原创 Fundamentals and design principles of RF antennas

2009-6-19 14:55 2811 7 5 分类: 模拟

Antennas connect RF signals in an electrical circuit, such as between a PCB and an electromagnetic wave propagating in the transmission media between the transmitter and the receiver of a wireless link.

In the transmitter, the antenna transforms the electrical signal into an electromagnetic wave by exciting either an electrical or a magnetic field in its immediate surroundings, the near field. Antennas that excite an electrical field are referred to as electrical antennas; antennas exciting a magnetic field are called magnetic antennas. The oscillating electrical or magnetic field generates an electromagnetic wave that propagates with the velocity of light c. The speed of light in free space co is 300000 km/s. If the wave travels in a dielectric medium with the relative dielectric constant εr, the speed of light is reduced to:





We can calculate the wavelength from the frequency f of the signal and the speed of light c using the formula:





Using common units, the equation:





is often used for the wavelength in free space. If the wave travels in a dielectric medium, for instance in the PCB material, the wavelength has to be divided by the square root of εr. We can distinguish three field regions where the electromagnetic wave develops: reactive near field, radiating near field, and far field:


In the reactive near field, reactive field components predominate over the radiated field. This means that any variations in the electrical properties (for electrical antennas) or magnetic properties (for magnetic antennas) have a strong influence on the antenna's impedance at the antenna feed point. The distance from the antenna to the boundary of the reactive near field region is commonly assumed as:





In the radiating near field, the radiated field predominates, and the antenna impedance is only slightly influenced by the surrounding media in this region. But the dimensions of the antenna cannot be neglected with respect to the distance from the antenna. This means that the angular distribution of the radiation pattern is dependent on the distance. For measurements of the radiation pattern, the distance from the antenna should be larger than the radiating near field boundary, otherwise the measured pattern will be different from that under real life conditions. The diameter of the radiating near field is




with D as the largest dimension of the antenna.


For distances larger than R2, the radiation pattern is independent of the distance, meaning we are in the far field region. In a practical application, the distance between transmitter and receiver antennas is usually in this region.

In the receiver, the antenna gathers energy from the electromagnetic wave and transforms it into an electrical voltage and current in the electrical circuit. For better comprehension, the antenna parameters are often explained on a transmit antenna, but in most cases, if no nonlinear ferrites are involved, the characteristics of an antenna are identical in receive and transmit modes.

Polarized antenna
Polarization describes the trace that the tip of the electrical field vector builds during the propagation of the wave. In the far field, we can consider the electromagnetic wave as a plane wave. In a plane electromagnetic wave, the electrical and the magnetic field vectors are orthogonal to the direction of propagation and also orthogonal to each other. In the general case, the tip of the electrical field vector moves along an elliptical helix, giving an elliptical polarization. The wave is called right-hand polarized if the tip of the electrical field vector turns clockwise while propagating; otherwise it is left-hand polarized.

If the two axis of the ellipse have the same magnitude, the polarization is called circular. If one of the two axes of the ellipse becomes zero, we have linear polarization. Similarly, polarization is vertical if the electrical field vector oscillates perpendicularly to ground, and it is horizontal if its direction of oscillation is parallel to the ground plane.

A transmission system has the best performance (ideal case) when the polarization of the transmitter and the receiver antenna are identical to each other. Circular polarization on one end and linear polarization on the other gives 3dB loss compared to the ideal case. If both antennas are linearly polarized but 90? turned to each other, theoretically no power is received. The same phenomenon happens if one antenna is right-hand circularly polarized and the other one is left-hand circularly polarized.

In an indoor environment, reflections in the transmission path may change the polarization, which makes the polarization of the received wave difficult to predict. If one of the antennas is portable, we have to make sure that it works in any position. Circular polarization at one end and linear polarization at the other end results in a principal loss of 3dB, but avoids the case of a total blackout, where no power is received.

The concept of the isotropic radiator is often used to describe radiated power and antenna gain. The isotropic radiator is a hypothetical antenna, which radiates the supplied RF power equally in all directions. The power density at a distance r from the isotropic radiator is therefore the supplied power divided by the area of a sphere with the radius r.


EEOL_2008FEB18_RFD_NETD_NT.jpg

Figure 1: Isotropic radiator


If we measure the power density in some distance from a device under test, the effective isotropic radiated power (EIRP) is the power which we would have to supply to an isotropic radiator in order to get the same power density in the same distance. The EIRP describes the power radiation capability of a device (including its antenna).

From the EIRP, we can calculate the electrical field strength at a given distance from the radiator, which is specified in some government and regional regulations. The density of the radiated power D (in W/m2) measured in the distance r from an isotropic radiator radiating the total power EIRP is the radiated power divided by the surface area of the sphere with the radius r:




The relationship between the electrical field strength and the power density is the same as between voltage and power in an electrical circuit.

With the impedance of free space Zo = 377? = π 120?, the rms value of the electrical field strength is then:




This gives:




Or:




Taking the logarithm on both sides gives the EIRP value in dBm:

EIRP[dBm]=E[dBV/m]+20 logr[meters]-10-log30-90dB

In standard test setups, the electrical field strength is often measured at a distance of 3 m. In this case we can use the simple formula:

EIRP[dBm] = E[dBV/m] " 95.23dB

As opposed to the hypothetical isotropic radiator, real antennas exhibit more or less distinct directional radiation characteristics. The radiation pattern of an antenna is the normalized polar plot of the radiated power density, measured at a constant distance from the antenna in a horizontal or vertical plane.

The isotropic gain Giso of an antenna indicates how many times the power density of the described antenna in the main direction of propagation is larger than the power density from an isotropic radiator at the same distance. Antenna gain does not imply an amplification of power; it comes only from the bundling of the available radiated power in certain directions.

The radiation resistance (Rr) relates the power radiated from the antenna to the RF current fed into the antenna. For the same RF current, a resistor with the resistance Rr would dissipate exactly the same power into heat that the antenna radiates. Rr can be calculated from:




The radiation resistance is part of the impedance of the antenna at its feed point. Additionally, we have the loss resistance Rloss which accounts for the power dissipated into heat as well as reactive components L and C. Figure 2 has an equivalent circuit that describes the antenna around its resonant frequency.


EEOL_2008FEB18_RFD_NETD_NT1.jpg

Figure 2: Antenna equivalent circuit


The inductor and the capacitor in the equivalent circuit build a series resonant circuit. The antenna impedance Z is:




At the frequency of resonance,




the reactances of the capacitor and the inductor cancel each other out, soonly the resistive part of the antenna impedance remains. The inductance L and the capacitance C in the equivalent schematic are determined by the antenna geometry. If we want to build an antenna for a given frequency, we have to find a geometry that is resonant at the frequency of operation, such as a wire with a certain length.

At the frequency of resonance, the antenna input impedance equals Rr+ Rloss. The antenna efficiency h in resonance is the ratio of the radiated power to the total power accepted by the antenna from the generator:




At frequencies other than the resonant frequency, the antenna input impedance is either capacitive or inductive. This phenomenon is why it is possible to tune an existing antenna by adding a series capacitor or inductor.

The L-to-C ratio determines the bandwidth of the antenna for given radiation and loss resistances. For the same resistance values, a larger L-to-C ratio means a higher quality factor Q and a smaller bandwidth. The values of L and C in the equivalent schematic depend on the antenna geometry.Often we can deduct intuitively how a variation of the geometry can influence L and C. The quality factor is influenced by a contribution Qrad from the radiation resistance and Qloss from the loss resistance. The overall Q of the antenna is:




Chu [1] and Wheeler [2] gave the theoretical limit for the quality factor Q and the fractional bandwidth of a lossless antenna as:




with a as the radius of the smallest circumscribing sphere surrounding the antenna.

The selectivity of the antenna can help to suppress unwanted out-of-band emissions; but not always a small bandwidth is desirable. A small bandwidth means stringent requirements on the tolerances of the matching components and the antenna itself. For a given dimension of a small antenna, we can only increase the bandwidth if we introduce intentional losses. The bandwidth of an antenna with the efficiency ηis then:




The product of the bandwidth and the efficiency is a constant for a given antenna dimension. If we want to gain one, then we have to sacrifice from the other.

Reflect, match, tune
What happens if we connect a transmit antenna to a transmission line with the characteristic impedance Zo (usually 50?) and send a signal with the amplitude VIN into the transmission line?

In most cases, the antenna impedance Z will not be exactly the same as the transmission line impedance Zo. Then only a part of the incident wave will be transmitted to the antenna with an amplitude of Vaccent, while the remaining part will be reflected back to the generator with an amplitude of Vrefl.


EEOL_2008FEB18_RFD_NETD_NT2.jpg

Figure 3: Reflection at a discontinuity


The complex reflection coefficient Γ is defined as the ratio of the reflected wave's amplitude (e.g. voltage, current, or field strength) to the amplitude of the incident wave. We can calculate the reflection coefficient from the impedances of the antenna Z and the transmission line Zo:




For an arbitrary complex load impedance Z, the phase difference between the reflected and the incident wave may be anywhere in the range between 0 and 2π. The reflection coefficient is therefore a complex quantity. If we want to minimize the reflection loss, we must know the magnitude and phase angle of the reflection coefficient, which can be measured with a vector network analyzer. If the source is not a transmission line but the output of an IC, then the source impedance can be a complex quantity. The reflection coefficient is zero if Z equals Zo, the complex conjugate of the source impedance. In this case, all incident energy is accepted by the antenna, so we call the antenna perfectly matched.

The power ratio of the reflected to the incident wave is called the return loss (RL). The RL tells us how many dB the power of the reflected wave is below the power of the incident wave. A perfectly matched antenna has an infinite return loss, because no power is reflected, and all the power is accepted. The power of the accepted wave is smaller than the power of the incident wave by the amount of the mismatch loss (ML). The mismatch loss directly describes the impact of the usually unwanted reflection on the power radiated by the antenna. We can calculate RL and mismatch from the reflection coefficient using the formulas:




If we measure the voltage on a transmission line, we cannot distinguish between the incident and the reflected waves because we can only see the sum of both. At some locations, both waves interfere constructively, and at some other locations they partially cancel out each other.


EEOL_2008FEB18_RFD_NETD_NT3.jpg

Figure 4: Standing waves due to reflection


As we can see from Figure 4, the locations where maximum and minimum in the amplitude of the sum occur do not move. In fact, the incident and the reflected wave build a standing wave. The larger the amplitude of the reflected wave is, the more pronounced the standing wave pattern will be. The voltage standing wave ratio (VSWR) is defined as the ratio of the maximum to the minimum voltage of the standing wave pattern and can be calculated from the magnitude of the reflection coefficient:




The numerical value of VSWR is in the range between 1 (ideally matched load, no standing wave) and ∞ (|Γ| = 1, total reflection or complete mismatch).

VSWR, Γ, RL, and ML describe the same phenomenon of reflection and can be transformed into each other. While VSWR and RL are related to the amplitude of the reflected wave only, Γ contains the phase information too, as Γ is a complex quantity.

Often the antenna has an impedance different from that of the feeding transmission line. To minimize the mismatch loss, we have to transform one impedance to the complex conjugate of the other. A powerful tool that helps to determine the needed matching circuit is the Smith Chart. Basically, the Smith Chart plots the reflection coefficient Γ in the complex plane. For passive circuits, the length of the Γ -phasor varies between 0 (ideal match) and 1 (complete mismatch). The phase difference f between the reflected and the incident wave may assume any value between 0 and 2π. Therefore, all possible Γ-phasors (for passive circuits) are within a circle with the radius 1, which defines the outer boundary of the Smith Chart.

The reflection coefficient is +1 if the end of a transmission line is left open, "1 for a short at the end of the transmission line. An inductive load gives a reflection coefficient in the upper half, and a capacitive load gives one in the lower half of the Smith Chart. Any capacitors or inductors added to a given load move the reflection coefficient in the Smith Chart on circles: series components on a circle that goes through the open point at +1, parallel components on circles through the shortcut point at "1. Inductors shift the reflection coefficient upwards towards the inductive half; capacitors shift it downwards towards the capacitive half. Figure 5 shows how series or parallel inductors and capacitors influence a given reflection coefficient.


EEOL_2008FEB18_RFD_NETD_NT4.jpg

Figure 5: Series and parallel capacitors and Inductors in the Smith chart


Using the Smith Chart, we can find out what kind of components are needed to minimize the reflection coefficient for a given antenna impedance. In Figure 5 for example, a series capacitor could move the reflection coefficient on the circle through the open point (because it is a series component) towards the lower half of the Smith Chart (because it is a capacitor). The center of the Smith Chart (where the reflection coefficient is zero) can be reached by a proper capacitance value giving the perfect match.

For a system environment normalized to 50?, the center of the Smith Chart is 50?.



Antennas connect RF signals in an electrical circuit, such as between a PCB and an electromagnetic wave propagating in the transmission media between the transmitter and the receiver of a wireless link.

The second installment of the 3-part series discusses common antennas including half-wave dipole, quarter wave monopole, transversal mode helical, and small loop antennas.

The half-wave dipole antenna (Figure 6) is the basis of many other antennas and is also used as a reference antenna for the measurement of antenna gain and radiated power density.

At the frequency of resonance, i.e., at the frequency at which the length of the dipole equals a half-wavelength, we have a minimum voltage and a maximum current at the terminations in the center of the antenna, so the impedance is minimal. Therefore, we can compare the half-wave dipole antenna with a series RLC resonant circuit as given in Figure 2. For a lossless half-wave dipole antenna, the series resistance of the equivalent resonant circuit equals the radiation resistance, generally between 60? and 73?, depending on the ratio of its length to the diameter.

The bandwidth of the resonant circuit (or the antenna) is determined by the L-to-C ratio. A wire with a larger diameter means a larger capacitance and a smaller inductance, which gives a larger bandwidth for a given series resistance. That's why antennas made for measurement purposes have a particularly large wire diameter.

As opposed to the (only hypothetical) isotropic radiator, real antennas such as the half-wave dipole have a more or less distinct directional radiation characteristic. The radiation pattern of an antenna is the normalized polar plot of the radiated power density, measured at a constant distance from the antenna in a horizontal or vertical plane.

Figure 7 shows the radiation pattern of a half-wave dipole antenna.

Since the dipole is symmetrical around its axis, the three-dimensional radiation pattern rotates around the wire axis.

The isotropic gain of a half-wave dipole antenna is 2.15dB. Therefore, in the direction perpendicular to the wire axis, the radiated power density is 2.15dB larger than that of the isotropic radiator. There is no radiation in the wire axis. The half-wave dipole produces linear polarization with the electrical field vector in line with, or in other words parallel to, the wire axis.

Because the half-wave dipole is often used as a reference antenna for measurements, sometimes the gain of an antenna is referenced to the radiated power density of a half-wave dipole instead of an isotropic radiator. Also the effective radiated power (ERP), which is the power delivered to an ideal dipole that gives the same radiation density as the device under test, is used instead of the EIRP. The relations Gdipole = Gisotropic - 2.15dB and ERP = EIRP - 2.15dB can be applied.


EEOL_2008FEB28_RFD_NETD_NT.jpg

Figure 6: Half-wave dipole antenna


The half-wave dipole needs a differential feed because both of its terminations have the same impedance to ground. This can be convenient if the transmitter output or the receiver input have differential ports. A balun will be used along with the half-wave dipole in case of single-ended transmitters or receivers, or if an antenna switch is used. For external ready-manufactured half-wave dipoles, the balun is visually built-in to the antenna and provides a single-ended interface.

The half-wave dipole is an electrical antenna. This means that it is easily detuned by materials with a dielectric constant larger than 1 within its reactive near field. If, for instance, the housing of a device is in the reactive near field, the housing has to be present when the antenna is matched. The human body has a large dielectric constant of approximately 75. As a result, if an electrical antenna is worn on the body or held in the hand, it can be strongly detuned.


EEOL_2008FEB28_RFD_NETD_NT1.jpg

Figure 7: Radiation pattern of a half-wave dipole antenna


If the antenna is built as two traces on a PCB, the dielectric constant of the PCB material has to be considered. The electrical field in the reactive near field region spreads out partially into the PCB material, partially into the surrounding air. This gives an effective dielectric constant eeff between that of the air and the PCB material:


EEOL_2008FEB28_RFD_NETD_NT_1.jpg

Where h is the thickness of the PCB material, w is the trace width of the dipole arms. The required length of the half-wave dipole is then:


EEOL_2008FEB28_RFD_NETD_NT_2.jpg

Underneath the dipole and within the reactive near field, no ground plane is allowed.

Monopole structure
In many cases, the half-wave dipole is just too large. Also, the needed differential feed is often a disadvantage. If we replace one branch of the dipole antenna by an infinitely large ground plane, due to the effect of mirroring, the radiation pattern above the ground plane remains unaffected. This new structure is called a monopole antenna.


EEOL_2008FEB28_RFD_NETD_NT2.jpg

Figure 8: Building up the quarter-wave monopole


Because all the radiated power is now concentrated in the half-space above the ground plane, the gain of the monopole is 3dB larger than the gain of the dipole.

Often a large ground plane is not feasible. The Marconi antenna replaces the (not realizable) infinitely large ground plane by several open-ended λ/4-Stubs, called the counterpoise.

A further reduction to only one stub gives a structure that looks like a bent dipole antenna. When designing a monopole antenna, the radiator should go as long as possible perpendicular to the ground stub or the ground plane. Bends close to the feeding point reduce the radiation resistance and the efficiency of the antenna.

The ideal quarter-wave monopole has a linear polarization with the vector of the electrical field in the wire axis. If the ground plane becomes unsymmetrical, the direction of polarization will be tilted towards the larger part of the ground plane, but still remains linear.

The radiation resistance of an ideal quarter-wave monopole is half of that of a dipole; depending on the ratio of length to diameter of the radiator between 30? and 36.5?.

Like the half-wave dipole, the quarter-wave monopole is an electrical antenna. It is influenced by the dielectric constant of the material in the reactive near field. The same formulas for the effective dielectric constant and the required length as for the half-wave dipole hold for the quarter-wave monopole.

Table 1 gives the length of half-wave dipoles and quarter-wave monopoles in free space and on a PCB for commonly used short-range frequencies. For the PCB antennas, a PCB thickness of h = 1.5mm and a trace width of w = 1mm has been assumed; the PCB material is FR4 with εr = 4.2. This gives an effective dielectric constant of εr = 2.97.


点击看大图


It has to be mentioned that parasitic components, such as capacitance to ground, inductance introduced by bends in the antenna as well as the influence of the package, alter the antenna impedance. For monopole antennas, the ground plane is sometimes smaller than a quarter-wave length or not perpendicular to the radiator. In practice, the exact length of the dipole or the monopole has therefore to be determined by measuring the feed impedance with a vector network analyzer.

Sometimes the available space limits the length of an antenna. The antenna is made as long as the geometry permits, which can be smaller than one quarter wavelength. A monopole shorter than a quarter-wave length can be considered as a quarter-wave monopole, which is used at a frequency lower than the frequency of resonance.

Loaded stub antenna
According to the equivalent schematic given in Figure 2, the input impedance at the frequency of operation will then be a series connection of a resistor and a capacitor. The series capacitance can be resonated out by a series inductor. A monopole antenna shorter than l/4 with a series inductor is also referred to as a loaded stub antenna.

The radiation resistance of a loaded stub decreases with decreasing length. The smaller radiation resistance and the larger L-to-C ratio increase the quality factor and make the bandwidth smaller than for a quarter-wave monopole. Approximations for the radiation resistance of a monopole antenna are:


EEOL_2008FEB28_RFD_NETD_NT_3.jpg

At the frequency of operation (i.e., resonance), the impedance of the short stub will be that of a small resistor (radiation resistance plus loss resistance) with a series capacitor. From the Smith Chart in Figure 9 we can see that matching to a 50? source can be achieved by a series inductor and a parallel capacitor.


EEOL_2008FEB28_RFD_NETD_NT3.jpg

Figure 9: Matching of a short loaded stub antenna


Figure 10 shows an example of a loaded stub PCB antenna with matching components.


EEOL_2008FEB28_RFD_NETD_NT4.jpg

Figure 10: Loaded stub PCB antenna with matching components


The series inductor and the parallel capacitor transform the antenna impedance to 50?, the input impedance of the filter (FIL1).

For dipole or monopole antennas, the component values for the series inductor and the parallel capacitor (CP) have to be determined by measuring the feed impedance at point A in Figure 10 (with LS = 0? resistor and CP left unpopulated) with a vector network analyzer.

Once this is determined, we can use a Smith Chart to assist in matching the antenna to 50? using LS and CP.

Derivatives of the monopole are the inverted-L and inverted-F antennas as shown in Figure 11.


EEOL_2008FEB28_RFD_NETD_NT5.jpg

Figure 11: Inverted-L antenna and Inverted-F antenna


In the inverted-L antenna, the monopole does not run perpendicularly to the ground plane over its whole length but is bent parallel to the ground plane after some distance. This helps to save space, but decreases the radiation resistance because the radiator comes closer to the ground plane. An additional matching circuit is needed to match the low-feed impedance to the usual transmission line impedance of 50?.

If we proceed from the feed point of the inverted-L antenna to the end, we notice that the voltage increases (while the current decreases) from a maximum voltage value at the feeding point to almost zero at the end. This means, that the antenna impedance has its minimum if we feed the antenna as shown in Figure 11a) and increases if we move the feeding point towards the end. The inverted-F antenna in Figure 11b is an inverted-L antenna with a feeding tap that gives larger antenna impedance. If the antenna is tapped at the right location, no additional matching circuit is required.

The structure of inverted-F antennas and, in particular, the location of the tap, is usually determined by electromagnetic simulations.

Helical antennas
Another option to reduce the size of a monopole is to coil it up into a helix as shown in Figure 12.


EEOL_2008FEB28_RFD_NETD_NT6.jpg

Figure 12: Helix antenna on a ground plane


When the coil circumference and the spacing between adjacent turns are comparable to the wavelength, the antenna radiates a circular polarized beam in the axis of the helix. These antennas are called axial mode helicals.

In small short-range applications, the helix diameter and the spacing between turns are much smaller than a wavelength. So, the result is a normal mode helical antenna. The radiation pattern of a normal mode helix is similar to that of a monopole; the maximum radiation occurs perpendicular to the helix axis. Due to the shape and the size of the ground plane, radiation patterns of practical antennas can show deviations from this idealized form. The radiation from a normal mode helix is elliptically polarized. Usually the component having the electrical field vector parallel to the antenna axis is stronger than the component which is parallel to the ground plane.

The exact calculation of transversal mode helical antennas is not as simple as for dipole and monopole antennas. Usually they are designed empirically: start with a wire that is half a wavelength long, wind it up into a helix, and measure the antenna impedance using a vector network analyzer. Then, cut it back until nearly real input impedance at the frequency of operation is obtained. Real input impedance means that the antenna is in resonance. Fine-tuning of the frequency of resonance is possible by compressing or stretching the helix.

Even if the antenna is in resonance, it will not be matched to 50? yet. The input impedance will be the sum of the radiation and loss resistances, usually smaller than 50?. For the design of the needed additional matching circuit, we can use the Smith Chart as described above.

Chu's and Wheeler's limit on the bandwidth for a given dimension also holds for helix antennas. A small transversal mode helix, therefore, has tight bandwidth and is sensitive to tolerances of the matching components.



Antennas connect RF signals in an electrical circuit, such as between a PCB and an electromagnetic wave propagating in the transmission media between the transmitter and the receiver of a wireless link.


The conclusion of the three-part series focuses on small loop antennas with differential feed, single-ended loop and trapped PCB loop antennas.


The loop antenna shown in Figure 13 has a differential feed. Often a ground plane is made part of the loop, giving a single-ended feed as shown in Figure 14.


The small arrows indicate the current flow through the loop. On the ground plane, the current is mainly concentrated on the surface. The electrical behavior of the structure in Figure 14 is therefore similar to that of the loop with differential feed shown in Figure 13.


The following considerations on small loop antennas are based on and assume that the current is constant over the loop. This means that the circumference must be smaller than one tenth of a wavelength. Although this is rarely the case, the given formulas describe the principal behavior and can be used as a starting point for the loop antenna design.


If the current is constant over the loop, we can consider the loop as a radiating inductor with inductance L, where L is the inductance of the wire or PCB trace. Together with the capacitor C, this inductance L builds a resonant circuit. Often a resistor Ratt is added to reduce the quality factor of the antenna and to make it less sensitive to tolerances. Of course, this resistor dissipates energy and reduces the antenna's efficiency.


The following calculations hold for circular loops with the radius a for square loops with the side length a. A rectangular antenna with the sides a1 and a will be approximated by an equivalent square with the side length:



EEOL_2008MAR14_RFD_NETD_NT_S1.jpg


The length (circumference) of the wire building the loop will be called U, where U = 2πa for a circular loop, or 4a for a square loop.


For the calculation of the inductance, the wire radius b, where b is 1/2 the diameter of the actual wire used to fabricate the antenna, is needed. In the frequent case where a loop antenna is realized by a trace on a PCB, b = 0.35.d + 0.24.w can be used, where d is the thickness of the copper layer and w is the trace width.


Figure 15 shows the equivalent schematic of a small loop antenna.



EEOL_2008MAR14_RFD_NETD_NT_S2.jpg


The radiation resistance of loop antennas is small, typically smaller than 1?. The loss resistance Rloss describes the ohmic losses in the loop conductor and the losses in the capacitor (expressed by its ESR). Usually, the ESR of the capacitor cannot be neglected. Interestingly, the thickness of the copper foil is not needed for the calculation of the loss resistance because due to the skin effect, the current is confined on the conductor surface.



EEOL_2008MAR14_RFD_NETD_NT.jpg
Figure 13: Small loop antenna with differential feed


Together with the loop inductance L, which is the inductance of the wire, the capacitor C builds a series resonant circuit. In practice, the L-to-C ratio of this resonant circuit is large giving a high quality factor (Q). This would make the antenna sensitive to tolerances. That's why often an attenuating resistor Ratt is added to reduce the Q. To describe the influence of Ratt on the loop antenna, we make a parallel to series conversion and use the equivalent series resistance Ratt trans. The resistance value of Ratt trans is determined by the acceptable tolerance of the capacitor and the geometry of the loop.



EEOL_2008MAR14_RFD_NETD_NT1.jpg
Figure 14: Single-ended loop antenna


The maximum usable quality factor is calculated from the capacitance tolerances ΔC/C:



EEOL_2008MAR14_RFD_NETD_NT_S3.jpg


The series transformed attenuation resistance then will be:



EEOL_2008MAR14_RFD_NETD_NT_S4.jpg


This gives the efficiency of the loop antenna:



EEOL_2008MAR14_RFD_NETD_NT_S5.jpg


In most cases, the radiation resistance is much smaller than the loss resistance and the transformed attenuation resistance, giving a poor efficiency. In this case, the approximation:



EEOL_2008MAR14_RFD_NETD_NT_S6.jpg


can be used. Rr is determined by the loop area, which is πa2 for circular loops, a2 for square loops, and a1a2 for rectangular loops. Figure 16 shows the efficiency of small circular loop antennas versus their diameter for an assumed tolerance of 5 percent. The trace width has been assumed as 1 mm, the copper thickness as 50 um; but both values have only a minor influence on the efficiency, which is mainly determined by the attenuation resistance Ratt. As expected, the efficiency increases with increasing diameter.



EEOL_2008MAR14_RFD_NETD_NT2.jpg
Figure 15: Equivalent schematics of the small loop antenna in Figure 13



EEOL_2008MAR14_RFD_NETD_NT3.jpg
Figure 16: Efficiency of small loop antennas for five-percent tolerance


If we feed the loop antenna as shown in Figure 14, the series equivalent circuit of Figure 15 describes the antenna impedance. Even including the effect of Ratt, the total series resistance will be small, usually below 10?. If we feed the antenna directly at the capacitor, the parallel equivalent circuit describes the antenna impedance. A small series loss resistor transforms into a large parallel resistor, usually several k?s.


In both cases, matching to 50? will be difficult. That's why the loop antenna is often tapped, giving an impedance in between the too small and the too large values. Figure 17 shows an example:



EEOL_2008MAR14_RFD_NETD_NT4.jpg
Figure 17: Example of a tapped PCB loop antenna


A series feed (in the lower right corner) would give a small impedance. A parallel feed (directly at the capacitors) would give a much too large impedance. The tap provides an impedance close to 50? in this example. The loop capacitor has been split into two series capacitors C1 and C2. This makes it possible to realize non-IEC capacitance values. R1 is the damping resistor which de-Qs the circuit, thus increasing the bandwidth and subsequently reducing the tolerance requirements.


Unfortunately, there are no easy formulas that describe the tapped structure and give the right location for the tap. The line from the antenna termination to the tap is not a transmission line and will disturb the field in the antenna. Therefore, we have to find out the optimal structure by electromagnetic simulations. Often a trial and error procedure is used as an alternative. For example, using a vector network analyzer, we determine the capacitance value that gives the best return loss and the largest resistance value that gives the required bandwidth.


The loop antenna gives a linear polarization with the vector of the electric field oscillating in the plane built by the loop.


In contrast to all of the antennas discussed so far, loop antennas are magnetic antennas. This means that they are not detuned by the dielectric constant of the material in their reactive near field. That's why loop antennas are often used for body-worn or hand-held equipment.


Table 2 shows a feature comparison of the discussed antennas.



点击看大图


Antenna design rules
We can summarize the considerations made so far in the following rules of thumb:






If the available space is sufficient, use a half-wave dipole (for differential feed) or quarter-wave monopole (for single-ended feed) antenna for best efficiency.



If possible, keep the space around the antenna clear from conducting or dielectric materials, such as electronic components, the casing or the user's body.



Sometimes, dielectric materials in the reactive near field are unavoidable. In these cases, measure the antenna impedance under real application conditions and match it to the needed characteristic impedance.



Due to space limitations, the ground plane of quarter-wave monopoles is often too small. In these cases try to create as much ground plane around the feed point as possible, measure the resulting antenna impedance and match it to the needed characteristic impedance. Good performance can be obtained from a counterpoise made from a quarter-wavelength conductor that is connected to ground in the vicinity of the antenna's feeding point. The counterpoise should run as long as possible perpendicular to the monopole radiator.



When using premanufactured antennas, keep in mind that their performance depends on the attached ground plane. The manufacturer's specifications are only achieved if the ground plane has the same size and shape as the manufacturer's evaluation board. In all other cases, you have to measure the impedance of the premanufactured antenna under application conditions and to match it to the needed characteristic impedance.



Small loop antennas are insensitive to varying dielectric conditions in their reactive near field. They can be a good solution for portable and hand-held devices but have a much lower efficiency than electrical antennas. Only antennas with a circumference smaller than one tenth of a wavelength can be considered as purely magnetic antennas. Larger loops have a higher gain but also a higher sensitivity to the environmental conditions.



Size matters: Always keep in mind that Chu's and Wheeler's limit determines the product of the bandwidth and the efficiency for a given antenna dimension. An extremely small antenna cannot be efficient and tolerance-insensitive at the same time.




TRF6901 ref design
Figure 18 shows the structure of the antenna used in the TRF6901 reference design:



EEOL_2008MAR14_RFD_NETD_NT5.jpg
Figure 17: PCB antenna layout on the TRF6901 reference design


Beginning from the feeding point, two legs with different lengths run in parallel to the PCB ground plane and can be terminated at their ends by SMD components to ground. Depending on the used termination elements the layout can be used as an inverted-F antenna or a tapped small loop antenna.


The short leg is usually terminated by a 0? resistor. If the long arm is left open, we get an inverted-F antenna. Terminating the long arm with a capacitor and a resistor in parallel gives a tapped loop antenna similar to the one shown in Figure 17; 1 k? and 0.5pF bring the loop into resonance at 915MHz.


When the antenna is used as a loop antenna, we have to consider the circumference of the loop in relation to the wavelength on the PCB. The trace width of the antenna in the reference design is 1.5mm and the thickness of the PCB material is also 1.5mm. As an approximation, we calculate the effective dielectric constant according to Section 2.2 and get εeff = 3.1. The wavelength of a 915MHz signal on the PCB is then:



EEOL_2008MAR14_RFD_NETD_NT_S7.jpg


The circumference of the loop in the reference design is 91mm, which is almost half a wavelength. The antenna behavior will therefore be different from that of a pure magnetic antenna; the antenna will excite some electrical field in the reactive near field too. This gives a gain larger than predicted for the loop antenna in Figure 17.


As we can see from Figure 18, the antenna is bent around the corner of the PCB. This gives radiation in both the x and y direction and helps to make the radiation pattern more omni directional.

文章评论0条评论)

登录后参与讨论
我要评论
0
7
关闭 站长推荐上一条 /2 下一条