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UIUC Physics 436 EM Fields & Sources II Fall Semester, 2011 Lect. Notes 10.5 Prof. Steven Errede © Professor Steven Errede, Department of Physics, University of Illinois at Urbana-Champaign, Illinois 2005-2011. All Rights Reserved. 1 LECTURE NOTES 10.5 EM Standing Waves in Resonant Cavities One can create a resonant cavity for EM waves by taking a waveguide (of arbitrary shape) and closing/capping off the two open ends of the waveguide. Standing EM waves exist in (excited) resonant cavity (= linear superposition of two counter- propagating traveling EM waves of same frequency). Analogous to standing acoustical/sound waves in an acoustical enclosure. Rectangular resonant cavity – use Cartesian coordinates Cylindrical resonant cavity – use cylindrical coordinates to solve the EM wave eqn. Spherical resonant cavity – use spherical coordinates A.) Rectangular Resonant Cavity ( L W H a b d × × = × × ) with perfectly conducting walls (i.e. no dissipation/energy loss mechanisms present), with 0 x a , 0 y b , 0 z d . n.b. Again, by convention: a > b > d. Since we have rectangular symmetry, we use Cartesian coordinates - seek monochromatic EM wave solutions of the general form: ( ) ( ) ( ) ( ) , ,, , , , ,, , , i t o i t o Exyzt E xyze B xyzt B xyze ω ω = = G G G G Maxwell’s Equations (inside the rectangular resonant cavity – away from the walls): (1) Gauss’ Law : (2) No Monopoles : 0 E = G G i 0 o E = G G i 0 B = G G i 0 o B = G G i (3) Faraday’s Law : (4) Ampere’s Law : B E t ∇× =− G G G o o E i B ω ∇× = G G G 2 1 E B c t ∇× = G G G 2 o o B i E c ω ∇× =− G G Take the curl of (3): = 0 {Gauss’ Law} ( ) ( ) ( ) 2 2 o o o o o E i B E E i B E c ω ω ω ∇× ∇× = ∇× =∇× ∇ −∇ = ∇× = G G G G G G G G G G G G i {using (4) Ampere’s Law} 2 2 2 2 2 2 ox ox oy oy oz oz E E c E E c E E c ω ω ω =− =− =− G G G ( ) ( ) ( ) ( ) , , , , i.e. each is a fcn , , , , ox ox oy oy oz oz E E xyz E E xyz xyz E E xyz = = = Subject to the boundary conditions || 0 E = and 0 B = at all inner surfaces.
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Page 1: P436_Lect_10p5

UIUC Physics 436 EM Fields & Sources II Fall Semester, 2011 Lect. Notes 10.5 Prof. Steven Errede

© Professor Steven Errede, Department of Physics, University of Illinois at Urbana-Champaign, Illinois 2005-2011. All Rights Reserved.

1

LECTURE NOTES 10.5

EM Standing Waves in Resonant Cavities

• One can create a resonant cavity for EM waves by taking a waveguide (of arbitrary shape) and closing/capping off the two open ends of the waveguide.

• Standing EM waves exist in (excited) resonant cavity (= linear superposition of two counter-propagating traveling EM waves of same frequency).

• Analogous to standing acoustical/sound waves in an acoustical enclosure. • Rectangular resonant cavity – use Cartesian coordinates • Cylindrical resonant cavity – use cylindrical coordinates to solve the EM wave eqn. • Spherical resonant cavity – use spherical coordinates

A.) Rectangular Resonant Cavity ( L W H a b d× × = × × ) with perfectly conducting walls (i.e. no dissipation/energy loss mechanisms present), with 0 x a≤ ≤ , 0 y b≤ ≤ , 0 z d≤ ≤ . n.b. Again, by convention: a > b > d.

Since we have rectangular symmetry, we use Cartesian coordinates - seek monochromatic EM wave solutions of the general form:

( ) ( )( ) ( )

, , , , ,

, , , , ,

i to

i to

E x y z t E x y z e

B x y z t B x y z e

ω

ω

=

=

Maxwell’s Equations (inside the rectangular resonant cavity – away from the walls): (1) Gauss’ Law: (2) No Monopoles:

0E∇ =i ⇒ 0oE∇ =i 0B∇ =i ⇒ 0oB∇ =i

(3) Faraday’s Law: (4) Ampere’s Law:

BEt

∂∇× = −

∂ ⇒ o oE i Bω∇× = 2

1 EBc t

∂∇× =

∂ ⇒ 2o oB i E

∇× = − Take the curl of (3): = 0 {Gauss’ Law}

( ) ( ) ( )2

2o o o o oE i B E E i B E

cωω ω ⎛ ⎞∇× ∇× = ∇× = ∇× ∇ −∇ = ∇× = ⎜ ⎟⎝ ⎠

i {using (4) Ampere’s Law}

22

22

22

ox ox

oy oy

oz oz

E Ec

E Ec

E Ec

ω

ω

ω

⎛ ⎞∇ = −⎜ ⎟⎝ ⎠

⎛ ⎞∇ = −⎜ ⎟⎝ ⎠

⎛ ⎞∇ = −⎜ ⎟⎝ ⎠

( )( )( )

( ), ,

, , i.e. each is a fcn , ,

, ,

ox ox

oy oy

oz oz

E E x y z

E E x y z x y z

E E x y z

⎧ ⎫=⎪ ⎪⎪ ⎪=⎨ ⎬⎪ ⎪

=⎪ ⎪⎩ ⎭

Subject to the boundary conditions

|| 0E = and 0B⊥ = at all inner surfaces.

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UIUC Physics 436 EM Fields & Sources II Fall Semester, 2011 Lect. Notes 10.5 Prof. Steven Errede

© Professor Steven Errede, Department of Physics, University of Illinois at Urbana-Champaign, Illinois 2005-2011. All Rights Reserved.

2

For each component { } ( ), , of , ,ox y z E x y z we try product solutions and then use the separation of variables technique:

( ) ( ) ( ) ( ), ,io i i iE x y z X x Y y Z z≡ for ( )

22 , ,

i io oE x y z Ecω⎛ ⎞∇ = −⎜ ⎟⎝ ⎠

where subscript , ,i x y z= .

( ) ( ) ( ) ( ) ( ) ( ) ( ) ( ) ( ) ( ) ( ) ( )22 2 2

2 2 2i i i

i i i i i i i i i

X x Y y Z z cY y Z z X x Z z X x Y y X x Y y Z zx y z c

ω∂ ∂ ∂ ⎛ ⎞+ + = −⎜ ⎟∂ ∂ ∂ ⎝ ⎠

Divide both sides by ( ) ( ) ( )i i iX x Y y Z z :

The wave equation becomes: ( )

( )

( )

( )( )

( )

( )( )

( )

22 2 2

2 2 2

only only only

1 1 1i i i

i i i

fcn x fcn y fcn z

X x Y y Z zX x x Y y y Z z z c

ω

= =

∂ ∂ ∂ ⎛ ⎞+ + = −⎜ ⎟∂ ∂ ∂ ⎝ ⎠

This equation must hold/be true for arbitrary (x, y, z) pts. interior to resonant cavity 000

x ay bz d

≤ ≤⎧ ⎫⎪ ⎪≤ ≤⎨ ⎬⎪ ⎪≤ ≤⎩ ⎭

This can only be true if:

( )( )2

22

1 constantix

i

X xk

X x x∂

= − =∂

⇒ ( ) ( )

22

2 0ix i

X xk X x

x∂

+ =∂

( )

( )22

2

1 constantiy

i

Y yk

Y y y∂

= − =∂

⇒ ( ) ( )

22

2 0iy i

Y yk Y y

y∂

+ =∂

( )

( )22

2

1 constantiz

i

Z zk

Z z z∂

= − =∂

⇒ ( ) ( )

22

2 0iz i

Z zk Z z

z∂

+ =∂

with: 2

2 2 2 2x y zk k k k

cω⎛ ⎞≡ + + = ⎜ ⎟⎝ ⎠

⇐ characteristic equation

General solution(s) are of the form: ( ), , :i x y z=

( ) ( ) ( ) ( ) ( ) ( ) ( ), , cos sin cos sin cos sinio i x i x i y i y i z i zE x y z A k x B k x C k y D k y E k z F k z⎡ ⎤= + × + × +⎡ ⎤ ⎡ ⎤⎣ ⎦ ⎣ ⎦⎣ ⎦

n.b. In general, , and x y zk k k should each have subscript , , ,i x y z= but we will shortly find out that

ixk = same for all , , , iyi x y z k= = same for all , , ,i x y z= and

izk = same for all , ,i x y z= .

n.b. We want oscillatory

(not damped) solutions !!!

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UIUC Physics 436 EM Fields & Sources II Fall Semester, 2011 Lect. Notes 10.5 Prof. Steven Errede

© Professor Steven Errede, Department of Physics, University of Illinois at Urbana-Champaign, Illinois 2005-2011. All Rights Reserved.

3

Boundary Conditions: || 0E = @ boundaries and 0B⊥ = @ boundaries:

0, 0 at

0, ox

y y bE

z z d= =⎧ ⎫

= ⎨ ⎬= =⎩ ⎭ ⇒ coefficients

0

0x

x

E

C

⎧ =⎪⎨

=⎪⎩ and

, 1, 2,3,....

, 1, 2,3,....y

z

k n b n

k d

π

π

= =⎧ ⎫⎨ ⎬

= =⎩ ⎭

0, 0 at

0, oy

x x aE

z z d= =⎧ ⎫

= ⎨ ⎬= =⎩ ⎭ ⇒ coefficients

0

0y

y

A

E

⎧ =⎪⎨

=⎪⎩ and

, 1, 2,3,...., 1, 2,3,....

x

z

k m b mk d

ππ

= =⎧ ⎫⎨ ⎬= =⎩ ⎭

0, 0 at

0, oz

x x aE

y y b= =⎧ ⎫

= ⎨ ⎬= =⎩ ⎭ ⇒ coefficients

0

0z

z

A

C

⎧ =⎪⎨

=⎪⎩ and

, 1, 2,3,...., 1, 2,3,....

x

y

k m a mk n d n

ππ

= =⎧ ⎫⎪ ⎪⎨ ⎬= =⎪ ⎪⎩ ⎭

n.b. m = 0, and/or n = 0 and/or 0= are not allowed, otherwise ( ), , 0ioE x y z ≡ (trivial solution).

Thus we have (absorbing constants/coefficients, & dropping x,y,z subscripts on coefficients):

( ) ( ) ( ) ( ) ( )

( ) ( ) ( ) ( ) ( ) ( )

( ) ( ) ( ) ( ) ( )

, , cos sin sin sin

, , sin sin cos sin sin

, , sin sin cos sin

ox x x y z

oy x y y y z

ox x y z z

E x y z A k x B k x k y k z

E x y z k x k y C k y D k y k z

E x y z k x k y E k z F k z

⎡ ⎤= +⎣ ⎦⎡ ⎤= +⎣ ⎦⎡ ⎤= +⎣ ⎦

But (1) Gauss’ Law: 0E∇ =i ⇒ 0oyox ozEE Ex y z

∂∂ ∂+ + =

∂ ∂ ∂

Thus:

( ) ( ) ( ) ( )

( ) ( ) ( ) ( )

( ) ( ) ( ) ( )

sin cos sin sin

sin sin cos sin

sin sin sin cos 0

x x x y z

y x y y z

z x y z z

k A k x B k x k y k z

k k x C k y D k y k z

k k x k y E k z F k z

⎡ ⎤− +⎣ ⎦⎡ ⎤+ − +⎣ ⎦

⎡ ⎤+ − + =⎣ ⎦

This equation must be satisfied for any/all points inside rectangular cavity resonator. In particular, it has to be satisfied at ( ), ,x y z = ( )0,0,0 . We see that for the locus of points associated with (x = 0,y,z) and (x,y = 0,z) and (x,y,z = 0), we must have 0B D F= = = in the above equation. Note also that for the locus of points associated with ( )2 , ,xx m k y zπ= and ( ), 2 ,yx y n k zπ=

and ( ), , 2 zx y z kπ= where , ,m n = odd integers (1, 3, 5, 7, etc. …) we must have:

0x y zAk Ck Ek+ + = . Note further that this relation is automatically satisfied for , ,m n = even integers (2, 4, 6, 8, etc. …).

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UIUC Physics 436 EM Fields & Sources II Fall Semester, 2011 Lect. Notes 10.5 Prof. Steven Errede

© Professor Steven Errede, Department of Physics, University of Illinois at Urbana-Champaign, Illinois 2005-2011. All Rights Reserved.

4

Thus:

( ) ( ) ( ) ( )( ) ( ) ( ) ( )( ) ( ) ( ) ( )

1, 2,3, 4,, , cos sin sin

, , sin cos sin 1, 2,3, 4,

, , sin sin sin 1, 2,3, 4,

x

ox x y z

oy x y z y

oz x y z

z

mk maE x y z A k x k y k z

nE x y z C k x k y k z k nb

E x y z E k x k y k zk

d

π

π

π

⎧ ⎛ ⎞= =⎜ ⎟⎪ ⎝ ⎠⎫= ⎪⎪⎪⎪ ⎛ ⎞= = =⎬⎨ ⎜ ⎟⎝ ⎠⎪⎪

= ⎪⎪⎭ ⎛ ⎞= =⎪ ⎜ ⎟⎝ ⎠⎩

With: ( ) ˆ ˆ ˆ, ,o ox oy ozE x y z E x E y E z= + + n.b.: 0m n= = = simultaneously is not allowed!

Now use Faraday’s Law to determine B :

( )iB Eω

= − ∇×

( ) ( ) ( ) ( ) ( ) ( )sin cos cos sin cos cosoyozox y x y z z x y z

EEi iB Ek k x k y k z Ck k x k y k zy zω ω

⎛ ⎞∂∂ ⎡ ⎤= − − = − −⎜ ⎟ ⎣ ⎦⎜ ⎟∂ ∂⎝ ⎠

( ) ( ) ( ) ( ) ( ) ( )cos sin cos cos sin cosox ozoy z x y z x x y z

E Ei iB Ak k x k y k z Ek k x k y k zz xω ω

⎛ ⎞∂ ∂ ⎡ ⎤= − − = − −⎜ ⎟ ⎣ ⎦∂ ∂⎝ ⎠

( ) ( ) ( ) ( ) ( ) ( ) cos cos sin cos cos sinoy oxoz x x y z y x y z

E Ei iB Ck k x k y k z Ak k x k y k zx yω ω

⎛ ⎞∂ ∂ ⎡ ⎤= − − = − −⎜ ⎟ ⎣ ⎦⎜ ⎟∂ ∂⎝ ⎠

OR:

( )

( ) ( ) ( ) ( ){( ) ( ) ( ) ( )

( ) ( ) ( ) ( ) }

ˆ ˆ ˆ, ,

ˆ sin cos cos

ˆ cos sin cos

ˆ cos cos sin

o ox oy oz

y z x y z

z x x y z

x y x y z

B x y z B x B y B z

i Ek Ck k x k y k z x

Ak Ek k x k y k z y

Ck Ak k x k y k z y

ω

= + +

= − −

+ −

+ −

This expression for ( ), ,oB x y z (already) automatically satisfies boundary condition (2) 0B⊥ = : 0oxB = at 0,x x a= = 0oyB = at 0,y y b= = 0ozB = at 0,z z d= =

with xmkaπ⎛ ⎞≡ ⎜ ⎟

⎝ ⎠ with y

nkbπ⎛ ⎞≡ ⎜ ⎟

⎝ ⎠ with zk

dπ⎛ ⎞≡ ⎜ ⎟

⎝ ⎠

0,1, 2,m = … 0,1, 2,n = … 0,1, 2,= …

Page 5: P436_Lect_10p5

UIUC Physics 436 EM Fields & Sources II Fall Semester, 2011 Lect. Notes 10.5 Prof. Steven Errede

© Professor Steven Errede, Department of Physics, University of Illinois at Urbana-Champaign, Illinois 2005-2011. All Rights Reserved.

5

Does ( ), , 0oB x y z∇ =i ???

( )

( ){ ( ) ( ) ( )

, ,

cos cos cos

oyox ozo

x y z x y z x y

BB BB x y zx y z

i ik Ek Ck k x k y k z k k Eω ω

∂∂ ∂∇ = + +

∂ ∂ ∂

= − − = −

i

{ x zk k C−

( ) ( ) ( ) ( ) cos cos cos y z x x y z y zk Ak Ek k x k y k z k k A+ − + x yk k E−

( ) ( ) ( ) ( )} cos cos cos z x y x y z x zk Ck Ak k x k y k z k k C+ − + y zk k A− }( ) ( ) ( ) cos cos cosx y zk x k y k z⎡ ⎤× ⎣ ⎦

∴ ( ), , 0oB x y z∇ =i YES!!!

For TE modes:

0zE = ⇒ coefficient 0E = . Then 0x y zAk Ck Ek+ + = tells us that: 0x yAk Ck+ = or: x

y

kC Ak

⎛ ⎞= − ⎜ ⎟⎜ ⎟

⎝ ⎠

( ) ( ) ( ) ( ), , cos sin sinox x y zE x y z A k x k y k z= , 1, 2,xmk maπ⎛ ⎞= =⎜ ⎟

⎝ ⎠…

( ) ( ) ( ) ( ), , sin cos sinxoy x y z

y

kE x y z A k x k y k zk

⎛ ⎞= − ⎜ ⎟⎜ ⎟

⎝ ⎠ , 1, 2,y

nk nbπ⎛ ⎞= =⎜ ⎟

⎝ ⎠…

( ), , 0ozE x y z = , 1, 2,zkdπ⎛ ⎞= =⎜ ⎟

⎝ ⎠…

(n = 0 is NOT allowed for TE modes!!!)

( ) ( ) ( ) ( ), , sin cos cosxox z x y z

y

kiB x y z A k k x k y k zkω

⎛ ⎞= − ⎜ ⎟⎜ ⎟

⎝ ⎠

( ) ( ) ( ) ( ), , cos sin cosoy x y ziB x y z A k x k y k zω

= −

( ) ( ) ( ) ( ), , cos cos sinxoz x y x y z

y

kiB x y z A k k k x k y k zkω

⎡ ⎤⎛ ⎞= + +⎢ ⎥⎜ ⎟⎜ ⎟⎢ ⎥⎝ ⎠⎣ ⎦

The lowest

, ,m nTE mode

( )a b d> >

is: 111TE

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UIUC Physics 436 EM Fields & Sources II Fall Semester, 2011 Lect. Notes 10.5 Prof. Steven Errede

© Professor Steven Errede, Department of Physics, University of Illinois at Urbana-Champaign, Illinois 2005-2011. All Rights Reserved.

6

For TM modes:

0zB = ⇒ ( ) 0x yCk Ak− = or: y

x

kC A

k⎛ ⎞

= + ⎜ ⎟⎝ ⎠

( ) ( ) ( ) ( ), , cos sin sinox x y zE x y z A k x k y k z= , 1, 2,xmk maπ⎛ ⎞= =⎜ ⎟

⎝ ⎠…

( ) ( ) ( ) ( ), , sin cos cosyoy x y z

x

kE x y z A k x k y k z

k⎛ ⎞

= ⎜ ⎟⎝ ⎠

, 1, 2,ynk nbπ⎛ ⎞= =⎜ ⎟

⎝ ⎠…

(m = 0 is NOT allowed for TM modes!!!) , 1,2,zkdπ⎛ ⎞= =⎜ ⎟

⎝ ⎠…

( ) ( ) ( ) ( ), , sin sin cosy yxoz x y z

z x z

k kkE x y z A k x k y k zk k k

⎡ ⎤⎛ ⎞⎛ ⎞ ⎛ ⎞= − +⎢ ⎥⎜ ⎟⎜ ⎟ ⎜ ⎟

⎝ ⎠ ⎝ ⎠⎝ ⎠⎣ ⎦

( ) ( ) ( ) ( ), , sin cos cosy y yox x y z x y z

x z x

k k kiB x y z A k k A k k x k y k zk k kω

⎧ ⎫⎡ ⎤⎛ ⎞ ⎛ ⎞⎛ ⎞⎪ ⎪= + + +⎨ ⎬⎢ ⎥⎜ ⎟ ⎜ ⎟⎜ ⎟⎝ ⎠⎝ ⎠ ⎝ ⎠⎪ ⎪⎣ ⎦⎩ ⎭

( ) ( ) ( ) ( ), , cos sin cosy xoy z x y x y z

x x

k kiB x y z Ak A k k k x k y k zk kω

⎧ ⎫⎡ ⎤⎛ ⎞ ⎛ ⎞⎪ ⎪= − + +⎨ ⎬⎢ ⎥⎜ ⎟ ⎜ ⎟⎝ ⎠ ⎝ ⎠⎪ ⎪⎣ ⎦⎩ ⎭

( ), , 0ozB x y z =

For either TE or TM modes: 2

2 2 2 2x y zk k k k

cω⎛ ⎞≡ + + = ⎜ ⎟⎝ ⎠

with:

, 1, 2,xmk maπ⎛ ⎞= =⎜ ⎟

⎝ ⎠… , 1, 2,y

nk nbπ⎛ ⎞= =⎜ ⎟

⎝ ⎠… , 1,2,zk

dπ⎛ ⎞= =⎜ ⎟

⎝ ⎠…

The angular cutoff frequency for th, ,m n mode is the same for TE/TM modes in a rectangular cavity:

2 2 2

mnm nca b dπ π πω ⎛ ⎞ ⎛ ⎞ ⎛ ⎞= + +⎜ ⎟ ⎜ ⎟ ⎜ ⎟

⎝ ⎠ ⎝ ⎠ ⎝ ⎠ and: prop phasev c v

= = = no dispersion.

The lowest

, ,m nTM mode

( )a b d> >

is: 111TM

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UIUC Physics 436 EM Fields & Sources II Fall Semester, 2011 Lect. Notes 10.5 Prof. Steven Errede

© Professor Steven Errede, Department of Physics, University of Illinois at Urbana-Champaign, Illinois 2005-2011. All Rights Reserved.

7

B.) The Spherical Resonant Cavity The general problem of EM modes in a spherical cavity is mathematically considerably more involved (e.g. than for the rectangular cavity) due to the vectorial nature of the and E B -fields. ⇒For simplicity’s sake, it is conceptually easier to consider the scalar wave equation, with a

scalar field ( ),r tψ satisfying the free-source wave equation ( ) ( )22

2

,1, 0r t

r tc t

ψψ

∂∇ − =

which can be Fourier-analyzed in the time domain ( ) ( ), , i tr t r e dωψ ψ ω ω∞ −

−∞= ∫ with each

Fourier component ( ),rψ ω satisfying the Helmholtz Wave Equation: ( ) ( )2 2 , 0k rψ ω∇ + =

with ( )22k cω= i.e. no dispersion. In spherical coordinates the Laplacian operator is:

( ) ( )( ) ( ) ( )222

2 2 2 2 2

, ,1 1 1, , sinsin sin

r rr r r

r r r rψ ω ψ ω

ψ ω ψ ω θθ θ θ θ ϕ

∂ ∂⎛ ⎞∂ ∂∇ = + +⎜ ⎟∂ ∂ ∂ ∂⎝ ⎠

To solve this scalar wave equation – we again try a product solution of the form:

( ) ( ) ( ) ( ), i tR rr P Q e

rωψ ω θ ϕ= ⇒ ( ) ( )

,sphericalharmonics

,m mm

f r Y θ ϕ∑

Plug this ( ),rψ ω into the above scalar wave equation, use the separation of variables technique:

Get radial equation: ( ) ( )

22

2 2

12 0d d k f rdr r dr r

+⎡ ⎤+ + − =⎢ ⎥

⎣ ⎦ where = 0, 1, 2, . . .

Let ( ) ( )1f r u rr

= . Then we obtain Bessel’s equation with index 12v = + :

( ) ( )22 1

222 2

1 0d d k u rdr r dr r

⎡ ⎤++ + − =⎢ ⎥

⎢ ⎥⎣ ⎦

Solutions of the (radial) Bessel’s equation are of the form: ( ) ( ) ( )1 12 2

1 12 2

Bessel fcn of 1st Bessel fcn of 2ndkind of order kind of order

m mm

A Bf r J kr N krr r+ +

+ +

= +

It is customary to define so-called spherical Bessel functions and spherical Hankel functions:

( ) ( )12

122

j x J xxπ

+⎛ ⎞≡ ⎜ ⎟⎝ ⎠

where: x kr=

( ) ( )12

122

n x N xxπ

+⎛ ⎞≡ ⎜ ⎟⎝ ⎠

The ( ),mY θ ϕ satisfy the angular portion of scalar wave equation…

Page 8: P436_Lect_10p5

UIUC Physics 436 EM Fields & Sources II Fall Semester, 2011 Lect. Notes 10.5 Prof. Steven Errede

© Professor Steven Errede, Department of Physics, University of Illinois at Urbana-Champaign, Illinois 2005-2011. All Rights Reserved.

8

and: ( ) ( ) ( ) ( ) ( ) ( )12

1 12 2

1,2 2

h x J x iN x j x i n xxπ

+ +⎛ ⎞ ⎡ ⎤≡ ± = ±⎜ ⎟ ⎣ ⎦⎝ ⎠

( ) ( ) ( )sin1 xdj x x

x dx x⎛ ⎞⎛ ⎞= − ⎜ ⎟⎜ ⎟

⎝ ⎠ ⎝ ⎠

( ) ( ) ( )cos1 xdn x xx dx x

⎛ ⎞⎛ ⎞= − − ⎜ ⎟⎜ ⎟⎝ ⎠ ⎝ ⎠

( ) ( )0

sin

xj x

x= ( ) ( )1

0 ixeh x

ix=

( ) ( )0

cos xn x

x= − ( ) ( )2

0

ixeh xix

=−

( ) ( ) ( )1 2

sin cos

x xj x

x x= − ( ) ( )1

1 1ixe ih xx x⎛ ⎞= − +⎜ ⎟⎝ ⎠

( ) ( ) ( )1 2

cos sinx xn x

x x= − − ( ) ( )2

1 1ixe ih x

x x

− ⎛ ⎞= − −⎜ ⎟⎝ ⎠

For 1, x :

( ) ( ) ( )2

1 ...2 1 !! 2 2 3

x xj x⎛ ⎞

≈ − +⎜ ⎟⎜ ⎟+ +⎝ ⎠ where: ( ) ( )( )( )2 1 !! 2 1 2 1 2 3 ... 5 3 1+ = + − − × × ×

( ) ( )( )

2

1

2 1 !!1 ...

2 1 2xn x

x +

⎛ ⎞−≈ − − +⎜ ⎟⎜ ⎟−⎝ ⎠

For 1, x :

( ) 1 sin2

j x xx

π⎛ ⎞≈ −⎜ ⎟⎝ ⎠

( ) 1 cos2

n x xx

π⎛ ⎞≈ − −⎜ ⎟⎝ ⎠

The general solution to Helmholtz’s equation in spherical coordinates can be written as:

( ) ( ) ( ) ( ) ( ) ( ) ( ) ( )1 1 2 2

,, ,m m m

m

r t A h kr A h kr Yψ θ ϕ⎡ ⎤

= +⎢ ⎥⎢ ⎥⎣ ⎦

Coefficients are determined by boundary conditions. For the case of EM waves in a spherical resonant cavity we will (here) only consider TM modes, which for spherical geometry means that the radial component of , 0rB B = . We further assume

(for simplicity’s sake) that the E and B -fields do not have any explicit ϕ -dependence.

n.b. If x = kr is real, then( ) ( ) ( ) ( )2 * 1h x h x=

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UIUC Physics 436 EM Fields & Sources II Fall Semester, 2011 Lect. Notes 10.5 Prof. Steven Errede

© Professor Steven Errede, Department of Physics, University of Illinois at Urbana-Champaign, Illinois 2005-2011. All Rights Reserved.

9

Hence: ( ) ( )( ) ( )2 1 !

, cos4 !

m imm

mY P e

mφθ ϕ θ

π+ −

=+

Will have some restrictions imposed on it Associated Legendré Polynomial

If 0rB = and B ≠ explicit function of ϕ , then: 0B∇ =i ⇒ 0Bϕ ≠ {necessarily}

But: BEt

∂∇× = −

∂ requires: 0Eϕ =

→ TM modes with no explicit ϕ -dependence involve only rE , Eθ and Bϕ

Combining BEt

∂∇× = −

∂ and 2

1 EBc t

∂∇× =

∂ with harmonic time dependence i te ω− of solutions,

We obtain: 2

0B Bcω⎛ ⎞ −∇×∇× =⎜ ⎟⎝ ⎠

The ϕ -component of this equation is:

( ) ( ) ( )2 2

2 2

1 1 sin 0sin

rB rB rBc r rϕ ϕ ϕω θ

θ θ θ∂ ∂ ∂⎛ ⎞ ⎡ ⎤+ + =⎜ ⎟ ⎢ ⎥∂ ∂ ∂⎝ ⎠ ⎣ ⎦

But: ( ) ( )2

~Legendré equation with 1

1 1sin sinsin sin sin

m

rB rBrB ϕ ϕ

ϕθ θθ θ θ θ θ θ θ

⎛ ⎞∂∂ ∂ ∂⎡ ⎤ ⎜ ⎟= −⎢ ⎥ ⎜ ⎟∂ ∂ ∂ ∂⎣ ⎦ ⎝ ⎠

⇒ Try product solutions of the form: ( ) ( ) ( )1, cosu r

B r Prϕ θ θ=

Substituting this into the above equation gives a differential equation for ( )u r of the form of:

Bessel’s equation: ( ) ( ) ( )

22

2 2

10

d u ru r

dr c rω⎡ ⎤+⎛ ⎞+ − ≡⎢ ⎥⎜ ⎟⎝ ⎠⎢ ⎥⎣ ⎦

with = 0, 1, 2, 3, . . . defining the

angular dependence of the TM modes. Let us consider a resonant spherical cavity as two concentric, perfectly conducting spheres of inner radius a and outer radius b.

If ( ) ( ) ( )1, cosu r

B r Prϕ θ θ= , the radial and tangential electric fields (using Ampere’s Law) are:

( ) ( ) ( ) ( ) ( )2 2

, sin 1 cossinr

u ric icE r B Pr r rϕθ θ θ

ω θ θ ω∂

= = − +∂

( ) ( ) ( ) ( )2 2

1, cosu ric icE r rB P

r r r rθ ϕθ θω ω

∂∂= − = −

∂ ∂

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UIUC Physics 436 EM Fields & Sources II Fall Semester, 2011 Lect. Notes 10.5 Prof. Steven Errede

© Professor Steven Errede, Department of Physics, University of Illinois at Urbana-Champaign, Illinois 2005-2011. All Rights Reserved.

10

But E Eθ = which must vanish at r = a and r = b ⇒ ( ) ( ) 0r a r b

u r u rr r= =

∂ ∂= =

∂ ∂

The solutions of the radial Bessel equation are spherical Bessel functions (or spherical Hankel functions).

The above radial boundary conditions on ( ) 0r ar b

u rr =

=

∂=

∂ lead to transcendental equations for the

characteristic frequencies, ω {eeeEEK}!!!

However {don’t panic!}, if: (b – a) = h is such that h a then: ( ) ( )

2 2

1 1constant!!!

r a+ +

≈ = And thus in this situation, the solutions of Bessel’s equation:

( ) ( ) ( )

22

2 2

10

d u ru r

dr c aω⎡ ⎤+⎛ ⎞+ − =⎢ ⎥⎜ ⎟⎝ ⎠⎢ ⎥⎣ ⎦

⇒ ( ) ( )

22

2 0d u r

k u rdr

+ = where: ( )2

22

1k

c aω +⎛ ⎞= −⎜ ⎟⎝ ⎠

are simply sin (kr) and cos (kr) !!! i.e. ( ) ( ) ( )cos sinu r A kr B kr= +

Then: ( ) ( )sin cos 0r a

u kA ka kB kar =

∂= − + =

∂ and ( ) ( )sin cos 0

r b

u kA kb kB kbr =

∂= − + =

For ( )b a h a− = an approximate solution is: ( ) [ ]cosu r A kr ka−

with: ( )kh k b a nπ= − = , n = 0, 1, 2, . . .

Thus: ( )2 2

22

1n

nkc a hω π+⎛ ⎞ ⎛ ⎞= − =⎜ ⎟ ⎜ ⎟⎝ ⎠ ⎝ ⎠

, n = 0, 1, 2, 3, . . . and = 0, 1, 2, 3, . . .

The corresponding angular cutoff frequency is:

( ) ( )22

2 2

1 1n n

nc k ca h a

πω+ +⎛ ⎞+ +⎜ ⎟

⎝ ⎠ for h a , n = 0, 1, 2, 3, . . . and = 0, 1, 2, 3, . . .

Because h a , we see that the modes with n = 1, 2, 3, . . . turn out to have relatively high

frequencies nnchπω ⎛ ⎞≈ ⎜ ⎟

⎝ ⎠ for 1n ≥ . However, the n = 0 modes have relatively low frequencies:

( ) ( )0 2

11cc

a aω

++ for h a .

An exact solution (correct to first order in (h/a) expansion) for n = 0 is: ( ) ( )0 1

2

1ca h

ω = ++

These eigen-mode frequencies are known as Schumann resonance frequencies. = 1, 2, 3, . . . (W.O. Schumann – Z. Naturforsch. 72, 149, 250 (1952))

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UIUC Physics 436 EM Fields & Sources II Fall Semester, 2011 Lect. Notes 10.5 Prof. Steven Errede

© Professor Steven Errede, Department of Physics, University of Illinois at Urbana-Champaign, Illinois 2005-2011. All Rights Reserved.

11

For n = 0, the EM fields are: 0 0Eθ = , ( )02

1 cosrE Pr

θ∼ and ( )0 11 cosB Prϕ θ∼

Very Useful Table:

ˆ ˆr θ ϕ× = ˆ ˆrθ ϕ× = − ˆ ˆ rθ ϕ× = ˆˆ rϕ θ× = −

ˆˆ rϕ θ× = ˆˆr ϕ θ× = − Poynting’s vector:

( ) ( ) ( ) ( ) ( ) ( )( )1 10 0 0 3 3

0

1 1 1 ˆˆˆ cos cos cos cosS E B r P P P Pr r

ϕ θ θ θ θ θμ

= × × −∼ ∼ ⇐

The Earth’s surface and the Earth’s ionosphere behave as a spherical resonant cavity (!!!) with the Earth’s surface {approximately} as the inner spherical surface: 6378 kma r rΕ ⊕≡ =

66.378 10 m= × (= Earth’s mean equatorial radius), the height h (above the surface of the Earth) of the ionosphere is: 5100 km 10 mh = ( a ) → b = a + h 6.478 x 106 m.

For the n = 0 Schumann resonances: ( ) ( )0 1

2

1ca h

ω = ++

for h a .

1:= ( )01 1

2

2ca h

ω+

⇒ 0101 10.5 Hz

2f ω

π= =

2 := ( )02 1

2

6ca h

ω+

⇒ 0202 18.3 Hz

2f ω

π= =

3 := ( )03 1

2

12ca h

ω+

⇒ 0303 25.7 Hz

2f ω

π= =

4 := ( )04 1

2

20ca h

ω+

⇒ 0404 33.2 Hz

2f ω

π= =

5 := ( )05 1

2

30ca h

ω+

⇒ 0505 46.7 Hz

2f ω

π= = (. . . etc.)

The n = 0 Schumann resonances in the Earth-ionosphere cavity manifest themselves as peaks in the noise power spectrum in the VLF (Very Low Frequency) portion of the EM spectrum → VLF EM standing waves in the spherical cavity of the Earth-ionosphere system!!!

y

z

x

ϕ

θ

0ˆ ˆ, Bϕϕ ϕ 0ˆ ˆ, rr E r

θ

0S

a

b

Circumpolar N-S waves!

n.b. For the n = 1 Schumann resonances:

1 1.5 f KHz≈

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UIUC Physics 436 EM Fields & Sources II Fall Semester, 2011 Lect. Notes 10.5 Prof. Steven Errede

© Professor Steven Errede, Department of Physics, University of Illinois at Urbana-Champaign, Illinois 2005-2011. All Rights Reserved.

12

Schumann resonances in the Earth-ionosphere cavity are excited by the radial E -field component of lightning discharges (the frequency component of EM waves produced by lightning at these Schumann resonance frequencies). Lightning discharges (anywhere on Earth) contain a wide spectrum of frequencies of EM radiation – the frequency components f01, f02, f03, f04, . . excite these resonant modes – the Earth literally “rings like a bell” at these frequencies!!! The n = 0 Schumann resonances are the lowest-lying normal modes of the Earth-ionosphere cavity. Schumann resonances were first definitively observed in 1960. (M. Balser and C.A. Wagner, Nature 188, 638 (1960)). → Nikola Tesla may have observed them before 1900!!! (Before the ionosphere was known to even exist!!!) He also estimated the lowest modal frequency to be f01 ~ 6 Hz!!! n = 0 Schumann Resonances:

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UIUC Physics 436 EM Fields & Sources II Fall Semester, 2011 Lect. Notes 10.5 Prof. Steven Errede

© Professor Steven Errede, Department of Physics, University of Illinois at Urbana-Champaign, Illinois 2005-2011. All Rights Reserved.

13

The observed Schumann resonance frequencies are systematically lower than predicted,

(primarily) due to damping effects: 2 20

11 iQ

ω ω⎡ ⎤+

≈ −⎢ ⎥⎣ ⎦

where Q = Quality factor 0ω≡Γ

= “Q”

of resonance, and Γ = width at half maximum of power spectrum: The Earth’s surface is also not perfectly conducting. Seawater conductivity 0.1Cσ Siemens!! Neither is the ionosphere! → Ionosphere’s conductivity 4 710 10Cσ

− −− Siemens

• On July 9, 1962, a nuclear explosion (EMP) detonated at high altitude (400 km) over Johnson Island in the Pacific {Test Shot: Starfish Prime, Operation Dominic I}. - Measurably affected the Earth’s ionosphere and radiation belts on a world-wide scale! - Sudden decrease of ~ 3 – 5% in Schumann frequencies – increase in height of ionosphere! - Change in height of ionosphere: ( )2 0.03 0.05 400 600 h h h R km⊕′Δ = − ⋅ − ≈ − !!! - Height changes decayed away after ~ several hours. - Artificial radiation belts lasted several years!

• Note that # of lightning strikes, (e.g. in tropics) is strongly correlated to average temperature. ⇒Scientists have used Schumann resonances & monthly mean magnetic field strengths to monitor lightning rates and thus monitor monthly temperatures – they all correlate very well!!!

• Monitoring Schumann Resonances → Global Thermometer → useful for Global Warming studies!!

Earth Coordinate System

( ) ( )0 12

12

cfa hπ

++

0 0Eθ = (north – south)

( )02

1 cosrE Pr

θ∼ (up – down)

( )0 11 cosB Prϕ θ∼ (east – west)

( ) ( )( )10 3

1 ˆcos cosS P Pr

θ θ θ−∼ (north – south) For the n = 0 modes of Schumann Resonances:

ˆE r (up – down) ˆB ϕ (east – west) ˆS θ− (north – south)

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UIUC Physics 436 EM Fields & Sources II Fall Semester, 2011 Lect. Notes 10.5 Prof. Steven Errede

© Professor Steven Errede, Department of Physics, University of Illinois at Urbana-Champaign, Illinois 2005-2011. All Rights Reserved.

14

We can observe Schumann resonances right here in town / @ UIUC!! Use e.g. Gibson P-90 single-coil electric guitar pickup ( )90 10 Henrys, ~10K turns #42AWG copper wirePL − for detector of Schumann waves and a spectrum analyzer (e.g. HP 3562A Dynamic Signal Analyzer) – read out the HP 3562A into PC via GPIB. → Orientation/alignment of Gibson P-90 electric guitar pickup is important – want axis of pickup aligned ˆB ϕ (i.e. oriented east – west) as shown in figure below. n.b. only this orientation yielded Schumann-type resonance signals {also tried 2 other 90o orientations {up-down} and {north-south} but observed no signal(s) for Schumann resonances for these.} Electric guitar PU’s are very sensitive – e.g. they can easily detect car / bus traffic on street below from 6105 ESB (6th Floor Lab) – can easily see car/bus signal from PU on a ‘scope!!! n.b. PU housed in 4π closed, grounded aluminum sheet-metal box to suppress electric noise.

Page 15: P436_Lect_10p5

UIUC Physics 436 EM Fields & Sources II Fall Semester, 2011 Lect. Notes 10.5 Prof. Steven Errede

© Professor Steven Errede, Department of Physics, University of Illinois at Urbana-Champaign, Illinois 2005-2011. All Rights Reserved.

15