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Electromagnetic Fields Lecture-13: Static Magnetic Fields 3 Chadi Abou-Rjeily Department of Electrical and Computer Engineering Lebanese American University [email protected] March 30, 2017 Chadi Abou-Rjeily Electromagnetic Fields Lecture-13: Static Magnetic Fields 3 Inductance and Inductors: Definition (1) Consider two neighboring closed loops C1 and C2 bounding surfaces S1 and S2 respectively. ~ 1 will be If a current I1 flows in C1 , then a magnetic field B created. The flux that flows through S2 due to the current in C1 can be expressed as (flux from 1 → 2): Z ~ 1 .d~s2 Φ12 = B (Wb) S2 If C2 has N2 turns, the flux linkage from (1) to (2) is: Λ12 = N2 Φ12 Chadi Abou-Rjeily (Wb) Electromagnetic Fields Lecture-13: Static Magnetic Fields 3 Inductance and Inductors: Definition (2) The mutual inductance between loops C1 and C2 is defined as: Λ12 L12 = (H) I1 It can be proven that L12 = L21 . In other words: Z Z N2 ~ 1 .d~s2 = N1 ~ 2 .d~s1 B B I1 S2 I2 S1 The self inductance of loop C1 is defined as: Z Λ11 N1 ~ 1 .d~s1 L11 = = B I1 I1 S1 A conductor arranged in an appropriate shape to supply a certain amount of self inductance is called an inductor. Just as a capacitor can store electric energy, an inductor can store magnetic energy. For a linear medium, the inductances do not depend on the current in the circuit. Chadi Abou-Rjeily Electromagnetic Fields Lecture-13: Static Magnetic Fields 3 Inductance and Inductors: Example-1 (1) Example: Assume that N turns of a wire are tightly wound on a toroidal frame of rectangular cross section. Assuming that the permeability of the medium is µ0 , find the self inductance of the toroidal coil. Assume a current I in the wire. Because of the symmetry ~ is along the ~aφ direction and its of the problem, B magnitude is constant along a circular path. Apply Ampere’s law over a circular path with radius r (a < r < b). This path encircles a total current NI: I ~ ~l = µ0 NI B.d C Chadi Abou-Rjeily Electromagnetic Fields Lecture-13: Static Magnetic Fields 3 Inductance and Inductors: Example-1 (2) The last equation implies that: Z 2π Bφ~aφ r dφ~aφ = µ0 NI 0 ⇒ 2πrBφ = µ0 NI ~ = µ0 NI ~aφ ⇒ B 2πr The flux that flows through the cross section of the toroid is: Z ~ ~s Φ= B.d S Z µ0 NI ~aφ .(~aφ hdr ) = 2πr S Z µ0 NIh b dr µ0 NIh b = = ln 2π 2π a a r Chadi Abou-Rjeily Electromagnetic Fields Lecture-13: Static Magnetic Fields 3 Inductance and Inductors: Example-1 (3) The flux linkage is: Λ = NΦ = µ0 N 2 Ih b ln 2π a Finally, the self inductance (or simply inductance) is given by: Λ µ0 N 2 h b L= = ln I 2π a Chadi Abou-Rjeily Electromagnetic Fields Lecture-13: Static Magnetic Fields 3 Inductance and Inductors: Example-2 (1) Example: Find the inductance per unit length of a very long solenoid with air core having n turns per unit length. ~ For a current I in the wire, we have previously seen that B is parallel to the axis of the solenoid and has a constant magnitude given by: B = µ0 nI If S is the cross-sectional area of the solenoid, the flux linkage per unit length is: Λ = nΦ = n(BS) = µ0 n2 SI Therefore, the inductance per unit length is: L= Λ = µ0 n 2 S I Chadi Abou-Rjeily (H/m) Electromagnetic Fields Lecture-13: Static Magnetic Fields 3 Inductance and Inductors: Example-3 (1) Example: Two coils of N1 and N2 turns are wound concentrically on a straight cylindrical core of radius a and permeability µ. The windings have lengths l1 and l2 respectively. Find the mutual inductance between the coils. Assuming a current I1 in coil 1, from the previous example, ~ 1 is: we can deduce that the magnitude of B N1 B1 = µn1 I1 = µ I1 l1 For coil 1, n1 is the number of turns per unit length while N1 is the number of turns. Chadi Abou-Rjeily Electromagnetic Fields Lecture-13: Static Magnetic Fields 3 Inductance and Inductors: Example-3 (2) The flux of the magnetic field caused by coil 1 in coil 2 is given by: N1 Φ12 = µ (πa2 )I1 l1 Since the outer coil has N2 turns, the flux linkage between coil 1 and coil 2 is given by: Λ12 = N2 Φ12 = µ N1 N2 πa2 I1 l1 Therefore, the mutual inductance is: L12 = Λ12 µ = N1 N2 πa2 I1 l1 Chadi Abou-Rjeily (H) Electromagnetic Fields Lecture-13: Static Magnetic Fields 3 Inductance and Inductors: Example-4 (1) Example: Determine the mutual inductance between a conducting triangular loop and a very long straight wire as shown in the adjacent figure. Designate the triangular loop as circuit 1 and the long wire as circuit 2. Assuming a current I2 in the wire, then the magnetic flux density at a distance r from the wire is given by: ~ 2 = µ0 I2 ~aφ B 2πr Chadi Abou-Rjeily Electromagnetic Fields Lecture-13: Static Magnetic Fields 3 Inductance and Inductors: Example-4 (2) The flux linkage Λ21 = Φ21 is: Z ~ 2 .d~s1 B Λ21 = S1 where: d~s1 = zdr ~aφ h π i = [(d + b) − r ] tan dr ~aφ 3 √ = 3 [(d + b) − r ] dr ~aφ Consequently: √ 3µ0 I2 2π Z d+b 1 [(d + b) − r ] dr r d √ 3µ0 I2 b = (d + b) ln 1 + −b 2π d Λ21 = Chadi Abou-Rjeily Electromagnetic Fields Lecture-13: Static Magnetic Fields 3 Inductance and Inductors: Example-4 (3) Therefore, the mutual inductance is: Λ21 I √2 b 3µ0 = (d + b) ln 1 + −b 2π d L21 = (H) Note that the mutual inductance can be calculated from either Λ21 /I2 or Λ12 /I1 . However, it is difficult to calculate ~ 1 caused by a current I1 Λ12 since it is difficult to calculate B in the triangular loop everywhere. Chadi Abou-Rjeily Electromagnetic Fields Lecture-13: Static Magnetic Fields 3 Magnetic Energy: Definition (1) Consider a system of N loops carrying currents I1 , I2 , . . . , IN . The magnetic energy stored in this system is given by: N 1X Wm = Ik Φk 2 k =1 where Φk is the flux linkage through the k-th circuit: Φk = N X Ljk Ij j=1 For j 6= k , Ljk is the mutual inductance between circuits j and k . For j = k , Ljj is the self inductance of circuit j. Consequently, Wm can be expressed as: N Wm = N 1 XX Ljk Ij Ik 2 j=1 k =1 Chadi Abou-Rjeily Electromagnetic Fields Lecture-13: Static Magnetic Fields 3 Magnetic Energy: Definition (2) For a current I flowing in a single inductor with inductance L, the stored magnetic energy is: Wm = 1 2 LI 2 (J) In terms of the field quantities, Wm can be written as: Z 1 ~ Bdv ~ ′ Wm = H. 2 V′ V ′ is the volume in which the magnetic energy is stored. ~ = µH: ~ Given that for a linear medium B Z 1 B2 ′ Wm = dv 2 V′ µ Z 1 = µH 2 dv ′ 2 V′ Chadi Abou-Rjeily Electromagnetic Fields Lecture-13: Static Magnetic Fields 3 Magnetic Energy: Example (1) Example: Starting from the formula of the stored magnetic energy, determine the inductance per unit length of an air coaxial transmission line that has a solid inner conductor of radius a and a very thin outer conductor of inner radius b. Assume that a current I flows in the inner conductor and returns via the outer conductor in the opposite sense. ~ has only a Because of the cylindrical symmetry, B φ-component. Assuming that the current is uniformly distributed over the cross section of the inner conductor, then the magnitude of the current density is: I J= πa2 Apply Ampere’s law over a circular contour of radius r . Chadi Abou-Rjeily Electromagnetic Fields Lecture-13: Static Magnetic Fields 3 Magnetic Energy: Example (2) Inside the inner conductor (0 ≤ r ≤ a): I ~ 1 .d~l = µ0 I (πr 2 ) B πa2 C Z 2π r 2 ⇒ Bφ1~aφ r dφ~aφ = µ0 I a 0 r 2 ⇒ Bφ1 (2πr ) = µ0 I a ~ 1 = Bφ1~aφ = µ0 rI ~aφ ⇒ B 2πa2 The magnetic energy stored per unit length in the inner conductor is: Z 1 Wm1 = B 2 dv ′ 2µ0 V ′ φ1 Z a Z 1 µ0 I 2 a 3 µ0 I 2 2 = Bφ1 2πr dr = r dr = (J/m) 2µ0 0 16π 4πa4 0 Chadi Abou-Rjeily Electromagnetic Fields Lecture-13: Static Magnetic Fields 3 Magnetic Energy: Example (3) Between the inner and outer conductors (a ≤ r ≤ b): I ~ 2 .d~l = µ0 I B C ⇒ Bφ2 (2πr ) = µ0 I ~ 2 = Bφ2~aφ = µ0 I ~aφ ⇒ B 2πr The magnetic energy per unit length stored in the region between the inner and outer conductors is: Z 1 Wm2 = B 2 dv ′ 2µ0 V ′ φ2 Z b 1 = B 2 2πr dr 2µ0 a φ2 Z µ0 I 2 b 1 µ0 I 2 b = dr = ln (J/m) 4π a r 4π a Chadi Abou-Rjeily Electromagnetic Fields Lecture-13: Static Magnetic Fields 3 Magnetic Energy: Example (4) Consequently, the magnetic energy stored per unit length of the transmission line is: Wm = Wm1 + Wm2 µ0 I 2 1 b = + ln 4π 4 a On the other hand: 1 2 LI 2 Comparing the above expressions results in: Wm = L= µ0 µ0 b + ln 8π 2π a Chadi Abou-Rjeily (H/m) Electromagnetic Fields Lecture-13: Static Magnetic Fields 3 Magnetic Forces and Torques (1) A charge q moving with a velocity ~u in a magnetic field with ~ will experience a magnetic force F ~ m given flux density B by: ~ m = q~u × B ~ F (N) Consider a closed circuit of contour C that carries a current ~ The magnetic force I in the presence of a magnetic field B. on an element d~l of the circuit can be written as: ~ ~ m = q~u × B ~ = (Idt) dl × B ~ dF dt ~ = Id~l × B Consequently, the magnetic force on the complete circuit is: I ~ ~ Fm = I d~l × B (N) C Chadi Abou-Rjeily Electromagnetic Fields Lecture-13: Static Magnetic Fields 3 Magnetic Forces and Torques (2) Consider the case of two circuits C1 and C2 carrying currents I1 and I2 respectively. ~ 21 on C1 resulting from the magnetic field The force F caused by the current I2 in C2 is: I ~ ~ 21 F21 = I1 d~l1 × B C1 ~ 21 is caused by C2 . From Biot-Savart law: where B I d~l2 × ~aR21 µ0 I2 ~ B21 = 2 4π C2 R21 The combination of the above equations results in Ampere’s law of forces: I I d~l1 × d~l2 × ~a R21 ~ 21 = µ0 I1 I2 F 2 4π R21 C1 C2 Chadi Abou-Rjeily Electromagnetic Fields Lecture-13: Static Magnetic Fields 3 Magnetic Forces and Torques (3) ~ 12 on circuit C2 in From the previous equation, the force F the presence of the magnetic field set up by the current I1 in C1 takes the following form: I I d~l2 × d~l1 × ~a R 12 ~ 12 = µ0 I2 I1 F 2 4π R12 C2 C1 Newton’s third law governing the forces of action and reaction holds. It can be proven that: ~ 12 = −F ~ 21 F even though: d~l1 × d~l2 × ~aR21 6= −d~l2 × d~l1 × ~aR12 . Chadi Abou-Rjeily Electromagnetic Fields Lecture-13: Static Magnetic Fields 3 Magnetic Forces and Torques (4) Example: Determine the force per unit length between two infinitely long parallel conducting wires carrying currents I1 and I2 in the same direction. The wires are separated by a distance d . Let the wires be in the yz-plane and parallel to the z-axis. By applying Ampere’s circuital law, we can directly deduce ~ 12 at wire 2 set up by the that the magnetic flux density B current I1 in wire 1 is: ~ 12 = µ0 I1 (−~ax ) B 2πd Chadi Abou-Rjeily Electromagnetic Fields Lecture-13: Static Magnetic Fields 3 Magnetic Forces and Torques (5) Consequently: ~ 12 = I2 d~l2 × B ~ 12 dF µ0 I1 I2 = (dz~az ) × (−~ax ) 2πd µ0 I1 I2 =− dz~ay 2πd Therefore, the force per unit length of wire 2 is: ~ ~ ′ = dF12 = − µ0 I1 I2 ~ay F 12 dz 2πd In the same way: ~ 21 = I1 d~l1 × B ~ 21 = I1 (dz~az ) × dF ⇒ µ0 I2 ~ax 2πd ~ ~′ ~ ′ = dF21 = µ0 I1 I2 ~ay = −F F 21 12 dz 2πd Chadi Abou-Rjeily Electromagnetic Fields Lecture-13: Static Magnetic Fields 3 Magnetic Forces and Torques (6) Consider a circular loop of radius b and carrying a current I ~ in a uniform magnetic field of flux density B. ~ B can be resolved into two components: ~ =B ~⊥ + B ~k B ~ ⊥ is perpendicular to the plane of the loop. B ~ k is parallel to the plane of the loop. B ~ ⊥ tends to expand the loop (or contract it if the direction B ~ ⊥ exerts no net force to move the loop. of I is reversed). B Chadi Abou-Rjeily Electromagnetic Fields Lecture-13: Static Magnetic Fields 3 Magnetic Forces and Torques (7) ~ k produces a force dF ~ 1 on element d~l1 and a force B ~ 2 = −dF ~ 1 on the symmetrically located element d~l2 . dF ~ 1 is out from the paper while that of dF ~2 The direction of dF is into the paper. ~ k is zero. The net force on the entire loop caused by B However, a torque exists on the loop. This torque tends to rotate the loop about the x-axis in such a way as to align ~ k field. the magnetic field due to I with the external B ~ 1 and dF ~ 2 is: The differential torque produced by dF ~ = [(dF )2b sin φ] ~ax dT h i ~ k 2b sin φ ~ax = Id~l1 × B = IdlBk sin φ 2b sin φ ~ax h i = 2Ib 2 Bk sin2 φdφ ~ax ~ 1 | = |dF ~ 2 | and dl = |d~l1 | = |d~l2 |. where dF = |dF Chadi Abou-Rjeily Electromagnetic Fields Lecture-13: Static Magnetic Fields 3 Magnetic Forces and Torques (8) The total torque acting on the loop is: Z Z π 2 2 ~ ~ T = dT = 2Ib Bk sin φdφ ~ax 0 h i = I πb 2 Bk ~ax On the other hand, the magnetic dipole moment of the loop is given by: ~ = I πb 2 ~an m ~an is the unit vector normal to the loop (its direction verifies the right hand rule). ~ can be written ~ , the torque T Based on the expression of m as: ~ =m ~ ~ ×B T (N.m) ~ was used instead of B ~ k because: Note that B ~ ~ ~ ~ ⊥. ~ × (B⊥ + Bk ) = m ~ × Bk since m ~ is parallel to B m Chadi Abou-Rjeily Electromagnetic Fields Lecture-13: Static Magnetic Fields 3 Magnetic Forces and Torques (9) ~ can be generalized to any The previous expression of T planar loop of any shape placed in a uniform magnetic field: ~ =m ~ ~ ×B T (N.m) ~ = IS~an where S is the cross-sectional area of the loop, I m is the current carried by the loop and ~an is the unit normal vector. Chadi Abou-Rjeily Electromagnetic Fields Lecture-13: Static Magnetic Fields 3 Magnetic Forces and Torques (10) Example: A rectangular loop in the xy-plane with sides b1 and b2 carrying a current I lies in a uniform magnetic field ~ = Bx ~ax + By ~ay + Bz ~az . Determine the B force and the torque on the loop. ~ into its perpendicular and parallel components: Resolve B ~ ⊥ = Bz ~az B ~ k = Bx ~ax + By ~ay B Chadi Abou-Rjeily Electromagnetic Fields Lecture-13: Static Magnetic Fields 3 Magnetic Forces and Torques (11) ~ ⊥ is given by: The force on side 1 due to B Z ~ ⊥1 = I d~l × B ~⊥ F Z b1 /2 =I (dx ~ax ) × (Bz ~az ) = −Ib1 Bz ~ay −b1 /2 ~ ⊥ is: The force on side 3 due to B ~ ⊥3 = −F ~ ⊥1 = Ib1 Bz ~ay F ~ ⊥ is: In the same way, the force on side 2 due to B Z −b2 /2 ~ F⊥2 = I (dy ~ay ) × (Bz ~az ) = −Ib2 Bz ~ax b2 /2 ~ ⊥ is: The force on side 4 due to B ~ ⊥4 = −F ~ ⊥2 = Ib2 Bz ~ax F Chadi Abou-Rjeily Electromagnetic Fields Lecture-13: Static Magnetic Fields 3 Magnetic Forces and Torques (12) ~ ⊥1 , F ~ ⊥2 , F ~ ⊥3 and F ~ ⊥4 are all directed toward the Note that F center of the loop. The sum of these contracting forces is zero: ~ ⊥2 + F ~ ⊥3 + F ~ ⊥4 = 0 ~ ⊥1 + F F The above forces produce no torque. Chadi Abou-Rjeily Electromagnetic Fields Lecture-13: Static Magnetic Fields 3 Magnetic Forces and Torques (13) ~ k on side 1 is: The force produced by B ~ k1 = I(b1~ax ) × (Bx ~ax + By ~ay ) F = Ib1 By ~az ~ k on side 3 is: The force produced by B ~ k3 = −F ~ k1 = −Ib1 By ~az F ~ k on side 2 is: The force produced by B ~ k2 = I(−b2~ay ) × (Bx ~ax + By ~ay ) F = Ib2 Bx ~az ~ k on side 4 is: The force produced by B ~ k4 = −F ~ k2 = −Ib2 Bx ~az F Chadi Abou-Rjeily Electromagnetic Fields Lecture-13: Static Magnetic Fields 3 Magnetic Forces and Torques (14) Again, the net force on the loop is zero. However, the above four forces result in a torque. ~ 13 due to forces F ~ k1 and F ~ k3 is: The torque T ~ 13 = Ib1 b2 By ~ax T ~ 24 due to forces F ~ k2 and F ~ k4 is: The torque T ~ 24 = −Ib1 b2 Bx ~ay T The total torque on the loop is then: ~ =T ~ 13 + T ~ 24 = Ib1 b2 (By ~ax − Bx ~ay ) T ~ from: Note that it was possible to calculate T ~ =m ~ ~ ×B T = (−Ib1 b2~az ) × (Bx ~ax + By ~ay + Bz ~az ) = Ib1 b2 (By ~ax − Bx ~ay ) Chadi Abou-Rjeily Electromagnetic Fields Lecture-13: Static Magnetic Fields 3