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Electromagnetic Waves, Antennas, and RF: Boundary Waves - Reflection, Transmission, and Refraction

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Electromagnetic Waves, Antennas, and RF: Boundary Waves - Reflection, Transmission, and Refraction

EM20 showed how a uniform electromagnetic wave propagates inside a homogeneous material. Real propagation paths are rarely uniform forever. A wave eventually meets a boundary: air to glass, air to soil, free space to a radome, dielectric to Conductor, or one layer of a circuit or antenna structure to another.

At that boundary, Maxwell’s Equations do not permit the fields to change arbitrarily. Their allowed discontinuities are fixed by the electromagnetic boundary conditions. Those conditions, together with the plane-wave relation between electric and magnetic fields, determine how much of the incident wave is reflected, how much is transmitted, whether the transmitted wave changes direction, and whether a phase reversal occurs [1, 3, 4, 5].

The central chain developed in this article is

  • Maxwell equations;
  • boundary conditionse;
  • Γ,τ;
  • R,T;
  • Snell and Fresnel laws;

1 The interface geometry

Let medium 1 occupy z < 0 and medium 2 occupy z > 0. The interface is the plane z = 0, with unit Normal

ˆn = ˆz
(1)

pointing from medium 1 into medium 2.

Each medium has constitutive parameters

(𝜖1,μ1, σ1),    (𝜖2,μ2,σ2),
(2)

and therefore its own propagation constant and intrinsic impedance,

                          ∘ -----------
                             --iωμm-----
γm =  αm + iβm,     ηm  =    σ  + iω𝜖  ,    m  = 1, 2.
                              m      m
(3)

For the first derivation we use lossless media, so η1 and η2 are real. The complex-impedance extension is introduced later.

2 Boundary conditions come directly from Maxwell’s equations

The wave-interface formulas are not separate laws added to Electromagnetism. They follow from the integral forms of Maxwell’s equations by shrinking the integration surface or contour around the interface [1, 2, 3].

2.1 Tangential electric field

Faraday’s law in integral form is

∮             d ∫
   E ⋅ dℓ = −--    B ⋅ da.
 C           dt  S
(4)

Take a narrow rectangular contour that straddles the interface. As its height tends to zero, the enclosed area tends to zero, so the magnetic-flux term vanishes for finite fields. The two long sides remain, giving

|-------------------|
ˆn × (E2 −  E1) = 0. |
---------------------
(5)

Thus the tangential electric field is continuous across an ordinary interface.

2.2 Tangential magnetic field

Ampere-Maxwell law gives

∮                    ∫
   H  ⋅ dℓ = I  +  d-   D  ⋅ da.
  C          free   dt  S
(6)

If a free surface-current density Ks exists at the interface, the limiting contour gives

|----------------------|
|ˆn × (H   − H  ) = K  .|
--------2-----1------s-
(7)

For the dielectric interfaces considered first,

K  =  0,
  s
(8)

so the tangential magnetic field is also continuous.

2.3 Normal electric flux density

Gauss’s Law applied to a thin pillbox gives

|--------------------|
|ˆn ⋅ (D2 − D1 ) = ρs,|
---------------------
(9)

where ρs is free surface-charge density.

2.4 Normal magnetic flux density

Gauss’s law for magnetism similarly gives

|------------------|
-ˆn-⋅ (B2-−-B1-) =-0.
(10)

The normal component of B is therefore continuous because magnetic monopole surface charge does not appear in classical electromagnetism.

PIC

Figure 1. Maxwell boundary conditions at an interface. A narrow loop isolates tangential-field conditions while a pillbox isolates normal-flux conditions.

3 Normal incidence: incident, reflected, and transmitted waves

Consider a linearly polarized plane wave incident normally from medium 1. Choose

Ei(z) = ˆxEi0e− iβ1z
(11)

for the incident phasor. The reflected wave propagates in the −z direction,

Er (z ) = xˆEr0e+i β1z,
(12)

and the transmitted wave propagates in the +z direction,

Et (z ) = xˆEt0e −iβ2z.
(13)

For a uniform plane wave,

     1
H  = --ˆk × E.
     η
(14)

Therefore

Hi  = ˆy Ei0e−iβ1z,
        η1
(15)

Hr  = − ˆyEr0-e+iβ1z,
          η1
(16)

and

H   = ˆy Et0e−iβ2z.
  t     η2
(17)

The minus sign in Hr is essential: the reflected wave carries energy toward −z.

4 Deriving the normal-incidence reflection coefficient

At z = 0, tangential E is continuous:

Ei0 + Er0 = Et0.
(18)

Tangential H is also continuous when Ks = 0:

Ei0-−  Er0-= Et0-.
 η1    η1     η2
(19)

Define the electric-field reflection coefficient

|--------|
|    Er0-|
Γ  ≡ E   |
-------i0--
(20)

and transmission coefficient

|--------|
τ ≡  Et0.|
-----Ei0--
(21)

The first boundary condition gives

1 + Γ = τ.
(22)

The magnetic-field condition gives

1-−-Γ-=  τ-.
  η1     η2
(23)

Substitute τ = 1 + Γ:

η (1 − Γ ) = η (1 + Γ ).
 2           1
(24)

Collect the Γ terms:

η2 − η1 = Γ (η2 + η1).
(25)

Hence

|------------|
Γ =  η2-−-η1.|
|    η2 + η1 |
--------------
(26)

Then

|--------------------|
|            --2η2-- |
τ =  1 + Γ = η  + η .|
--------------1----2--
(27)

These two compact expressions are the normal-incidence Fresnel amplitude coefficients written in impedance form.

5 What the sign of the reflection coefficient means

If

η2 < η1,
(28)

then

Γ < 0.
(29)

The reflected electric field is then reversed in sign relative to the incident electric field at the boundary. For a sinusoid, this is a 180∘ phase reversal.

If

η >  η ,
 2    1
(30)

then

Γ > 0,
(31)

and there is no such sign reversal.

If

|η2 =-η1,|
---------|
(32)

then

|------|
-Γ-=-0.-
(33)

The interface is impedance matched and no plane-wave reflection occurs at normal incidence.

PIC

Figure 2. At normal incidence the reflected and transmitted amplitudes are fixed by continuity of tangential E and H. Reflection occurs when the intrinsic impedances differ.

6 Power reflection and transmission coefficients

The time-averaged power density of a sinusoidal plane wave in a lossless medium is

      |E0|2
⟨S ⟩ = -----.
       2η
(34)

Define the reflected power fraction

     ⟨Sr⟩
R ≡  ----.
     ⟨Si⟩
(35)

Because the incident and reflected waves are in the same medium,

|--------2-|
-R--=-|Γ |.|
(36)

For the transmitted power fraction,

     ⟨St⟩
T ≡  ⟨Si⟩,
(37)

so

     |Et0|2∕(2η2)
T =  ----2------.
     |Ei0|∕(2η1)
(38)

Therefore

|------------|
|T =  η1|τ|2.|
|     η2     |
-------------
(39)

For two lossless media with no absorption at the boundary,

-------------
R +  T = 1. |
-------------
(40)

This is simply energy conservation applied to the interface.

7 Example: air into a dielectric with relative permittivity 4

Let medium 1 be air, approximated as free space,

η1 = η0,
(41)

and let medium 2 be a nonmagnetic lossless dielectric with

𝜖r2 = 4,     μr2 = 1.
(42)

Its intrinsic impedance is

     ∘  μ0--  η0
η2 =    --- = --.
        4𝜖0    2
(43)

Thus

     η0∕2 − η0     1
Γ =  η-∕2-+-η--= − 3,
      0      0
(44)

so

|------------|
-Γ-=-−-0.333.-
(45)

The reflected electric field has one-third the incident amplitude and is phase reversed.

The transmitted electric-field coefficient is

τ = 1 + Γ =  2.
             3
(46)

The reflected power fraction is

|----------------|
|     1          |
|R =  --≈ 0.111. |
------9----------
(47)

The transmitted power fraction is

          (  )
     -η0--  2- 2   8-
T =  η ∕2   3   =  9,
      0
(48)

so

|----------|
T--≈-0.889.-
(49)

Notice the important distinction: τ = 2∕3 is a field-amplitude ratio, not a power ratio.

8 Reflection from a lossy medium

The same normal-incidence amplitude formula remains valid when medium 2 has complex intrinsic impedance:

|----η--−-η--|
Γ =  -2----1.|
-----η2-+-η1--
(50)

Now Γ is generally complex. Its magnitude gives the reflected field-amplitude fraction and its argument gives the reflection phase shift:

Γ = |Γ |eiϕΓ .
(51)

The transmitted wave also attenuates after entering medium 2 because

Et(z) ∝ e−α2z.
(52)

Thus two physically distinct effects must be separated:

------------------------------------------------------------------
boundary   reflection   versus  propagation loss after transmission.|
------------------------------------------------------------------
(53)

For a general lossy medium at normal incidence, the time-average power flux should be computed from

      1            ∗
⟨S⟩ = --Re (E × H  ) ,
      2
(54)

rather than by blindly using the lossless expression |E|2∕(2η) with a complex η.

9 Why refraction occurs at oblique incidence

Now let the incident wave strike the boundary at angle 𝜃i measured from the normal. The reflected and transmitted waves make angles 𝜃r and 𝜃t.

At every point along the interface, the boundary conditions must hold for all time. Therefore the incident, reflected, and transmitted waves must have the same phase variation parallel to the interface. If the interface lies along x, phase matching requires

|------------------------------|
|β  sin 𝜃 = β  sin𝜃  = β  sin 𝜃. |
--1-----i----1----r----2-----t-
(55)

The first equality gives

|--------|
|𝜃  = 𝜃 .|
--r----i-
(56)

The second gives

β  sin 𝜃 =  β sin𝜃 .
  1    i    2     t
(57)

For lossless isotropic media,

β =  nω-,
      c
(58)

so

|------------------|
n1 sin 𝜃i = n2sin 𝜃t.|
--------------------
(59)

This is Snell’s law, obtained directly from electromagnetic phase continuity along the boundary.

PIC

Figure 3. Oblique incidence requires equal tangential phase variation along the interface. This gives 𝜃r = 𝜃i and Snell’s law.

10 TE and TM polarizations at an interface

At oblique incidence, polarization matters because the electric and magnetic fields project differently onto the interface.

10.1 TE polarization

For transverse-electric (TE, or s) polarization, the electric field is perpendicular to the plane of incidence. Applying the tangential E and H boundary conditions gives

|--------------------------|
|       η cos 𝜃 − η cos 𝜃  |
|Γ TE = -2-----i---1-----t.|
--------η2cos-𝜃i +-η1cos-𝜃t-
(60)

The corresponding electric-field transmission coefficient is

|--------------------------|
|       ----2η2-cos𝜃i----- |
|τTE =  η2cos𝜃i + η1cos 𝜃t.|
---------------------------
(61)

10.2 TM polarization

For transverse-magnetic (TM, or p) polarization, the magnetic field is perpendicular to the plane of incidence. The electric-field reflection coefficient is

|--------------------------|
|Γ   =  η2cos-𝜃t −-η1-cos𝜃i.
| TM    η2cos 𝜃t + η1 cos𝜃i|
----------------------------
(62)

The electric-field transmission coefficient is

|--------------------------|
|           2η2 cos𝜃i      |
|τTM =  ------------------.|
--------η2cos-𝜃t +-η1cos-𝜃i-
(63)

At normal incidence,

𝜃i = 𝜃t = 0,
(64)

and both TE and TM reflection coefficients reduce to

     η  − η
Γ =  -2----1.
     η2 + η1
(65)

11 Power coefficients at oblique incidence

For lossless media, the normal component of average power flow is proportional to

    2
|E0-| cos𝜃.
  2η
(66)

Therefore, for either TE or TM polarization,

|--------|
R  = |Γ |2
----------
(67)

and

|-----------------|
|    η1-cos𝜃t- 2  |
T  = η  cos𝜃 |τ|. |
------2-----i-----
(68)

For lossless interfaces,

R +  T = 1.
(69)

The cosine factor appears because the relevant conserved quantity is power crossing the interface, not power along the slanted propagation direction.

12 Brewster angle

A special feature appears for TM polarization. At one incidence angle the numerator of ΓTM can vanish:

Γ TM = 0.
(70)

For nonmagnetic lossless media, this occurs at the Brewster angle

|------------|
tan 𝜃B =  n2.|
----------n1--
(71)

At 𝜃i = 𝜃B, an ideal TM-polarized plane wave has zero reflected amplitude.

For air to glass with

n1 =  1,    n2 = 1.5,
(72)

𝜃B = tan− 1(1.5) ≈ 56.3∘.
(73)

This effect is polarization selective: the TE reflection coefficient does not vanish at the same angle.

13 Critical angle and total internal reflection

Suppose the wave travels from a higher-index medium into a lower-index medium,

n1 > n2.
(74)

Snell’s law requires

sin 𝜃t = n1sin𝜃i.
         n2
(75)

At a sufficiently large 𝜃i, the right side would exceed 1 if interpreted as an ordinary propagating transmitted angle. The limiting incidence angle is the critical angle,

|----------(----)--|
|        −1  n2    |
|𝜃c = sin     ---  .|
-------------n1----
(76)

For

𝜃i > 𝜃c,
(77)

there is no propagating transmitted plane wave carrying power away from the boundary in the usual refracted direction. Instead, the field in medium 2 is evanescent in the normal direction while the reflection magnitude becomes

|--------|
||Γ | = 1.|
---------
(78)

The phase of Γ remains nontrivial even though all time-average normal power is reflected. This phenomenon is total internal reflection.

14 Fresnel reflectance versus angle

For air-to-glass incidence, n1 = 1 and n2 = 1.5. The TE and TM reflection coefficients behave differently as the incidence angle grows. The TM reflectance falls to zero at the Brewster angle, while the TE reflectance rises monotonically toward unity near grazing incidence.

PIC

Figure 4. Fresnel power reflectance for an air-to-glass interface. TM reflection vanishes at the Brewster angle, while both polarizations approach total reflection near grazing incidence.

15 Standing-wave structure on the incident side

When a reflected wave is present, the total electric field in medium 1 is

             −iβ1z       +iβ1z
E1 (z ) = Ei0e     + Er0e     .
(79)

Using

Er0 = Γ Ei0,
(80)

we obtain

|------------------------------|
|           (  −iβ1z     +iβ1z) |
-E1(z)-=-Ei0--e-----+-Γ e-----.-
(81)

The reflected and incident fields interfere, producing spatial maxima and minima. For a lossless medium and fixed |Γ| < 1,

|E |max =  |Ei0|(1 + |Γ |),
(82)

|E |min = |Ei0|(1 − |Γ |).
(83)

Their ratio is

|----------------|
|        1 + |Γ ||
|SWR   = -------.|
---------1-−-|Γ |-
(84)

This same mathematical structure later reappears in transmission-line voltage standing-wave ratio (VSWR). The transmission-line result is not a coincidence: it is another manifestation of forward and backward waves meeting an impedance discontinuity.

16 Several important limiting cases

16.1 Matched boundary

If

η1 = η2,
(85)

then at normal incidence

Γ = 0,     R =  0.
(86)

No reflection occurs even though other material properties may differ.

16.2 Perfect electric conductor

For an ideal perfect electric conductor, the tangential electric field at the surface must vanish. The reflected field therefore cancels the incident tangential electric field at the boundary:

Er0 = − Ei0.
(87)

Hence

|------------|   |-------|
-Γ PEC-=-− 1,|   -R-=--1.|
(88)

This is complete reflection with a 180∘ electric-field phase reversal.

16.3 Very good but finite conductor

A good conductor has a small complex intrinsic impedance compared with free space. Therefore

Γ ≈ − 1,
(89)

but not exactly. A small transmitted field enters the conductor and then decays over the skin depth developed in EM20.

17 The boundary-wave workflow

A reliable interface calculation can be organized as follows:

  1. determine 𝜖, μ, and σ in each medium;
  2. compute γ and η as needed;
  3. identify the incidence angle and polarization;
  4. enforce tangential phase matching to obtain reflection and refraction angles;
  5. apply the appropriate TE or TM Fresnel coefficient;
  6. convert field-amplitude coefficients into power coefficients with the correct impedance and angle factors;
  7. if a transmitted medium is lossy, propagate the transmitted field with e−αz after the interface.

This workflow keeps three distinct physical mechanisms separate:

  • reflection at the boundary;
  • refraction at the boundary;
  • attenuation inside the material

18 Connection to RF systems and antennas

Boundary-wave physics appears throughout RF engineering. Examples include radomes, dielectric antenna substrates, soil and seawater propagation, building penetration, microwave windows, coaxial and waveguide discontinuities, and the transition from an antenna’s near environment into free space.

The reflection coefficient also foreshadows impedance matching in circuit and transmission-line language. At normal incidence,

Γ = η2-−-η1
    η2 + η1
(90)

has exactly the same algebraic form as the voltage reflection coefficient at a transmission-line load,

Γ L = ZL-−--Z0.
      ZL +  Z0
(91)

The common structure arises because both problems enforce continuity relations between paired wave variables and their impedance ratios.

19 What EM21 adds to the series

EM20 described propagation within one uniform medium. EM21 adds the physics of crossing between media. The key results are

|----------------------------|
|    η2 − η1            2η2  |
Γ =  -------,    τ =  -------|
-----η2 +-η1----------η1 +-η2-
(92)

for normal incidence,

|----------|
|        2 |
-R--=-|Γ |,
(93)

|------------------|
n1-sin-𝜃i =-n2sin-𝜃t,-
(94)

and the TE/TM Fresnel coefficients for oblique incidence.

These results establish the mathematical foundation for multilayer propagation, transmission lines, Standing Waves, impedance matching, waveguides, radomes, and antenna-to-medium coupling. The natural companion is an EM21E1 problem set devoted to boundary-condition derivations, Fresnel coefficients, Brewster angle, total internal reflection, and power bookkeeping.

References

References

[1]   D. J. Griffiths, Introduction to Electrodynamics, 4th ed., Cambridge University Press, 2017.

[2]   J. D. Jackson, Classical Electrodynamics, 3rd ed., Wiley, 1999.

[3]   D. K. Cheng, Field and Wave Electromagnetics, 2nd ed., Addison-Wesley, 1989.

[4]   F. T. Ulaby and U. Ravaioli, Fundamentals of Applied Electromagnetics, 7th ed., Pearson, 2015.

[5]   C. A. Balanis, Advanced Engineering Electromagnetics, 2nd ed., Wiley, 2012.

[6]   D. M. Pozar, Microwave Engineering, 4th ed., Wiley, 2012.


"Electromagnetic Waves, Antennas, and RF: Boundary Waves - Reflection, Transmission, and Refraction" is owned by bloftin.
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Other names:  EM21
Also defines:  electromagnetic boundary conditions, electric field reflection coefficient, electric field transmission coefficient, power reflection coefficient, power transmission coefficient, Snell's law, TE polarization, TM polarization, Brewster angle, critical angle, total internal reflection, standing-wave ratio
Keywords:  electromagnetic boundary conditions, reflection, transmission, refraction, intrinsic impedance, reflection coefficient, transmission coefficient, Fresnel equations, Snell law, TE polarization, TM polarization, Brewster angle, critical angle, total internal reflection, standing wave, RF interface

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Electromagnetic Waves, Antennas, and RF: Boundary Waves - Exercises and Complete Worked Solutions (Example) by bloftin

Cross-references: EM21E1, Standing Waves, transmission lines, algebraic, skin depth, voltage standing-wave ratio, average power, flux, magnitude, energy conservation, power, impedance, energy, charge, Gauss's Law, electric field, Electromagnetism, formulas, intrinsic impedance, propagation constant, parameters, Normal, unit, magnetic fields, relation, Maxwell's Equations, Conductor, glass, boundary, electromagnetic wave, EM20
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This is version 3 of Electromagnetic Waves, Antennas, and RF: Boundary Waves - Reflection, Transmission, and Refraction, born on 2026-10-09, modified 2026-10-09.
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Classification:
Physics Classification: 42.25.Gy (Edge and boundary effects; reflection and refraction)
 41.20.Jb (Electromagnetic wave propagation; radiowave propagation )
 42.25.Bs (Wave propagation, transmission and absorption radiation interactions with plasma and 52.38-r Laser-plasma interactions-in pla)
 41.20.-q (Applied classical electromagnetism)
 84.40.-x (Radiowave and microwave technology)

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