=
l
µ0 µ r S
l1
R1 =
→ l = magnetic path length , S = cross sectional area
µ 0 µ r S1
R2 =
R3 =
R4 =
,
l2
µ0 µr S2
,
l3
µ 0 µ r S3
,
l 41
µ0 µr S4
∴ψ m (R1 + R2 + R3 + R4 ) = ΝΙ
64
AAST
Prof. Darwish
∴ψ m =
ΝΙ
= Β⋅ Α = Β⋅S
R1 + R2 + R3 + R4
Example:
U
I
Rg =
lg
µ0 S2
∴ψ m (R1 + R2 + R3 + R4 + Rg ) = ΝΙ
ψm =
ΝΙ
= B.S
(R1 + R2 + R3 + R4 + Rg )
65
AAST
Prof. Darwish
Example:
U
≡
ψ m3 = ψ m1 + ψ m 2
Rt = Rg + R3 +
R1R2
R1 + R2
ψ m 3 ⋅ Rt = ΝΙ
R2
∴ψ m1 = ψ m3 .
R1 + R2
ψ m2
ψ m3 =
→
ΝΙ
Rt
,
R1
= ψ m3.
R1 + R2
66
AAST
Prof. Darwish
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