electrodinamics

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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 ( ) ( ) ( ) ( ) , , , , . . each is a fcn , , , , ox ox oy oy oz oz E E xyz E E xyz ie xyz E E xyz = = = Subject to the boundary conditions || 0 E = and 0 B = 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.

    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

    ==

    G G G G

    Maxwells Equations (inside the rectangular resonant cavity away from the walls): (1) Gauss Law: (2) No Monopoles:

    0E =G Gi 0oE =G Gi 0B =G Gi 0oB =

    G Gi (3) Faradays Law: (4) Amperes Law:

    BEt

    = GG G

    o oE i B =G G G 2

    1 EBc t

    = GG G

    2o oB i Ec = G G

    Take the curl of (3): = 0 {Gauss Law}

    ( ) ( ) ( ) 22o o o o oE i B E E i B Ec = = = = G G G G G G G G G G G G i {using (4) Amperes Law}

    22

    22

    22

    ox ox

    oy oy

    oz oz

    E Ec

    E Ec

    E Ec

    = = =

    G

    G

    G

    ( )( )( )

    ( ), ,

    , , . . each is a fcn , ,

    , ,

    ox ox

    oy oy

    oz oz

    E E x y z

    E E x y z i e x y z

    E E x y z

    = = =

    Subject to the boundary conditions

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

  • 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 zG we try product solutions and then use the separation of variables technique:

    ( ) ( ) ( ) ( ), ,io i i i

    E x y z X x Y y Z z for ( ) 22 , ,i io o

    E x y z Ec =

    where subscript , ,i x y z= .

    ( ) ( ) ( ) ( ) ( ) ( ) ( ) ( ) ( ) ( ) ( ) ( )22 2 22 2 2i i ii i i i i i i i iX 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 + + =

    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 ii i i

    fcn x fcn y fcn z

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

    = =

    + + =

    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 constanti xi

    X xk

    X x x = =

    ( ) ( )2 22 0i x iX x k X xx + =

    ( )( )2 22

    1 constanti yi

    Y yk

    Y y y = =

    ( ) ( )2 22 0i y iY y k Y yy + =

    ( )( )2 22

    1 constanti zi

    Z zk

    Z z z = =

    ( ) ( )2 22 0i z iZ z k Z zz + =

    with: 2

    2 2 2 2x y zk k k k c

    + + = 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 z

    E 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 !!!

  • 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, oxy y b

    Ez z d= = = = = coefficients

    0

    0x

    x

    E

    C

    = = and

    , 1, 2,3,....

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

    z

    k n b nk d

    = = = = A A

    0, 0 at

    0, oyx x a

    Ez z d= = = = = coefficients

    0

    0y

    y

    A

    E

    = = and

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

    x

    z

    k m b mk d

    = = = = A A

    0, 0 at

    0, ozx x a

    Ey y b= = = = = coefficients

    0

    0z

    z

    A

    C

    = = and

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

    x

    y

    k m a mk n d n

    = = = =

    n.b. m = 0, and/or n = 0 and/or 0=A are not allowed, otherwise ( ), , 0io

    E x y z (trivial solution).

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

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

    , , cos sin sin sin

    , , sin cos sin sin

    , , sin sin cos sin

    ox x x y z

    oy x 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 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 =G Gi 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 z= and ( ), 2 ,yx y n k z= and ( ), , 2 zx y z k= A where , ,m n =A 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 =A even integers (2, 4, 6, 8, etc. ).

  • 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 cos 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

    = = = = = = = = =

    A A

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

    Now use Faradays Law to determine BG

    :

    ( )iB E= G G G ( ) ( ) ( ) ( ) ( ) ( )sin cos cos sin cos cosoyozox y x y z z x y zEEi iB Ek k x k y k z Ck k x k y k zy z

    = =

    ( ) ( ) ( ) ( ) ( ) ( )cos sin cos cos sin cosox ozoy z x y z x x y zE Ei iB Ak k x k y k z Ek k x k y k zz x = =

    ( ) ( ) ( ) ( ) ( ) ( ) cos cos sin cos cos sinoy oxoz x x y z y x y zE Ei iB Ck k x k y k z Ak k x k y k zx y = =

    OR:

    ( )( ) ( ) ( ) ( ){( ) ( ) ( ) ( )( ) ( ) ( ) ( ) }

    , ,

    sin cos cos

    cos sin cos

    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 zi 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

    = + +=

    + +

    G

    This expression for ( ), ,oB x y zG (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 xmka with y

    nkb with zk d

    A

    0,1, 2,m = 0,1, 2,n = 0,1, 2,=A

  • 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 =G Gi ???

    ( )( ){ ( ) ( ) ( )

    , ,

    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 E

    = + + = =

    G Gi

    { 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 =G Gi YES!!!

    For TE modes:

    0zE =G

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

    kC Ak

    =

    ( ) ( ) ( ) ( ), , cos sin sinox x y zE x y z A k x k y k z= , 1, 2,x mk ma = = ( ) ( ) ( ) ( ), , sin cos sinxoy x y z

    y

    kE x y z A k x k y k zk

    = , 1, 2,y nk nb

    = =

    ( ), , 0ozE x y z = , 1, 2,zk d = = A A

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

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

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

    =

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

    y

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

    = + +

    The lowest

    , ,m nTE A mode

    ( )a b d> > is: 111TE

  • 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 =G

    ( ) 0x yCk Ak = or: yx

    kC A

    k = +

    ( ) ( ) ( ) ( ), , cos sin sinox x y zE x y z A k x k y k z= , 1, 2,x mk ma = = ( ) ( ) ( ) ( ), , sin cos cosyoy x y z

    x

    kE x y z A k x k y k z

    k = , 1, 2,y nk nb

    = =

    (m = 0 is NOT allowed for TM modes!!!) , 1,2,zk d = = A A

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

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

    = + + +

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

    k kiB x y z Ak A k k k x k y k zk k

    = + +

    ( ), , 0ozB x y z =

    For either TE or TM modes: 2

    2 2 2 2x y zk k k k c

    + + = with:

    , 1, 2,xmk ma = = , 1, 2,y

    nk nb = = , 1,2,zk d

    = = A A

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

    2 2 2

    mnm nca b d = + + A

    A and: prop phasev c vk

    = = = no dispersion.

    The lowest

    , ,m nTM A mode

    ( )a b d> > is: 111TM

  • 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

    G G-fields.

    For simplicitys sake, it is conceptually easier to consider the scalar wave equation, with a scalar field ( ),r t G satisfying the free-source wave equation ( ) ( )22 2 ,1, 0r tr t c t

    =GG

    which can be Fourier-analyzed in the time domain ( ) ( ), , i tr t r e d = G G with each Fourier component ( ),r G satisfying the Helmholtz Wave Equation: ( ) ( )2 2 , 0k r + =G with ( )22k c= i.e. no dispersion. In spherical coordinates the Laplacian operator is:

    ( ) ( )( ) ( ) ( )222 2 2 2 2 2, ,1 1 1, , sinsin sinr r

    r r rr r r r

    = + +

    G GG G

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

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

    =G ( ) ( ),

    sphericalharmonics

    ,m mm

    f r Y A AA

    Plug this ( ),r G into the above scalar wave equation, use the separation of variables technique: Get radial equation:

    ( ) ( )2 22 2 12 0d d k f rdr r dr r+ + + = A

    A A where A = 0, 1, 2, . . .

    Let ( ) ( )1f r u rr

    =A A . Then we obtain Bessels equation with index 12v = +A :

    ( ) ( )22 1

    222 2

    1 0d d k u rdr r dr r

    ++ + = A

    A

    Solutions of the (radial) Bessels 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+ +

    + +

    = +A AA A AA A

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

    ( ) ( )12

    122

    j x J xx

    + A A where: x kr=

    ( ) ( )12

    122

    n x N xx

    + A A

    The ( ),mY A satisfy the angular portion of scalar wave equation

  • 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 xx

    + + = A A AA A

    ( ) ( ) ( )sin1 xdj x xx dx x

    = A

    AA

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

    = A

    AA

    ( ) ( )0 sin xj x x= ( ) ( )10 ixeh x

    ix=

    ( ) ( )0 cos xn x x= ( ) ( )20ixeh xix

    =

    ( ) ( ) ( )1 2sin cos x xj x x x= ( ) ( )11 1ixe ih xx x = +

    ( ) ( ) ( )1 2cos sinx xn x x x= ( ) ( )21 1ixe ih x

    x x

    =

    For 1, x A :

    ( ) ( ) ( )2

    1 ...2 1 !! 2 2 3

    x xj x + + +

    A

    A A A where: ( ) ( )( )( )2 1 !! 2 1 2 1 2 3 ... 5 3 1+ = + A A A A

    ( ) ( ) ( )2

    1

    2 1 !!1 ...

    2 1 2xn x

    x + + A A

    AA

    For 1, x A : ( ) 1 sin

    2j x x

    x AA

    ( ) 1 cos2

    n x xx

    AA

    The general solution to Helmholtzs equation in spherical coordinates can be written as:

    ( ) ( )N ( ) ( ) ( )N ( ) ( ) ( )1 1 2 2,

    , ,m m mm

    r t A h kr A h kr Y = + A A A A AAG

    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 =

    G. We further assume

    (for simplicitys sake) that the EG

    and BG

    -fields do not have any explicit -dependence.

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

  • 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

    m

    + = +A AA A

    A

    Will have some restrictions imposed on it Associated Legendr Polynomial

    If 0rB = and B G

    explicit function of , then: 0B =G Gi 0B {necessarily} But:

    BEt

    = GG G

    requires: 0E = TM modes with no explicit -dependence involve only rE , E and B Combining

    BEt

    = GG G

    and 21 EBc t

    = GG G

    with harmonic time dependence i te of solutions,

    We obtain: 2

    0B Bc =

    G G G G

    The -component of this equation is:

    ( ) ( ) ( )2 22 21 1 sin 0sinrB rB rBc r r + + =

    But: ( ) ( ) 2~Legendr equation with 1

    1 1sin sinsin sin sin

    m

    rB rBrB

    =

    =

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

    = A A

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

    ( ) ( ) ( )22 2 2 1 0d u r u rdr c r + +

    AA

    A A with A = 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 rB r Pr

    = A A , the radial and tangential electric fields (using Amperes Law) are:

    ( ) ( ) ( ) ( ) ( )2 2, sin 1 cossinr u ric icE r B Pr r r = = + A AA A ( ) ( ) ( ) ( )2 2 1, cosu ric icE r rB Pr r r r = = A A

  • 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 E = & which must vanish at r = a and r = b ( ) ( ) 0r a r bu r u rr r= = = =

    A A 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 ==

    =A lead to transcendental equations for the

    characteristic frequencies, A {eeeEEK}!!! However {dont panic!}, if: (b a) = h is such that h a then: ( ) ( )2 21 1 constant!!!r a

    + + =A A A A And thus in this situation, the solutions of Bessels equation:

    ( ) ( ) ( )22 2 2 1 0d u r u rdr c a

    + + = A

    AA A

    ( ) ( )2 22 0d u r k u rdr + =A A where: ( )22

    2

    1k

    c a + =

    A A

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

    Then: ( ) ( )sin cos 0r a

    u kA ka kB kar =

    = + =A and ( ) ( )sin cos 0

    r b

    u kA kb kB kbr =

    = + =A

    For ( )b a h a = an approximate solution is: ( ) [ ]cosu r A kr kaA with: ( )kh k b a n= = , n = 0, 1, 2, . . .

    Thus: ( )2 22

    2

    1n

    nkc a h + = = A

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

    The corresponding angular cutoff frequency is:

    ( ) ( )222 2

    1 1n n

    nc k ca h a

    + + + + AA A A A for h a , n = 0, 1, 2, 3, . . . and A = 0, 1, 2, 3, . . .

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

    nch A for 1n . However, the n = 0 modes have relatively low frequencies:

    ( ) ( )0 2 1 1cc a a+ +A A A A A for h a .

    An exact solution (correct to first order in (h/a) expansion) for n = 0 is: ( ) ( )0 12 1c

    a h = ++A A A

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

  • 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 0E =A , ( )0 21 cosrE Pr A A and ( )0 11 cosB Pr

    A A Very Useful Table:

    r = r = r = r =

    r = r = Poyntings vector:

    ( ) ( ) ( ) ( ) ( ) ( )( )1 10 0 0 3 30

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

    = A A A A A A AG G G

    The Earths surface and the Earths ionosphere behave as a spherical resonant cavity (!!!) with the Earths surface {approximately} as the inner spherical surface: 6378 kma r r =

    66.378 10 m= (= Earths 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 12 1

    ca h

    = ++A A A for h a .

    1:=A ( )01 122c

    a h +

    0101 10.5 Hz2

    f = =

    2 :=A ( )02 126c

    a h +

    0202 18.3 Hz2

    f = =

    3 :=A ( )03 1212c

    a h +

    0303 25.7 Hz2

    f = =

    4 :=A ( )04 1220c

    a h +

    0404 33.2 Hz2

    f = =

    5 :=A ( )05 1230c

    a h +

    0505 46.7 Hz2

    f = = (. . . 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

    0 , B A 0 , rr E rA

    0S AG

    a

    b

    Circumpolar N-S waves!

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

    1 1.5 f KHzA

  • 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 EG

    -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:

  • 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 2011 iQ

    + where Q = Quality factor 0 = Q

    of resonance, and = width at half maximum of power spectrum: The Earths surface is also not perfectly conducting. Seawater conductivity 0.1C Siemens!! Neither is the ionosphere! Ionospheres conductivity 4 710 10C 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 Earths 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 = !!! - 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 12cf

    a h ++A A A 0 0E =A (north south)

    ( )0 21 cosrE Pr A A (up down) ( )0 11 cosB P

    rA A (east west)

    ( ) ( )( )10 31 cos cosS P Pr A A AG (north south) For the n = 0 modes of Schumann Resonances:

    E rG & (up down) B G & (east west) S G & (north south)

  • 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 B G& & (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 PUs 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 4 closed, grounded aluminum sheet-metal box to suppress electric noise.

  • 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