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ANTENNA NEAR FIELD
As noted in the sections on RF propagation and the radar equation, electromagnetic radiation expands
spherically (Figure 1) and the power density at a long range (R) from the transmitting antenna is:
[1]
When the range is large, the spherical surface of uniform power density appears flat to a receiving antenna
which is very small compared to the surface of the sphere. This is why the far field wave front is considered
planar and the rays approximately parallel. Also, it is apparent that at some shorter range, the spherical surface
no longer appears flat, even to a very small receiving antenna.
The distances where the planer, parallel
ray approximation breaks down is known as the near field. The crossover distance between near and far fields (R_{ff})
is taken to be where the phase error is 1/16 of a wavelength, or about 22.5°. [2]
where λ is the wavelength and D is the largest dimension of the transmit antenna.
If
the same size antenna is used for multiple frequencies, R_{ff} will increase with increasing frequency.
However, if various size antennas are used for different frequencies and each antenna is designed with D as a
function of λ (λ/2 to 100λ), then R_{ff} will vary from c/2f to 20000c/f. In this case Rff will decrease
with increasing frequency. For example: a 10λ antenna at 3 GHZ has a D of 100 cm and corresponding R_{ff}
of 20 m, while a 10λ antenna at 30 GHz has a D of 10 cm and corresponding R_{ff} of 2 m.
While the
above analogy provides an image of the difference between the near and far fields, the relationship must be
defined as a characteristic of the transmitting antenna. Actual antennas, of course, are not ideal point
source radiators but have physical dimensions. If the transmitting antenna placed at the origin of Figure 1
occupies distance D along the Zaxis and is boresighted along the Yaxis (ф = 90), then the geometry of point P on
the sphere is represented in two dimensions by Figure 2. For convenience, the antenna is represented by a series
of point sources in an array.
When point P is close to the antenna, as in Figure 2, then the difference in
distance of the two rays r and R taken respectively from the center of the antenna and the outer edge of the
antenna varies as point P changes.
Derivation
of equation [2] is given as follows:
From Figure 2, the following applies:
[3] r2 = z2 + y2
[4] z = r cos θ
[5] y = r sin θ and
[6]
Substituting [3] and [4] into [6]
[7]
which puts point P into spherical coordinates.
Equation [7] can be expanded by the binomial theorem
which for the first three terms, reduces to:
[8]
In the parallel ray approximation for far field calculations (Figure 3) the third term of [8] is neglected.
The distance where the far field begins (R_{ff}) (or where the near field ends) is the value of r
when the error in R due to neglecting the third term of equation [8], equals 1/16 of a wavelength.
R_{ff}
is usually calculated on boresight, so θ = 90° and the second term of equation [8] equals zero (Cos 90° = 0),
therefore from Figure 3, where D is the antenna dimension, R_{ff} is found by equating the third term of
[8] to 1/16 wavelength.
Sin θ = Sin 90 = 1 and z' = D/2 so:
[9]
Equation [9] is the standard calculation of far field given in all references.
Besides [9] some
general rules of thumb for far field conditions are:
r >> D or r >> λ
If the sphere and point P are a very great distance from the antenna, then the rays are very nearly parallel
and this difference is small as in Figure 3.
Figure 3  Far Field Parallel Ray Approximation for Calculations.
The power density within the near field varies as a function of the type of aperture illumination and is
less than would be calculated by equation [1]. Thus, in the antenna near field there is stored energy. (The
complex radiation field equations have imaginary terms indicating reactive power.) Figure 4 shows normalized power
density for three different illuminations.
Curve A is for reference only and shows how power density would vary if it were
calculated using equation [1].
Curve B shows power density variations on
axis for an antenna aperture with a cosine amplitude distribution. This is typical of a horn antenna in the
Hplane.
Curve C shows power density variations on axis for a uniformly illuminated antenna
aperture or for a line source. This is typical of a horn antenna in the Eplane.
Curve
D
shows power density variations on axis for an antenna aperture with a tapered illumination.
Generally the
edge illumination is approximately 10 dB from the center illumination and is typical of a parabolic dish antenna.
Point E  For radiation safety purposes, a general rule of thumb for tapered
illumination is that the maximum safe level of 10 mW/cm2 (200 V/m) is reached in the near field if the level at R
reaches 0.242 mW/cm^{2} as can be ff verified by computing the power density at point E in Figure 4. (10
mW/cm^{2}
at point E extrapolates to 0.242 mW/cm^{2} [16 dB lower] at R=R_{ff} , or Y axis value =1). Figure
1 in Section 36 depicts more precise values for radiation hazard exposure.
Point F
 Far Field Point. At distances closer to the source than this point (near field), the power density from any
given antenna is less than that predicted using Curve A. At farther distances, (far field) power densities from
all types of antennas are the same.
Figure 4  Antenna NearField OnAxis Power Density (Normalized) For Various
Aperture Illuminations
For Various Aperture Illuminations
FOR FAR FIELD MEASUREMENTS:
When free space measurements are performed at a known distance from a source, it is often necessary to
know if the measurements are being performed in the far field. As can be seen from Curve A on Figure 4, if the
distance is halved (going from 1.0 to 0.5 on the Y axis), the power density will increase by 6 dB (going from 0 to
6 dB on the X axis). Each reduction in range by ½ results in further 6 dB increases. As previously mentioned,
Curve A is drawn for reference only in the near field region, since at distances less than R_{ff} the
power density increases less than 6 dB when the range is halved. In the far field, all curves converge and
Equation [1] applies.
When a measurement is made in free space, a good check to ensure that is was
performed in the far field is to repeat the measurement at twice the distance. The power should decrease by
exactly 6 dB. A common error is to use 3 dB (the half power point) for comparison. Conversely, the power
measurement can be repeated at half the distance, in which case you would look for a 6 dB increase, however the
conclusion is not as sure, because the first measurement could have been made in the far field, and the second
could have been made in the near field.
Table of Contents
for Electronics Warfare and Radar Engineering Handbook
Introduction 
Abbreviations  Decibel  Duty
Cycle  Doppler Shift  Radar Horizon / Line
of Sight  Propagation Time / Resolution  Modulation
 Transforms / Wavelets  Antenna Introduction
/ Basics  Polarization  Radiation Patterns 
Frequency / Phase Effects of Antennas 
Antenna Near Field  Radiation Hazards 
Power Density  OneWay Radar Equation / RF Propagation
 TwoWay Radar Equation (Monostatic) 
Alternate TwoWay Radar Equation 
TwoWay Radar Equation (Bistatic) 
Jamming to Signal (J/S) Ratio  Constant Power [Saturated] Jamming
 Support Jamming  Radar Cross Section (RCS) 
Emission Control (EMCON)  RF Atmospheric
Absorption / Ducting  Receiver Sensitivity / Noise 
Receiver Types and Characteristics 
General Radar Display Types 
IFF  Identification  Friend or Foe  Receiver
Tests  Signal Sorting Methods and Direction Finding 
Voltage Standing Wave Ratio (VSWR) / Reflection Coefficient / Return
Loss / Mismatch Loss  Microwave Coaxial Connectors 
Power Dividers/Combiner and Directional Couplers 
Attenuators / Filters / DC Blocks 
Terminations / Dummy Loads  Circulators
and Diplexers  Mixers and Frequency Discriminators 
Detectors  Microwave Measurements 
Microwave Waveguides and Coaxial Cable 
ElectroOptics  Laser Safety 
Mach Number and Airspeed vs. Altitude Mach Number 
EMP/ Aircraft Dimensions  Data Busses  RS232 Interface
 RS422 Balanced Voltage Interface  RS485 Interface 
IEEE488 Interface Bus (HPIB/GPIB)  MILSTD1553 &
1773 Data Bus  This HTML version may be printed but not reproduced on websites.
