Controlling Radiated Emissions by Design
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Controlling Radiated Emissions by Design - Michel Mardiguian
© Springer International Publishing Switzerland 2014
Michel MardiguianControlling Radiated Emissions by Design10.1007/978-3-319-04771-3_2
2. Electric and Magnetic Fields from Simple Circuit Shapes
Michel Mardiguian¹
(1)
EMC Consultant, St Remy-les-Chevreuse, France
If one wants to avoid empirical recipes and the wait and see if it passes
strategy, the calculation of radiated fields from electric circuits and their associated transmission cables is of paramount importance to proper EMI control. Unfortunately, precisely calculating the fields radiated by a modern electronic equipment is a hopeless challenge. In contrast to a CW transmitter, where the radiation source characteristics (e.g., transmitter output, antenna gain and pattern, spurious harmonics, feeder and coupler losses, etc.) are well identified, a digital electronic assembly, with its millions of input/output circuits, printed traces, flat cables, and so forth, is impossible to mathematically model with accuracy, at least within a reasonable computing time by today’s state of the art. The exact calculation of the E and H fields radiated by a simple parallel pair excited by a pulse train is already a complex mathematical process.
However, if we accept some drastic simplification, it is possible to establish an order of magnitude of the field by using fairly simple formulas. Such simplification includes:
1.
Retaining only the value of the field in the optimum direction
2.
Having the receiving antenna aligned with the maximum polarization
3.
Assuming a uniform current distribution over the wire length, which can be acceptable by using an average equivalent current instead of the maximum value
4.
Ignoring dielectric and resistive losses in the wires or traces
The formulas described hereafter were derived by S. Schelkunoff [5] from more complex equations found in the many books on antenna theory. They allow us to resolve most of the practical cases, which can be reduced to one of the two basic configurations:
1.
The closed loop (i.e., magnetic excitation)
2.
The straight open wire (i.e., electric excitation)
2.1 Field Radiated by a Loop
An electromagnetic field can be created by a circular loop carrying a current I (Fig. 2.1). Assuming that:
A103098_3_En_2_Fig1_HTML.gifFig. 2.1
Radiation from a small magnetic loop
I is uniform along the loop.
There is no impedance in the loop other than its own reactance.
The loop size is ≪λ.
The loop size is
The loop is in free space, not close to a metallic surface.
E and H can be found by using the simple solutions that Schelkunoff derived from Maxwell’s equations. Replacing some terms by more practical expressions:
$$ {H}_r\;\mathrm{A}/\mathrm{m}=\frac{ IA}{\lambda}\left[\frac{j}{D^2}+\frac{\lambda }{2\pi {D}^3}\right] \cos \sigma $$(2.1)
$$ {H}_{\sigma}\;\mathrm{A}/\mathrm{m}=\frac{\pi IA}{\lambda^2D}\sqrt{1-{\left(\frac{\lambda }{2\pi D}\right)}^2+{\left(\frac{\lambda }{2\pi D}\right)}^4} \sin \sigma $$(2.2)
$$ {E}_{\phi}\;\mathrm{V}/\mathrm{m}=\frac{Z_0\pi IA}{\lambda^2D}\sqrt{1+{\left(\frac{\lambda }{2\pi D}\right)}^2} \sin \sigma $$(2.3)
where:
I = loop current, in amperes
A = loop area in m²
λ = wavelength in meters = 300/F(MHz)
D = distance to observation point, in meters
Z0 = free space impedance = 120π or 377 Ω
Comparing this with Fig. 2.1, we see that for σ = 0, E ø and H ø are null (sin σ = 0), while H r is maximum (cos σ = 1). Except near the center of a solenoid or a transmitting loop antenna, this H r term in the Z-axis direction is of little interest because it vanishes rapidly, by its 1/D ² and 1/D ³ multipliers. Notice also that there is no E r term.
To the contrary, in the equatorial plane, for σ = π/2, H r is null, and E ø, H ø get their maximum value. So from now on, we will consider systematically this worst-case azimuth angle.
Looking at Equ. (2.2) and Equ. (2.3) and concentrating on boundary conditions, we see two domains, near field and far field, plus a transition region.
Near Field: For λ/2πD > 1, i.e., D < λ/2π or D < 48/F(MHz)
Under the square root in Equ. (2.2) and Equ. (2.3), the larger terms are the ones with the higher exponent. Thus, neglecting the other second- or third-order terms, we have:
$$ {H}_{\mathrm{A}/\mathrm{m}}=\frac{ IA}{4\pi {D}^3} $$(2.4)
$$ {E}_{\mathrm{V}/\mathrm{m}}=\frac{Z_0 IA}{2\lambda {D}^2} $$(2.5)
We remark that H is independent of λ, i.e., independent of frequency: the formula remains valid down to DC. H falls off as 1/D ³. E increases with F and falls off as 1/D ².
In this region called near-field or induction zone, fields are strongly dependent on distance. Any move toward or away from the source will cause a drastic change in the received field. Getting ten times closer, for instance, will increase the H field strength 1,000 times.
Since dividing volt/m by amp/m produces ohms, the E/H ratio, called the wave impedance for a radiating loop, is
$$ {Z}_w\;\left(\mathrm{near}\;\mathrm{loop}\right)={Z}_0\frac{2\pi D}{\lambda } $$(2.6)
When D is small and λ is large, the wave impedance is low. We may say that in the near field, Z w relates to the impedance of the closed loop circuit which created the field, i.e., almost a short. As D or F increases, Z w increases.
Far Field: For λ/2πD < 1, i.e., D > λ/2π, or D > 48/F(MHz)
The expressions under the square roots in Equ. (2.2) and Equ. (2.3) are dominated by the terms with the smallest exponent. Neglecting the second- and third-order terms, only the 1
remains, so:
(2.7)
$$ {E}_{\mathrm{V}/\mathrm{m}}=\frac{Z_o\pi IA}{\lambda^2D} $$(2.8)
In this region, often called the far-field, radiated-field, or plane wave region ¹, both E and H fields decrease as 1/D (see Fig. 2.2). Their ratio is constant, so the wave impedance is
$$ {Z}_w=E/H=120\pi \kern0.48em \mathrm{or}\kern0.49em 377\;\varOmega $$A103098_3_En_2_Fig2_HTML.gifFig. 2.2
E and H fields from a perfect loop
This term can be regarded as a real impedance since E and H vectors are in the same plane and can be multiplied to produce a radiated power density, in W/m². E and H increase with F ², an important aspect that we will discuss further in our applications.
Transition Region: For λ/2πD = 1 or D = 48/F(MHz)
In this region, all the real and imaginary terms in field equations are equal, so all terms in 1/D, 1/D ², and 1/D ³ are equal and summed with their sign. This zone is rather critical because of the following:
1.
With MIL-STD-461 testing (RE102 test for instance), the test distance being 1 m, the near-far-field transition is taking place around 48 MHz, which complicates the prediction.
2.
Speculations concerning the wave impedance are hazardous due to very abrupt changes caused by the combination of real and imaginary terms for E and H.
2.2 Fields Radiated by a Straight Wire
It does not take a closed loop to create an electromagnetic field. A straight wire carrying a current, I, creates an electromagnetic field (most radio communication antennas are wire antennas). The practical difficulty is that, in contrast to the closed loop, it is impossible to realize an isolated dipole with a DC current: only AC current can circulate in an open-wire self-capacitance. Fields generated from a short, straight wire are shown in