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Electromagnetic Waves, Antennas, and RF: Antenna Directivity, Radiation Efficiency, Gain, EIRP, and Effective Aperture

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Electromagnetic Waves, Antennas, and RF: Antenna Directivity, Radiation Efficiency, Gain, EIRP, and Effective Aperture

EM23 derived the radiation field of a Hertzian dipole and showed that a localized time-varying current distribution launches electromagnetic power into different directions with different strengths. EM24 now turns that radiation pattern into the antenna quantities used throughout RF engineering: directivity, radiation efficiency, gain, equivalent isotropically radiated power, and effective aperture. The central objective is to connect every one of these quantities back to electromagnetic power flow rather than treat them as isolated link-budget definitions [1, 2, 3, 4].

The central chain is

|---------------------------------------------------------|
E, H  −→  ⟨S⟩ −→  U (𝜃,ϕ) −→  D − →  G − → EIRP   −→  Ae. |
-----------------------------------------------------------
(1)

The final result,

|--------2-|
Ae =  G-λ-,|
-------4π---
(2)

will be derived first for the Hertzian dipole and then generalized using antenna reciprocity. This relation is the missing bridge between a transmitting antenna’s directional gain and a receiving antenna’s ability to intercept power. EM25 will use it to derive the Friis transmission equation and free-space path loss.

1 Radiation intensity revisited

In the far field, the time-average Poynting vector is approximately radial,

⟨S⟩ ≈ ˆr⟨Sr⟩.
(3)

Because a radiated field amplitude decreases as 1∕r, its power density decreases as 1∕r2. It is therefore useful to remove this purely geometric spreading by defining the radiation intensity

|------------------------|
|U (𝜃, ϕ) = r2⟨Sr(r,𝜃,ϕ)⟩.|
-------------------------
(4)

Its units are watts per steradian,

[U ] = W/sr.
(5)

The total radiated power is obtained by integrating over solid angle:

|-------∫--------------|
|                      |
|Prad =    U (𝜃,ϕ )dΩ. |
---------4π------------
(6)

With spherical coordinates,

dΩ = sin𝜃 d𝜃 dϕ,
(7)

so

       ∫    ∫
         2π   π
Prad =         U (𝜃,ϕ) sin 𝜃d𝜃 dϕ.
        0    0
(8)

An isotropic radiator is the reference source that distributes the same power equally into every direction. Its radiation intensity is therefore

|------------|
|U   =  Prad.|
--iso----4π---|
(9)

PIC

Figure. Directivity compares the actual radiation intensity in a selected direction with the intensity that an isotropic radiator would produce if it radiated the same total power.

2 Directivity

The directional directivity is defined as

|--------------------------------|
|D (𝜃,ϕ) = U-(𝜃,ϕ-)=  4πU-(𝜃,ϕ). |
-------------Uiso--------Prad-----|
(10)

Directivity is dimensionless. It measures only how the radiated power is distributed in angle. It does not yet penalize Conductor loss, dielectric loss, or other dissipative mechanisms inside the antenna.

The maximum directivity is

|----------------|
|D    =  4πUmax-.|
| max     Prad   |
------------------
(11)

Antenna values are often expressed logarithmically relative to an isotropic radiator:

|------------------|
-DdBi-=-10-log10D.-|
(12)

The suffix dBi means decibels relative to an ideal isotropic radiator.

3 Beam solid angle

Let the normalized power pattern be

           U-(𝜃,ϕ)
Pn (𝜃,ϕ) =  U     .
              max
(13)

Then

            ∫
Prad = Umax     Pn(𝜃,ϕ) dΩ.
             4π
(14)

Define the beam solid angle

|------∫---------------|
|                      |
|ΩA  =     Pn(𝜃,ϕ) dΩ. |
--------4π-------------
(15)

Substituting into the maximum-directivity definition gives

         4πUmax
Dmax  =  -------,
         UmaxΩA
(16)

so

|------------|
|D    =  4π-.|
--max----ΩA---
(17)

This expression captures the physical idea of directivity: a pattern concentrated into a smaller solid angle has a larger peak directivity.

4 Example: Hertzian-dipole directivity

EM23 found the normalized power pattern of a Hertzian dipole,

Pn(𝜃) = sin2 𝜃.
(18)

Therefore

ΩA = ∫ 02π ∫ 0π sin 2𝜃 sin 𝜃 d𝜃 dϕ (19)
= 2π ∫ 0π sin 3𝜃 d𝜃. (20)

Using

∫  π
    sin3 𝜃 d𝜃 = 4,
  0            3
(21)

we obtain

Ω  =  8π-.
 A     3
(22)

Hence

|------------------------|
|         4π     3       |
Dmax  =  -----=  --= 1.5.|
---------8π∕3----2--------
(23)

In logarithmic form,

|----------------|
Dmax  = 1.76 dBi.|
------------------
(24)

This value describes angular concentration only. An ideal Hertzian dipole is being treated as lossless here.

5 Radiation efficiency

A real antenna may accept power at its terminals without radiating all of it. Let

Pacc
(25)

be the time-average power accepted by the antenna terminals. This power is divided into radiated power and dissipative loss,

P   = P    + P   .
 acc    rad    loss
(26)

The radiation efficiency is

|------------|
|       P    |
|ηrad =  -rad.|
--------Pacc-
(27)

Therefore

0 ≤  ηrad ≤ 1.
(28)

For a simple equivalent circuit containing radiation resistance Rrad and loss resistance Rloss in series,

       1
Prad = --|I |2Rrad,
       2
(29)

Ploss = 1-|I |2Rloss,
       2
(30)

so

|-------------------|
η   =  ----Rrad---. |
|rad   Rrad + Rloss  |
---------------------
(31)

This makes the difficulty of electrically small antennas visible. If Rrad becomes very small while conductor and matching-network losses remain finite, the radiation efficiency can fall sharply.

6 Gain

Directivity normalizes radiation intensity by the power actually radiated. Gain instead normalizes by the power accepted at the antenna terminals:

|--------------------|
G (𝜃,ϕ) =  4πU-(𝜃,ϕ).|
|            Pacc    |
----------------------
(32)

Using

          4πU (𝜃,ϕ)
D (𝜃, ϕ) = ----------
             Prad
(33)

and

ηrad =  Prad,
       Pacc
(34)

we obtain

|----------------------|
|G (𝜃,ϕ) = ηradD (𝜃,ϕ ).|
-----------------------
(35)

Thus directivity answers

|-----------------------------------|
Where  does the radiated power  go? |
------------------------------------
(36)

while gain answers

|------------------------------------------------------------------|
How   much radiation intensity is produced per accepted input watt? |
--------------------------------------------------------------------
(37)

Maximum gain is usually quoted in dBi:

|------------------|
|GdBi = 10 log  G. |
--------------10---
(38)

PIC

Figure. Accepted terminal power is first reduced by dissipative antenna losses; the remaining radiated power is then distributed directionally. Gain combines radiation efficiency and directivity.

7 Mismatch and realized gain

The gain defined above uses power accepted by the antenna. If a source delivers incident power toward an antenna port with reflection coefficient ΓA, the accepted fraction is

1 − |Γ A|2.
(39)

A useful quantity that includes this mismatch is the realized gain,

|------------------------|
|Grealized = (1 − |Γ A|2)G.|
-------------------------
(40)

The distinction matters in practical link budgets:

|----------------------------------|
|directivity ⁄= gain ⁄= realized gain. |
-----------------------------------
(41)

Cable and feed losses before the antenna are normally accounted for separately unless they have explicitly been included in the quoted system gain.

8 Equivalent isotropically radiated power

Suppose an antenna accepts transmit power Pacc and has directional gain G(𝜃,ϕ). In its far field,

          PaccG(𝜃,ϕ-)
U(𝜃,ϕ ) =     4π     .
(42)

Therefore the power density at range r is

|------------------------|
|S(r,𝜃,ϕ ) = PaccG(𝜃,ϕ-).|
----------------4πr2-----|
(43)

The product

|------------------------|
EIRP--(𝜃,ϕ)-=-PaccG-(𝜃,ϕ)-
(44)

is the equivalent isotropically radiated power: the power an isotropic radiator would need in order to produce the same far-field power density in that direction.

In logarithmic units,

|----------------------------|
-EIRPdBW---=-Pacc,dBW-+--GdBi.-
(45)

If cable, filter, or connector loss Lfeed,dB lies between the transmitter and antenna, a common system form is

|--------------------------------------|
|EIRPdBW   = Ptx,dBW − Lfeed,dB + GdBi. |
---------------------------------------
(46)

For free-space propagation, the corresponding RMS electric-field magnitude is

    E2rms
S =   η0 .
(47)

Substituting

     EIRP
S  = ----2-
      4πr
(48)

gives

       1∘  η-EIRP---
Erms = --  -0------.
       r      4π
(49)

Because

-η0 ≈ 30,
4 π
(50)

we obtain the useful free-space relation

|-------√----------|
|       --30-EIRP--|
Erms ≈      r     .|
--------------------
(51)

Here EIRP is in watts, r in meters, and the result is in volts per meter.

9 Example: efficiency, gain, and EIRP

Consider an antenna with maximum directivity

Dmax = 10
(52)

and radiation efficiency

η   =  0.75.
 rad
(53)

The maximum gain is

Gmax = (0.75)(10) = 7.5.
(54)

In dBi,

Gmax,dBi = 10 log10(7.5) ≈ 8.75 dBi.
(55)

If the antenna accepts

Pacc = 20 W,
(56)

then

|------------------------------|
|EIRPmax  = (20)(7.5) = 150 W. |
--------------------------------
(57)

This does not mean the antenna radiates 150 W of total power. The total radiated power is only

Prad = ηradPacc = 15 W.
(58)

The larger EIRP expresses directional concentration relative to an isotropic radiator.

10 Receiving antennas and effective aperture

Now reverse the problem. Let a plane wave with time-average power density

Sinc
(59)

arrive at a receiving antenna from some direction. The antenna produces electrical power at its terminals. For conjugate load matching and matched polarization, define the effective aperture by

|-----P----|
|Ae = --av,|
------Sinc--
(60)

where Pav is the maximum available receive power.

Therefore

|-------------|
Pav-=-SincAe.--
(61)

Although Ae has units of square meters, it is not necessarily the literal geometric shadow of the antenna. A wire antenna may have negligible physical cross-sectional area yet possess a finite effective aperture.

PIC

Figure. Effective aperture converts incident electromagnetic power density into maximum available terminal power. It is an electromagnetic receiving property, not simply the antenna’s physical silhouette.

11 The receive effective length

A receiving antenna can also be characterized by an effective length vector he. The open-circuit terminal voltage is

|--------------|
Voc-=-Einc-⋅ he.
(62)

For an ideal Hertzian dipole oriented parallel to the incident Electric Field at broadside,

|-------|
he-=-ℓ,--
(63)

so

Voc = E ℓ.
(64)

Here E is the peak phasor magnitude, consistent with the phasor convention used in EM23.

If the antenna input impedance is purely resistive at Resonance,

ZA =  RA,
(65)

and a conjugate matched load is connected, the load voltage amplitude is V oc∕2. The maximum time-average delivered power is therefore

|------------|
|      |Voc|2-|
Pav =  8R   .|
----------A---
(66)

For an ideal lossless Hertzian dipole,

RA  = Rrad.
(67)

12 Deriving the effective aperture of a Hertzian dipole

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

|------------|
|       |E-|2 |
|Sinc = 2 η .|
-------------
(68)

For the broadside, polarization-matched Hertzian dipole,

Voc = E ℓ,
(69)

so

      |E |2ℓ2
Pav = ------ .
       8Rrad
(70)

Hence

Ae = Pav-
Sinc (71)
= |E |2ℓ2∕ (8R    )
-----2----rad-
  |E| ∕(2η) (72)
=  ηℓ2
4R----
  rad. (73)

EM23 derived the radiation resistance of the ideal current element in a lossless medium,

       ηk2-ℓ2
Rrad =   6π  .
(74)

Substituting gives

Ae =   2
ηℓ--
 4--6π--
ηk2 ℓ2 (75)
= 3π
--2-
2k. (76)

Using

    2π-
k =  λ ,
(77)

we obtain

|----------------------------------------|
|         3λ2                            |
|Ae,max =  ----    (ideal Hertzian dipole).|
----------8π------------------------------
(78)

But EM23 also found

        3
Dmax =  -.
        2
(79)

Therefore

Dmax λ2    (3 ∕2)λ2   3λ2
--------=  --------= ----.
  4π         4π       8π
(80)

Thus the transmit directivity and receive effective aperture satisfy

|----------------|
|         Dmaxλ2-|
Ae,max =    4π   |
------------------
(81)

for the ideal lossless Hertzian dipole.

PIC

Figure. For the Hertzian dipole, receive voltage and maximum available power lead directly to Ae = 3λ2∕(8π). The transmit result D max = 3∕2 then reveals the general λ2∕(4π) normalization.

13 From the Hertzian dipole to the general aperture-gain theorem

For a linear reciprocal antenna, the Lorentz reciprocity theorem implies that the angular and polarization properties used to transmit a field are the same properties that govern reception from that direction [1, 2]. Therefore the directional receive aperture has the same normalized angular dependence as the transmit gain.

For a lossless antenna, the Hertzian result generalizes to

|------------2---------|
|Ae(𝜃,ϕ ) = λ--D(𝜃,ϕ ).|
------------4π---------|
(82)

If the antenna has radiation efficiency less than unity, only the fraction ηrad of the receive-mode electromagnetic power associated with the antenna mode is available at the terminals. Since

G  = ηradD,
(83)

the general matched-polarization, conjugate-match relation becomes

-----------------------
|                   2  |
|Ae (𝜃,ϕ) = G-(𝜃,ϕ)λ-. |
---------------4-π-----|
(84)

At the direction of maximum gain,

|------------------|
|         Gmax λ2  |
|Ae,max = --------.|
-------------4π----
(85)

This is one of the most important antenna relations in RF engineering.

14 Physical meaning of the λ2 factor

At fixed dimensionless gain,

A   ∝ λ2.
  e
(86)

Thus the same 0 dBi receiving antenna has a larger effective area at a lower frequency. This does not violate energy conservation. Gain is a dimensionless statement about angular coupling to a propagating spatial mode, while the transverse spatial scale of that mode grows with wavelength.

Conversely, for a fixed physical aperture whose effective area is nearly fixed, the gain rises approximately as

|-----------|
|    4πAe-  |
G  ≈   λ2 . |
-------------
(87)

This is why a fixed-size dish antenna becomes more directive as frequency increases.

15 Example: effective aperture at GPS L1

For the GPS L1 carrier,

f = 1.57542 GHz.
(88)

The free-space wavelength is approximately

λ =  c-≈  0.1903 m.
     f
(89)

For an antenna with

G =  1    (0 dBi),
(90)

its maximum effective aperture is

Ae = λ2
---
4π (91)
≈ 2.88 × 10−3 m2. (92)

Therefore

|--------------|
Ae--≈-28.8cm2.--
(93)

The effective electromagnetic collection area is much more meaningful than the visible cross-sectional area of a small GNSS antenna.

16 Example: Hertzian-dipole effective aperture

At

f = 300 MHz,
(94)

the wavelength is approximately

λ ≈ 1.00 m.
(95)

For the ideal Hertzian dipole,

Gmax =  Dmax =  1.5.
(96)

Hence

Ae,max =            2
(1.5)(1.00-)-
     4π (97)
≈ 0.119 m2. (98)

So an electrically tiny ideal current element can possess an effective aperture of order a tenth of a square meter at a one-meter wavelength. Effective aperture is a coupling area, not a literal metal area.

17 Polarization mismatch

EM19 showed that a receiving antenna need not be polarization matched to the incident wave. If the normalized incident polarization vector is ei and the receive polarization vector is er, the polarization loss factor is

|---------∗----2-|
PLF--=--|^e-r ⋅^ei|-.
(99)

The available receive power becomes

|------------------|
-Pav-=-SincAePLF.--|
(100)

For two linearly polarized antennas misaligned by angle ψ,

PLF  = cos2ψ.
(101)

Thus effective aperture should normally be interpreted as the aperture under matched-polarization conditions unless a polarization factor is stated separately.

18 Physical aperture and aperture efficiency

For aperture antennas such as horns, reflectors, or planar arrays, it is useful to compare effective aperture with physical aperture Aphys. Define the aperture efficiency

|------------|
|      -Ae---|
|ηap = A    .|
--------phys--
(102)

Then

Ae = ηapAphys.
(103)

Combining this with the aperture-gain theorem gives

|----------------|
|       4-πAphys |
G  = ηap   λ2   .|
------------------
(104)

For a circular aperture of diameter Da,

        πD2
Aphys = ---a-,
          4
(105)

so

|--------(-----)---|
|          πDa   2 |
|G = ηap   -λ---  .|
--------------------
(106)

This is the standard scaling behind parabolic-dish antenna gain. The aperture efficiency accounts for illumination taper, spillover, blockage, phase error, polarization effects, and other departures from ideal use of the physical opening.

19 Common conceptual mistakes

  • Directivity is not gain. Directivity ignores dissipative antenna loss; gain includes radiation efficiency.
  • Gain does not create power. A directional antenna redistributes radiated power so that some directions have larger radiation intensity than an isotropic reference.
  • EIRP is not total radiated power. EIRP is a directional isotropic-equivalent quantity.
  • Effective aperture is not necessarily geometric area. Wire antennas can have substantial Ae despite very small physical cross section.
  • The Ae relation uses gain, not directivity, for a lossy antenna. Radiation efficiency must be included.
  • Polarization and terminal mismatch still matter. The basic Ae = Gλ2∕(4π) expression assumes the stated gain direction, matched polarization, and the usual available-power definition.
  • Realized gain includes mismatch; ordinary gain does not. Be explicit about which quantity a data sheet quotes.

20 The bridge to the Friis equation

EM17 established spherical power spreading,

      P
S = ----2,
    4πr
(107)

while EM24 has now established the directional transmit form

     P G
S =  -t-t-
     4πr2
(108)

and the receive relation

Pr = SAe,r.
(109)

Using

       Grλ2-
Ae,r =   4π
(110)

immediately gives

            (     )
              -λ--  2
Pr = PtGtGr   4πr    .
(111)

EM25 will derive this carefully, identify the assumptions behind it, and separate the free-space spreading factor from antenna gain, polarization, mismatch, atmospheric loss, and other link-budget terms.

21 Summary

Radiation intensity removes the purely geometric 1∕r2 spreading from far-field power density:

|------------|
|U =  r2⟨Sr⟩.|
-------------
(112)

Directivity compares that intensity with an isotropic radiator having the same total radiated power:

|----------|
D  =  4πU-.|
|     Prad |
------------
(113)

Radiation efficiency measures how much accepted terminal power is actually radiated:

|------------|
|       P    |
|ηrad =  -rad.|
--------Pacc-
(114)

Gain combines the two:

|-----------|
G  = ηradD.  |
-------------
(115)

Equivalent isotropically radiated power is

|---------------|
EIRP  =  PaccG. |
----------------
(116)

Effective aperture connects incident power density to maximum available receive power:

|-------------|
P   = S   A . |
--av-----inc--e--
(117)

Finally, reciprocity connects transmit gain and receive aperture:

|----------------------|
|           G (𝜃,ϕ)λ2  |
|Ae (𝜃,ϕ) = ---------. |
---------------4-π-----
(118)

This identity completes the electromagnetic bridge from radiated fields to received power and prepares the series for Friis transmission, free-space path loss, and RF link budgets.

References

References

[1]   Constantine A. Balanis, Antenna Theory: Analysis and Design, 4th ed., Wiley, 2016.

[2]   Warren L. Stutzman and Gary A. Thiele, Antenna Theory and Design, 3rd ed., Wiley, 2012.

[3]   John D. Kraus and Ronald J. Marhefka, Antennas for All Applications, 3rd ed., McGraw-Hill, 2002.

[4]   IEEE, IEEE Standard for Definitions of Terms for Antennas, IEEE Std 145-2013, 2014.

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


"Electromagnetic Waves, Antennas, and RF: Antenna Directivity, Radiation Efficiency, Gain, EIRP, and Effective Aperture" is owned by bloftin.
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Other names:  EM24
Also defines:  antenna directivity, beam solid angle, radiation efficiency, antenna gain, realized gain, equivalent isotropically radiated power, effective aperture
Keywords:  antenna directivity, radiation intensity, beam solid angle, radiation efficiency, antenna gain, realized gain, EIRP, effective aperture, effective area, receiving antenna, reciprocity, Hertzian dipole, polarization mismatch, aperture efficiency, RF link budget

Attachments:
Electromagnetic Waves, Antennas, and RF: Antenna Directivity, Radiation Efficiency, Gain, EIRP, and Effective Aperture - Exercises and Complete Worked Solutions (Example) by bloftin

Cross-references: identity, EM17, cross section, polarization loss factor, EM19, energy conservation, theorem, Resonance, input impedance, Electric Field, square, magnitude, system, resistance, Conductor, spherical coordinates, solid, units, vector, relation, power, radiation, EM23
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This is version 1 of Electromagnetic Waves, Antennas, and RF: Antenna Directivity, Radiation Efficiency, Gain, EIRP, and Effective Aperture, born on 2026-10-10.
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Physics Classification: 84.40.Ba (Antennas: theory, components and accessories )
 41.20.Jb (Electromagnetic wave propagation; radiowave propagation )
 84.40.-x (Radiowave and microwave technology)
 03.50.De (Classical electromagnetism, Maxwell equations )
 41.20.-q (Applied classical electromagnetism)

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