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Radiation resistance
Radiation resistance
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Radiation resistance is that part of an antenna's feedpoint electrical resistance caused by the emission of radio waves from the antenna.[a][1][2] A radio transmitter applies a radio frequency alternating current to an antenna, which radiates the energy of the current as radio waves. Because the antenna is absorbing the energy it is radiating from the transmitter, the antenna's input terminals present a resistance to the current from the transmitter.

Radiation resistance is an effective resistance, due to the power carried away from the antenna as radio waves.[1][2] Unlike conventional ohmic resistance, radiation resistance is not an opposition to current (resistivity) of the imperfect conducting materials the antenna is made of. The radiation resistance () is conventionally defined as the value of electrical resistance that would dissipate the same amount of power as heat, as is dissipated by the radio waves emitted from the antenna.[1][3][4] From Joule's law, it is equal to the total power radiated as radio waves by the antenna, divided by the square of the RMS current into the antenna terminals:[4] [b][c]

The feedpoint and radiation resistances are determined by the geometry of the antenna, the operating frequency, and the antenna location (particularly with respect to the ground). The relation between the feedpoint resistance () and the radiation resistance () depends on the position on the antenna at which the feedline is attached.[d][7][1] The relation between feedpoint resistance and radiation resistance is particularly simple when the feedpoint is placed (as usual) at the antenna's minimum possible voltage / maximum possible current point; in that case, the total feedpoint resistance at the antenna's terminals is equal to the sum of the radiation resistance plus the loss resistance due to "Ohmic" losses in the antenna and the nearby soil: When the antenna is fed at some other point, the formula requires a correction factor discussed below. In a receiving antenna the radiation resistance represents the source resistance of the antenna, and the portion of the received radio power consumed by the radiation resistance represents radio waves re-radiated (scattered) by the antenna.[8][9]

Cause

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Electromagnetic waves are radiated by electric charges when they are accelerated.[2][10] In a transmitting antenna, radio waves are generated by time varying electric currents, consisting of electrons accelerating as they flow back and forth in the metal antenna, driven by the electric field due to the oscillating voltage applied to the antenna by the radio transmitter.[11][12] An electromagnetic wave carries momentum away from the electron which emitted it. The cause of radiation resistance is the radiation reaction, the recoil force on the electron when it emits a radio wave photon, which reduces its momentum.[13][14][2] This is called the Abraham–Lorentz force. The recoil force is in a direction opposite to the electric field in the antenna accelerating the electron, reducing the average velocity of the electrons for a given driving voltage, so it acts as a resistance opposing the current.

Radiation resistance and loss resistance

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The radiation resistance is only part of the feedpoint resistance at the antenna terminals. An antenna has other energy losses which appear as additional resistance at the antenna terminals; ohmic resistance of the metal antenna elements, ground losses from currents induced in the ground, and dielectric losses in insulating materials. When the feedpoint is (as usual) at a voltage minimum and current maximum, the total feedpoint resistance is equal to the sum of the radiation resistance and loss resistance

The power fed to the antenna is split proportionally between these two resistances.[1][15]

where

and

The power consumed by radiation resistance is converted to radio waves, the desired function of the antenna, while the power consumed by loss resistance is converted to heat, representing a waste of transmitter power.[1] So for minimum power loss it is desirable that the radiation resistance be much greater than the loss resistance. The ratio of the radiation resistance to the total feedpoint resistance is equal to the efficiency () of the antenna.

To transfer maximum power to the antenna, the transmitter and feedline must be impedance matched to the antenna. This means the feedline must present to the antenna a resistance equal to the input resistance and a reactance (capacitance or inductance) equal but opposite to the antenna's reactance. If these impedances are not matched, the antenna will reflect some of the power back toward the transmitter, so not all the power will be radiated. For "large" antennas, the radiation resistance is usually the main part of their input resistance, so it determines what impedance matching is necessary and what types of transmission line would match well to the antenna.

Effect of the feedpoint

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When the feedpoint is placed at a location other than the minimum-voltage / maximum current point, or if a "flat" voltage minimum does not occur on the antenna, then the simple relation no longer holds.

In a resonant antenna, the current and voltage form standing waves along the length of the antenna element, so the magnitude of the current in the antenna varies sinusoidally along its length. The feedpoint, the place where the feed line from the transmitter is attached, can be located anywhere along the antenna element. Since feedpoint resistance depends on the input current, it varies with the feedpoint.[5] It is lowest for feedpoints located at a point of maximum current (an antinode),[c] and highest for feedpoints located at a point of minimum current, a node, such as at the end of the element (theoretically, in an infinitesimally thin antenna element, radiation resistance is infinite at a node, but the finite thickness of actual antenna elements gives it a high but finite value, on the order of thousands of ohms).[16]

The choice of feedpoint is sometimes used as a convenient way to impedance match an antenna to its feed line, by attaching the feedline to the antenna at a point at which its input resistance happens to equal the feed line impedance.

In order to give a meaningful value for the antenna efficiency, the radiation resistance and loss resistance must be referred to the same point on the antenna, often the input terminals.[17][18] Radiation resistance is by convention calculated with respect to the maximum possible current on the antenna.[5] When the antenna is fed at a point of maximum current, as in the common center-fed half-wave dipole or base-fed quarter-wave monopole, that value is mostly the radiation resistance. However, if the antenna is fed at some other point, the equivalent radiation resistance at that point can easily be calculated from the ratio of antenna currents[16][18]

where and are the electrical lengths (as electrical degrees or radians) from the current node (usually measured from the tip of a linear antenna).

Receiving antennas

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In a receiving antenna, the radiation resistance represents the source resistance of the antenna as a (Thevenin equivalent) source of power. Due to electromagnetic reciprocity, an antenna has the same radiation resistance when receiving radio waves as when transmitting. If the antenna is connected to an electrical load such as a radio receiver, the power received from radio waves striking the antenna is divided proportionally between the radiation resistance and loss resistance of the antenna and the load resistance.[8][9] The power dissipated in the radiation resistance is due to radio waves reradiated (scattered) by the antenna.[8][9] Maximum power is delivered to the receiver when it is impedance matched to the antenna. If the antenna is lossless, half the power absorbed by the antenna is delivered to the receiver, the other half is reradiated.[8][9]

Radiation resistance of common antennas

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In all of the formulas listed below, the radiation resistance is the so-called "free space" resistance, which the antenna would have if it were mounted several wavelengths distant from the ground (not including the distance to an elevated counterpoise, if any). Installed antennas will have higher or lower radiation resistances if they are mounted near the ground (less than 1 wavelength) in addition to the loss resistance from the antenna's near electrical field that penetrates the soil.[d][1]

Antenna type Radiation resistance
(Ω)
Source
Center-fed half-wave dipole 73.1 [e][f] Kraus 1988:227
Balanis 2005:216
Short dipole of length Kraus 1988:216
Balanis 2005:165,215
Base-fed quarter-wave monopole
over a perfectly conducting ground plane
36.5 Balanis 2005:217
Stutzman & Thiele 2012:80
Short monopole of length
over a perfectly conducting ground plane
Stutzman & Thiele 2012:66
Resonant loop antenna, a little over
circumference
~100 Weston 2017:15
Schmitt 2002:236
Small loop of area with turns
(circumference )
Kraus 1988:251
Balanis 2005:238
Small loop of area with turns on a ferrite
core of effective relative permeability
Kraus 1988:259
Milligan 2005:260

The above figures assume the antennas are made of thin conductors and sufficiently far away from large metal structures, that the dipole antennas are sufficiently far above the ground, and the monopoles are mounted over a perfectly conducting ground plane.

The zero thickness half-wave dipole's radiation resistance of 73 Ω (approx. 67 Ω finite thickness) is near enough to the characteristic impedance of common 50 Ω and 75 Ω coaxial cable that it can usually be fed directly without need of an impedance matching network. This is one reason for the wide use of the half wave dipole as a driven element in antennas.[21]

Relationship of monopoles and dipoles

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The radiation resistance of a monopole antenna created by replacing one side of a dipole antenna by a perpendicular ground plane is one-half of the resistance of the original dipole antenna. This is because the monopole radiates only into half the space, the space above the plane, so the radiation pattern is identical to half of the dipole pattern and therefore with the same input current it radiates only half the power.[22]

This is not obvious from the formulas in the table because the different lengths use the same symbol, the derived monopole antenna, however, is only half the length of the original dipole antenna. This can be shown by calculating the radiation resistance of a short dipole (length ), which is twice the length of the corresponding monopole ():

(dipole length ).

Comparing this to the formula for the short monopole shows the dipole has double the radiation resistance of the monopole:

(monopole of length ).

This confirms the consistency of physically modelling a center-fed dipole as two monopoles, placed end-to-end, with adjacent feedpoints.

Calculation

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Calculating the radiation resistance of an antenna directly from the reaction force on the electrons is very complicated, and presents conceptual difficulties in accounting for the self-force of the electron.[2] Radiation resistance is instead calculated by computing the far-field radiation pattern of the antenna, the power flux (Poynting vector) at each angle, for a given antenna current.[23] This is integrated over a sphere enclosing the antenna to give the total power radiated by the antenna. Then the radiation resistance is calculated from the law of conservation of energy, as the resistance the antenna must present to the input current to absorb the radiated power from the transmitter, using Joule's law [b]

Small antennas

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Electrically short antennas, antennas with a length much less than a wavelength, make poor transmitting antennas, as they cannot be fed efficiently due to their low radiation resistance.

At frequencies below 1 MHz the size of ordinary electrical circuits and the lengths of wire used in them is so much smaller than the wavelength, that when considered as antennas they radiate an insignificant fraction of the power in them as radio waves. This explains why electrical circuits can be used with alternating current without losing energy as radio waves.[g]

As can be seen in the above table, for linear antennas shorter than their fundamental resonant length (shorter than 1/ 2  λ  for a dipole antenna, 1/ 4  λ  for a monopole) the radiation resistance decreases with the square of their length;[24] for loop antennas the change is even more extreme, with sub-resonant loops (circumference less than 1  λ  for a continuous loop, or 1/ 2  λ  for a split loop) the radiation resistance decreases with the fourth power of the perimeter length. The loss resistance is in series with the radiation resistance, and as the length decreases the loss resistance only decreases in proportion to the first power of the length (wire resistance) or remains constant (contact resistance), and hence makes up an increasing proportion of the feedpoint resistance. So with smaller antenna size, measured in wavelengths, loss to heat consumes a larger fraction of the transmitter power, causing the efficiency of the antenna to fall.

For example, navies use radio waves of about 15–30 kHz in the very low frequency (VLF) band to communicate with submerged submarines. A 15 kHz radio wave has a wavelength of 20 km. The powerful naval shore VLF transmitters which transmit to submarines use large monopole mast antennas which are limited by construction costs to heights of about 300 metres (980 ft) . Although these antennas are enormous compared to a human, at 15 kHz the antenna height is still only about 0.015 wavelength, so paradoxically, huge VLF antennas are electrically short. From the table above, a 0.015 λ monopole antenna has a radiation resistance of about 0.09 Ohm.

It is extremely difficult to reduce the loss resistance of an antenna to this level. Since the ohmic resistance of the huge ground system and loading coil cannot be made lower than about 0.5 ohm, the efficiency of a simple vertical antenna is below 20%, so more than 80% of the transmitter power is lost in the ground resistance. To increase the radiation resistance, VLF transmitters use huge capacitively top-loaded antennas such as umbrella antennas and flattop antennas, in which an aerial network of horizontal wires is attached to the top of the vertical radiator to make a 'capacitor plate' to ground, to increase the current in the vertical radiator. However this can only increase the efficiency to 50–70% at most.

Small receiving antennas, such as the ferrite loopstick antennas used in AM radios, also have low radiation resistance, and thus produce very low output. However at frequencies below about 20 MHz, where static is pervasive, this is not such a problem, since a weak signal from the antenna can simply be amplified in the receiver without the amplifier's noise adding any appreciable amount to the already substantial noise (N) accompanying the signal (S), keeping the ratio S/N as good (or bad) as before.

Definition of variables

[edit]
Symbol Unit Description
meter (m) Wavelength of radio waves
[none] math constant Pi ≈ 3.14159
[none] Effective relative permeability of ferrite rod in antenna
square meters
(m²)
Area enclosed within the perimeter of a loop antenna
hertz (Hz) Frequency of radio waves
ampere (A) RMS current driven into antenna terminals
ampere (A) Maximum RMS current in antenna element, at point #0
ampere (A) RMS current at an arbitrary point #1 in antenna element
meter (m) Tip-to-tip length of antenna
turns Number of times the loop antenna wire wraps around the perimeter
watt (W) Electric power delivered to antenna terminals
watt (W) Power radiated as radio waves by antenna
watt (W) Power consumed in loss resistances of antenna and the nearby ground
ohm (Ω) Nominal radiation resistance of antenna
ohm (Ω) Equivalent loss resistance of antenna at input terminals
ohm (Ω) Input resistance of antenna
ohm (Ω) Radiation-related resistance at point #0 on antenna (minimum voltage / maximum current)
ohm (Ω) Radiation-related resistance at point #1 on antenna

Footnotes

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See also

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References

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Sources

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Revisions and contributorsEdit on WikipediaRead on Wikipedia
from Grokipedia
Radiation resistance is a key in antenna theory, representing the portion of an antenna's feedpoint resistance attributable to the power radiated as electromagnetic waves rather than dissipated as . It is defined as the hypothetical resistance through which the antenna's input current would need to flow to dissipate an amount of power equal to the total power radiated by the antenna. This concept allows the radiated power PradP_{rad} to be expressed analogously to ohmic power loss as Prad=12I02RrP_{rad} = \frac{1}{2} I_0^2 R_r, where I0I_0 is the magnitude of the input current at the feed point and RrR_r is the radiation resistance in ohms. The value of radiation resistance depends on the antenna's geometry, size relative to the operating λ\lambda, and current distribution along its structure. For a short (Hertzian) with length lλl \ll \lambda, Rr=80π2(lλ)2R_r = 80 \pi^2 \left( \frac{l}{\lambda} \right)^2 ohms, resulting in very low values (e.g., approximately 0.0088 Ω for l=1l = 1 m at 1 MHz). In contrast, a half-wave (l=λ/2l = \lambda/2) has a much higher radiation resistance of about 73 Ω, making it easier to match to standard transmission lines like 50- or 75-Ω cables. For small loop antennas, radiation resistance scales with the fourth power of the loop's circumference relative to λ\lambda, Rr(C/λ)4R_r \propto (C/\lambda)^4; specialized formulas exist for larger loops or those with nonuniform current. Radiation resistance is calculated by integrating the far-field over a enclosing the antenna and equating it to the input power, often using methods or numerical simulations for complex structures. In the total antenna impedance ZA=RA+jXAZ_A = R_A + jX_A, the real part RAR_A comprises the radiation resistance RrR_r plus any loss resistance RLR_L due to ohmic heating in conductors or dielectrics, such that RA=Rr+RLR_A = R_r + R_L. Antenna η\eta is then given by η=RrRA\eta = \frac{R_r}{R_A}, quantifying the fraction of accepted power that is radiated rather than lost as heat; high efficiency requires RrRLR_r \gg R_L, which is desirable for practical designs to minimize power waste and maximize range. Radiation resistance influences , gain, and bandwidth, and techniques like folding or loading are used to adjust it for better in applications from wireless communications to .

Fundamentals

Definition

In antenna theory, radiation resistance, denoted as RradR_{\text{rad}}, is defined as the equivalent resistance that would dissipate the same amount of power as the power actually radiated by the antenna into free space for a given input current. This conceptual resistance allows the radiated power PradP_{\text{rad}} to be expressed analogously to ohmic dissipation using the formula Prad=12I2Rrad,P_{\text{rad}} = \frac{1}{2} I^2 R_{\text{rad}}, where II is the magnitude of the input current at the antenna's feedpoint. The concept of radiation resistance originated in the late 19th century through Heinrich Hertz's experimental demonstrations of electromagnetic waves using dipole antennas in the , which highlighted the power carried away by radiating fields. It was formalized in during the early , particularly through analyses like Brillouin's 1922 work on calculating radiation resistance from source current distributions, building on foundational electromagnetic principles to quantify antenna efficiency. Unlike physical ohmic resistance, radiation resistance is a fictitious that does not correspond to actual material losses but instead represents the portion of input power converted to far-field , as derived from . This theorem relates the power flow through the S=E×H\mathbf{S} = \mathbf{E} \times \mathbf{H} integrated over a closed surface enclosing the antenna, equating the radiated to an effective resistive dissipation without involving heat generation.

Physical Cause

Radiation resistance in antennas originates from the fundamental electromagnetic principle that accelerating electric charges produce propagating electromagnetic waves. In an antenna, time-varying currents cause charges to accelerate, generating dynamic electric and magnetic fields that extend beyond the near vicinity of the structure. These accelerating charges create a disturbance in the surrounding electromagnetic field, where the changing electric fields induce magnetic fields, and vice versa, resulting in self-sustaining transverse waves that carry energy away from the antenna as far-field radiation. Near the antenna, the fields are predominantly reactive, characterized by rather than , with components decaying rapidly (proportional to 1/r³) and magnetic fields similarly non-radiative. This near-field region, typically within distances much less than a (r << λ/2π), does not contribute significantly to net power flow away from the antenna, as the energy oscillates between electric and magnetic forms without net . In contrast, the far-field region (r >> λ/2π) features transverse electromagnetic waves where the electric and magnetic fields are perpendicular to each other and to the direction of propagation, enabling efficient energy transport outward as plane-like waves. This distinction underscores that radiation resistance pertains specifically to the far-field energy loss, not the localized near-field interactions. The , defined as the of the electric and magnetic fields (S = (1/2) Re[E × H*]), quantifies the directional density in the electromagnetic fields, pointing radially outward in the far field to indicate the power radiated per unit area. Integrating the over a closed surface enclosing the antenna yields the total radiated power, which manifests as an effective resistance at the antenna's input terminals, known as radiation resistance (R_rad). This resistance equates the electrical power delivered to the antenna (P = (1/2) I² R_rad) to the power carried away by the far-field waves, effectively modeling the irreversible energy loss due to as an ohmic , despite no actual heat generation in the conductor.

Impedance Components

Radiation Resistance vs. Loss Resistance

In antenna theory, radiation resistance, denoted as RrR_r, represents the equivalent resistance that accounts for the power radiated by the antenna into space, transforming into electromagnetic waves. This resistance is a fictitious but useful , derived from the relationship between the input current at the antenna terminals and the total radiated power, such that the radiated power is Prad=12I02RrP_{\text{rad}} = \frac{1}{2} |I_0|^2 R_r, or equivalently, Rr=2PradI02R_r = \frac{2 P_{\text{rad}}}{|I_0|^2}, where PradP_{\text{rad}} is the radiated power and I0I_0 is the magnitude of the input current at the feed point. In contrast, loss resistance, denoted as RLR_L, encompasses all non-radiative dissipative losses in the antenna system, primarily due to ohmic heating in the conducting elements, dielectric materials, or ground planes. These losses convert input power into heat rather than useful radiation, arising from the finite conductivity of materials and imperfections in the antenna structure. Unlike RrR_r, which contributes positively to the antenna's function by enabling power transfer to the far field, RLR_L introduces inefficiency, reducing the overall performance of the antenna. The key distinction between these resistances lies in their impact on power handling: RrR_r facilitates the desired radiation process, while RLR_L represents parasitic energy dissipation that degrades system . Antenna radiation , η\eta, quantifies this by measuring the ratio of radiated power to total power accepted by the antenna, given by η=RrRr+RL\eta = \frac{R_r}{R_r + R_L} This highlights how a high RrR_r relative to RLR_L yields near-unity , as seen in well-designed structures where losses are minimized through high-conductivity materials; conversely, elevated RLR_L from poor conductors or suboptimal dielectrics can drop η\eta significantly, limiting and signal strength in practical applications. The total input resistance of an antenna is simply the sum Rin=Rr+RLR_{\text{in}} = R_r + R_L, integrating these components into the broader impedance model.

Total Input Resistance

The total input resistance of an antenna, denoted as RinR_{in}, forms the real part of its input impedance Zin=Rin+jXinZ_{in} = R_{in} + j X_{in}, where it equals the sum of the radiation resistance RrR_r and the loss resistance RLR_L: Rin=Rr+RL.R_{in} = R_r + R_L. This combination represents the resistive components that govern power dissipation and radiation at the antenna terminals. The value of RinR_{in} critically influences impedance matching between the antenna and the feeding transmission line or transceiver. For optimal power transfer, the source impedance must conjugate match ZinZ_{in}, but high or mismatched RinR_{in} (e.g., exceeding 50–75 ohms in many systems) necessitates matching networks like transformers or stubs to minimize reflections and maximize efficiency. In real-world scenarios, proximity to nearby objects—such as metallic surfaces, human tissue, or enclosures—can alter RinR_{in} through electromagnetic , detuning the basic Rr+RLR_r + R_L split and introducing additional resistive loading. Electromagnetic simulation tools, including and statistical modeling approaches, allow precise prediction of these effects by incorporating environmental geometries, enabling design adjustments for robust performance.

Key Influences

Feedpoint Effects

The position of the feedpoint on an antenna plays a critical role in determining its radiation resistance, as this value is defined relative to the current at the feedpoint for a given radiated power. When the feedpoint is located at a voltage maximum—where the input current is relatively low—the radiation resistance is higher compared to placement at a current maximum, where the input current is larger. This occurs because radiation resistance is proportional to the square of the maximum current in the antenna's distribution divided by the square of the feedpoint current; a lower feedpoint current amplifies the effective resistance for the same total radiated power. In a half-wave , for instance, the center feedpoint coincides with the current maximum, resulting in a radiation resistance of approximately 73 Ω. Shifting the feedpoint off-center, such as to about one-third of the length from one end in an (OCFD), increases the radiation resistance to around 200–300 Ω due to the reduced current at that position relative to the antenna's peak current. This higher resistance aids with certain transmission lines, like 300-Ω , and enables broader bandwidth across multiple bands by reducing the Q-factor of the , although it may introduce minor asymmetry in the . The physical design of the feedpoint, including the gap size between the driven elements, further influences the measured radiation resistance. In theoretical models assuming an infinitesimal (delta) gap, the radiation resistance aligns closely with idealized calculations, but a finite gap introduces that perturbs the near-field current distribution, effectively lowering the observed resistance and broadening the impedance bandwidth. For thin-wire dipoles, gaps larger than about 0.01λ can decrease the resistance by 5–10% while enhancing operational bandwidth, as analyzed via the induced (EMF) method. Proper use of a at the feedpoint is essential to isolate the true radiation resistance from measurement artifacts. Without a , unbalanced currents on the feed line can propagate as common-mode signals, increasing loss resistance and distorting the , which may cause the measured radiation resistance to appear lower than actual. A 1:1 , for example, suppresses these currents, ensuring accurate radiation resistance values and stable performance, particularly in configurations where feed-line radiation could otherwise contribute up to 10–20% error in impedance readings. In practical adjustments, such as in a , optimizing the feedpoint location or incorporating a can elevate the radiation resistance to around 300 Ω, improving matching to balanced lines while maintaining efficiency; this ties into broader antenna geometry effects but highlights feedpoint-specific tuning for bandwidth enhancement.

Antenna Geometry and Size

The radiation resistance of an antenna is fundamentally influenced by its , defined as the physical dimension relative to the operating . For electrically small antennas, where dimensions are much less than λ/2, radiation resistance is low and scales proportionally to the square of the electrical length, resulting in inefficient power transfer to radiated fields. As the electrical length increases toward , such as λ/2, radiation resistance rises significantly; a thin half-wave , for example, exhibits a radiation resistance of approximately 73 Ω, enabling efficient radiation comparable to a matched load. Antenna geometry plays a critical role in determining radiation resistance through the distribution of currents and the resulting . Linear geometries, such as , generally yield higher radiation resistance than closed-loop geometries of comparable electrical size, as the linear current flow produces a more uniform azimuthal pattern that efficiently couples power to far-field radiation. In contrast, small loop antennas, with their magnetic -like behavior, exhibit much lower radiation resistance—often orders of magnitude smaller than that of a —for similar dimensions, due to the concentrated and toroidal that limits total radiated power. Advancements have leveraged and geometries to enhance radiation resistance in compact designs, addressing limitations of traditional small antennas. structures, such as Koch or Hilbert curves, increase the effective within a reduced physical by introducing self-similar iterations that extend current paths, thereby elevating radiation resistance closer to resonant values without proportional size increase; for instance, monopoles demonstrate radiation resistances comparable to larger Euclidean counterparts while maintaining miniaturization. integrations, including split-ring resonators loaded onto electrically small dipoles, further boost radiation resistance by tailoring local electromagnetic responses to amplify near-field currents and improve , achieving up to several times higher values in sub-wavelength structures for applications like sensors.

Applications by Antenna Type

Transmitting Antennas

In transmitting antennas, radiation resistance RradR_{\text{rad}} represents the portion of the antenna's that accounts for the power converted into radiated electromagnetic waves, directly determining the maximum radiated power for a given feedpoint current. The radiated power is given by Prad=12I02RradP_{\text{rad}} = \frac{1}{2} |I_0|^2 R_{\text{rad}}, where I0I_0 is the magnitude of the current at the antenna terminals. This relationship underscores the importance of RradR_{\text{rad}} in achieving high , as higher values allow more input power to be converted to useful radiated output rather than being dissipated elsewhere. For instance, a half-wave exhibits Rrad73ΩR_{\text{rad}} \approx 73 \, \Omega, enabling efficient transmission when properly matched. Design considerations for transmitting antennas often focus on to standard 50 Ω\Omega transmission lines to maximize power transfer and minimize reflections, which can otherwise lead to standing waves and reduced . Antenna systems are engineered such that the total input resistance, including RradR_{\text{rad}}, aligns closely with the of cables or waveguides, typically through tuning networks or element adjustments. This matching ensures that the voltage standing wave ratio (VSWR) remains low, typically below 2:1, optimizing the fraction of transmitter power that reaches the antenna. In practice, deviations in RradR_{\text{rad}} due to environmental factors or shifts necessitate adaptive matching to maintain across operating bands. Historically, early radio transmitting antennas, such as those developed by in the late 1890s, often featured low RradR_{\text{rad}} because they were electrically short compared to the operating wavelengths, necessitating high voltages to achieve sufficient current and radiated power. Marconi's vertical wire antennas, elevated on masts up to 61 meters with top loading, suffered from low due to this mismatch, requiring spark-gap transmitters with high voltages up to 150 kV to bridge transatlantic distances. These challenges highlighted the need for larger structures or loading techniques to boost RradR_{\text{rad}}, influencing subsequent antenna evolution for reliable long-range transmission. In contrast to receiving antennas, where RradR_{\text{rad}} primarily affects induced voltage sensitivity, transmitting applications prioritize it for output power scaling.

Receiving Antennas

In receiving antennas, the radiation resistance RradR_\mathrm{rad} plays a crucial role analogous to its function in transmission, but interpreted through the lens of power absorption from incident electromagnetic fields. According to the , the , including RradR_\mathrm{rad}, remains identical whether the antenna operates in transmit or receive mode, provided the medium is linear, isotropic, and reciprocal. In receive mode, RradR_\mathrm{rad} models the portion of the antenna's Thevenin equivalent resistance that corresponds to the power extracted from the incoming wave, representing the re-radiation capability if the antenna were to transmit. This equivalence ensures that the antenna's directional properties and are symmetric across modes. The effective area AeA_e of a receiving antenna quantifies its ability to capture power from an incident and directly incorporates RradR_\mathrm{rad} to account for reception efficiency. It is given by Ae=λ2G4π,A_e = \frac{\lambda^2 G}{4\pi}, where λ\lambda is the and GG is the antenna gain in the direction of the incident wave; the gain G=ηDG = \eta D, with radiation efficiency η=Rrad/Rin\eta = R_\mathrm{rad} / R_\mathrm{in} (where RinR_\mathrm{in} is the total input resistance including losses) and DD the . For a matched load, the maximum receivable power PrecP_\mathrm{rec} is then Prec=AeSP_\mathrm{rec} = A_e S, with SS being the power density of the incident field; high RradR_\mathrm{rad} relative to losses thus enhances sensitivity in applications like . In modern low-noise receivers, particularly those employing cryogenic cooling post-2010, RradR_\mathrm{rad} takes on added significance as an equivalent noise resistance. When receiver components are cooled to near-absolute (e.g., using InP HEMT or SiGe amplifiers in radio telescopes), ohmic losses are minimized, making the thermal noise from RradR_\mathrm{rad} — equivalent to Johnson-Nyquist noise at the antenna temperature TAT_A — the dominant contribution. This noise, v2=4kTARradΔf\langle v^2 \rangle = 4 k T_A R_\mathrm{rad} \Delta f, arises from the antenna's interaction with environmental or cosmic microwave background radiation, setting the fundamental sensitivity limit. Advancements in cryogenic systems, such as those integrated into the Atacama Large Millimeter/submillimeter Array (ALMA) receivers, have achieved system noise temperatures below 10 K, where RradR_\mathrm{rad}-induced noise equivalence enables detection of faint signals from distant astrophysical sources.

Common Configurations

Dipoles and Monopoles

antennas, particularly the half-wave , serve as foundational configurations for understanding radiation resistance in antenna . A half-wave consists of two collinear conductive elements, each of length λ/4, where λ is the , fed at the center. The radiation resistance of a center-fed half-wave in free space is approximately 73 Ω. This value represents the equivalent resistance that would dissipate the same power as the antenna radiates, assuming a thin wire approximation (wire radius much smaller than λ). The derivation of this radiation resistance involves calculating the total radiated power by integrating the far-field over a closed spherical surface enclosing the antenna. For a sinusoidal current distribution along the , I(z) = I_m cos(πz/λ), the far-field components are derived from the , leading to the power expression P_rad = (73.1) I_m² / 2 watts, where I_m is the maximum current at the feedpoint. Equating this to the input power P_in = (1/2) I_m² R_rad yields R_rad ≈ 73 Ω. Monopole antennas, often implemented as a quarter-wave element over a , exhibit radiation resistance closely related to that of the through the image principle. A quarter-wave monopole, with length λ/4 and mounted on an infinite perfect conducting , has a radiation resistance of approximately 36.5 Ω at the base feedpoint. This is exactly half the value of the corresponding half-wave because the ground plane creates an image that confines radiation to the upper half-space, effectively halving the integrated power while doubling the field intensity in that hemisphere. The monopole's derivation follows from the analysis by applying image theory, where the monopole plus its image forms an equivalent half-wave . The radiated power is thus integrated over the half-space above the , resulting in R_rad = (1/2) R_dipole for the base-fed configuration with sinusoidal current distribution. This interrelationship makes monopoles practical for applications requiring a ground reference, such as vertical antennas in .

Other Standard Antennas

The small , often used in applications requiring compact , exhibits a radiation resistance approximated by Rrad31,200(Aλ2)2ΩR_{\text{rad}} \approx 31{,}200 \left( \frac{A}{\lambda^2} \right)^2 \, \Omega, where AA is the physical area enclosed by the loop and λ\lambda is the . This formula applies to electrically small loops where the is much less than the , resulting in very low resistance values that necessitate careful matching to overcome high loss resistance relative to radiation. Patch antennas, particularly configurations, demonstrate radiation resistance that depends on substrate permittivity, thickness, and feeding technique, with typical values spanning 50-200 Ω for common designs aimed at to standard transmission lines. For instance, edge-fed rectangular patches often yield higher resistance around 200 Ω at , while inset or proximity-coupled feeds can adjust this to lower values near 50 Ω to optimize power transfer and bandwidth. These variations arise from the fringing fields at the patch edges, which dominate the mechanism in planar structures. In Yagi-Uda arrays, the driven element's radiation resistance closely resembles that of an isolated half-wave dipole, approximately 73 Ω, but mutual coupling from adjacent parasitic reflectors and directors modifies the effective input resistance, often reducing it to 20-50 Ω for optimized directional performance. This alteration enhances forward gain while requiring feed adjustments, such as folded dipoles, to achieve practical impedances like 50 Ω.

Special Cases

Small Antennas

Electrically small antennas, characterized by the parameter ka1ka \ll 1 where k=2π/λk = 2\pi / \lambda is the and aa is the radius of the smallest sphere enclosing the antenna, exhibit significantly reduced radiation resistance compared to their resonant counterparts. For a short , the radiation resistance is approximated as Rrad20(ka)2ΩR_{\mathrm{rad}} \approx 20 (ka)^2 \, \Omega. This low value arises from the limited ability of such compact structures to efficiently couple energy to free space, as the near-field dominates over the radiating far-field components. The diminished RradR_{\mathrm{rad}} imposes key trade-offs in performance. It results in a high quality factor QQ, typically scaling as Q1.5(ka)3Q \approx \frac{1.5}{(ka)^3} for ka1ka \ll 1, which confines the antenna's operational bandwidth to a narrow range around . , defined as the ratio of radiated power to input power, also suffers because ohmic losses in the antenna materials become comparable to or exceed the small RradR_{\mathrm{rad}}, leading to substantial dissipative heating unless mitigated. To address the inherent capacitive reactance and achieve , loading techniques—such as inductive coils or capacitive hats—are commonly employed, though these further constrain bandwidth while aiming to preserve . Recent advancements in the have explored superdirective configurations to counteract these limitations without enlarging the antenna size. By arranging elements, such as coupled self-resonant split-ring resonators into dimers, superdirectivity can be achieved with directivities exceeding 4, enhancing effective resistance and through optimized current distributions that excite higher-order modes. For instance, a "CC" configuration of split-ring resonators at approximately 1.85 GHz demonstrates a directivity of 4.65 while maintaining high via magneto-inductive wave propagation. More recent developments as of include miniaturized mechanical antennas, which use vibrating structures to improve resistance and in electrically small volumes, offering potential for biomedical and IoT applications. These -based and mechanical designs leverage near-field coupling or dynamic tuning to boost far-field , offering promising solutions for compact systems in constrained environments.

Electrically Short Antennas

Electrically short antennas, defined as those with physical dimensions much smaller than the operating (typically l/λ<0.1l / \lambda < 0.1), exhibit radiation resistance values that scale quadratically with their normalized size, resulting in inherently low without careful design. These antennas are characterized by a predominantly capacitive input reactance due to their inability to support a full quarter- current distribution, necessitating matching networks or loading elements for practical use. The low radiation resistance arises from the limited far-field radiation, as the near-field stored dominates, leading to high quality factors and narrow bandwidths. For the canonical case of a short dipole antenna of total length lλl \ll \lambda with a triangular current distribution, the radiation resistance is approximated as Rrad=20π2(lλ)2Ω.R_{\text{rad}} = 20 \pi^2 \left( \frac{l}{\lambda} \right)^2 \, \Omega. This formula derives from integrating the far-field contributions over the antenna length, assuming a linearly varying current from maximum at the center to zero at the ends, which reduces the effective radiating current compared to a uniform distribution. For example, at l/λ=0.05l / \lambda = 0.05, Rrad0.49ΩR_{\text{rad}} \approx 0.49 \, \Omega, illustrating the rapid decrease as size shrinks. The associated reactance is highly negative (capacitive), approximated as X492ln(l2a)l/λΩX \approx -\frac{492 \ln \left( \frac{l}{2a} \right)}{l / \lambda} \, \Omega where aa is the wire radius (typically on the order of thousands of ohms for thin wires and l/λ0.05l / \lambda \sim 0.05), requiring inductive tuning to achieve resonance and acceptable matching to typical 50-Ω systems. A common practical implementation for electrically short antennas is the base-loaded monopole, where an inductive coil at the base compensates for the capacitive reactance while slightly enhancing the radiation resistance by promoting a more uniform current distribution along the height hh. For an unloaded short monopole over a perfect , Rrad40π2(h/λ)2ΩR_{\text{rad}} \approx 40 \pi^2 (h / \lambda)^2 \, \Omega, but base loading can increase this value by up to 20-50% depending on the coil and , though it remains fundamentally low (e.g., below 10 Ω for h/λ<0.1h / \lambda < 0.1) due to the constrained effective . This enhancement occurs because the loading reduces current taper toward the top, increasing the average squared current that contributes to radiated power, yet the overall is still limited by ohmic losses in the coil and conductor. Such configurations are prevalent in applications like AM radio broadcast towers or portable devices, where physical constraints demand compact vertical radiators. Practical designs of electrically short antennas are further bounded by the Chu-Harrington limit, which establishes a fundamental minimum on the antenna's radiation quality factor Qmin1.5(ka)3+1.5kaQ_{\min} \approx \frac{1.5}{(ka)^3} + \frac{1.5}{ka} for an antenna enclosed in a of aa (where k=2π/λk = 2\pi / \lambda), with the cubic term dominating for ka1ka \ll 1. This limit implies that as size decreases, the stored non-radiating energy relative to radiated energy increases dramatically, leading to low radiation resistance and high sensitivity to losses, thereby preventing super-efficient operation without proportional increases in size or acceptance of narrow bandwidths. For instance, achieving better than 50% efficiency in a highly compact antenna often requires lossless materials and precise tuning, but the limit caps the efficiency-bandwidth product, guiding designers away from unattainable "super-gain" solutions.

Computation

Calculation Methods

Radiation resistance, a key parameter in antenna theory, quantifies the portion of an antenna's input power that is radiated as electromagnetic waves, expressed equivalently as the resistance that would dissipate the same power in a lossless circuit. The primary analytical method for its calculation involves integrating the over a closed surface enclosing the antenna, typically a large in the far field, to determine the total radiated power PradP_{rad}. This power is related to the antenna's input current II (peak value) by the Rrad=2PradI2R_{rad} = \frac{2 P_{rad}}{|I|^2}, where Prad=12S(E×H)daP_{rad} = \frac{1}{2} \Re \oint_{S} (\mathbf{E} \times \mathbf{H}^*) \cdot d\mathbf{a} and SS is the spherical surface. The induced EMF method provides an alternative analytical approach, particularly for wire antennas like dipoles, by assuming a prescribed current distribution (e.g., sinusoidal for thin dipoles) and computing the self-impedance from the interaction between the antenna's and its own current. In this method, the input voltage VinV_{in} is the negative of the tangential along the antenna, Vin=l/2l/2Ez(z)I(z)dz/IinV_{in} = -\int_{-l/2}^{l/2} E_z(z') I(z') \, dz' / I_{in}, yielding the impedance Zin=Vin/IinZ_{in} = V_{in} / I_{in}, whose real part is the radiation resistance for lossless structures. This technique is accurate for thin antennas with length-to-diameter ratios exceeding 100 and relies on closed-form expressions involving integrals for the field components. For complex geometries where analytical solutions are infeasible, numerical methods such as the method of moments (MoM) and finite-difference time-domain (FDTD) are employed to solve integral or differential forms of , respectively, enabling computation of currents, fields, and thus radiation resistance. MoM discretizes the antenna into segments, solves for current coefficients via matrix equations, and extracts RradR_{rad} from the real part of the input impedance, making it efficient for wire and surface structures. FDTD, in contrast, simulates time-domain wave propagation on a grid, suitable for broadband analysis of arbitrary shapes, with RradR_{rad} obtained post-processing the far-field Poynting flux or impedance via . Analytical methods remain preferred for canonical cases like half-wave dipoles, where Rrad73ΩR_{rad} \approx 73 \, \Omega. Recent advancements as of 2025 incorporate to accelerate electromagnetic solvers, providing rapid approximations of radiation resistance without full numerical simulations. For instance, models trained on datasets from traditional solvers can predict RradR_{rad} for antennas with high accuracy, reducing time for iterations. GPU-accelerated frameworks further enable -optimized simulations of complex antennas, integrating with tools like open-source EM software for efficient parameter sweeps.

Variable Definitions

In antenna theory, the radiation resistance, denoted as R\radR_{\rad}, represents the equivalent resistance at the antenna feedpoint that accounts for the power radiated into space as electromagnetic waves. It is defined through the relation P\rad=12I02R\radP_{\rad} = \frac{1}{2} |I_0|^2 R_{\rad}, where P\radP_{\rad} is the time-averaged total radiated power and I0I_0 is the peak magnitude of the complex input current at the antenna terminals. This notation assumes a sinusoidal time-harmonic excitation, with R\radR_{\rad} expressed in ohms (Ω\Omega). The input current I0I_0 is measured in amperes (A) and typically refers to the peak value rather than the root-mean-square (RMS) value. The factor of 12\frac{1}{2} in the power equation arises from time-averaging the instantaneous power over one period of the sinusoid; equivalently, using the RMS current I\rms=I02I_{\rms} = \frac{|I_0|}{\sqrt{2}}
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