5.1 Time-domain modeling of wire antennas by method of momentsAdvanced theoryIn this layer the implicit algorithm will
be derived by solving the system of the equations (5.1A.1) to (5.1A.6) for the wire dipole which is placed along the z axis (fig. 5.1B.1). Since only z components
of the vector potential and the intensity of electric field are in this system
of equations, it is not necessary to distinguish among the components of
vectors. Thus, in the following text, the subscript z will be omitted.
The implicit algorithm will be derived
from the equation (5.1A.5) which can be rewritten by considering the boundary condition (5.1A.6) to the following form
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( 5.1B.1 )
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Now, let’s carry out the first step of the solution, the application
of the method of moments to (5.1B.1). Let’s divide the wire dipole to N segments of the same length Δz and denote the ends of the segments by coordinates z0,
z1, …, zN+1 (fig. 5.1B.1). Further, let’s
denote the center of segments by z0+, z1+,
…, zN+, and z1-, z2-,
…, zN+1-, respectively. For the expansion of the
current distribution on the wire dipole in space, let’s use the constant basis functions: in the region of a current cell (fig. 5.1B.1), which is bounded by the coordinates either zn+,
zn+1+ or zn-1-, zn-,
the constant current distribution is supposed. It is appropriate to remember,
that the current at the end of the wire is equal to zero, because it can not
flow anywhere. In the region of a charge cell, which is bounded by the
coordinates zn, zn+1, the constant charge
density distribution is supposed.
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Fig. 5.1B.1 | Wire dipole discretization. |
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The constant basis functions are in the region of the current cell
defined by the following relation
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( 5.1B.2 )
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By these basis functions and time dependant unknown current
coefficients In (t) the time-space current
distribution in (5.1A.1) can be approximated
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( 5.1B.3 )
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Let’s discretize our wire dipole in time (the second step). Let’s
divide the time step to the equal intervals of the length Δt and denote the individual time instant on time axes by tk=kΔt for k = 0, 1, 2, …, ∞. At these time
instants the current distribution on the wire antenna is be computed.
Substituting (5.1B.3) to (5.1A.1) and
(considering (5.1B.2)) the vector potential at the point
zm and the time instant tk can be written
in the following form
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( 5.1B.4 )
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where
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( 5.1B.5 )
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( 5.1B.6 )
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( 5.1B.7a )
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( 5.1B.7b )
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For the evaluation
of the distance in (5.1B.6) the
accurate relation (5.1B.7a), or the approximate one (5.1B.7b), which neglects the
radius of a wire a, can be used. Using the approximate relation
increases the stability of the algorithm, however, it is possible to use it
only if the length of the time step multiplied by the speed of light in the
surrounding medium is much larger, than the radius of the wire (cΔt>>a). Otherwise, the accuracy falls down. Using the
approximate relation was introduced in [37] and if the mentioned condition is
met, it is appropriate to use (5.1B.7b). The interested reader can test the
influence of that neglect on the accuracy and stability of the algorithm.
Let’s discretize the scalar potential (5.1A.2) where the space-time charge
density distribution is the unknown quantity. The charge density can be
computed with the continuity equation (5.1A.4) which
can be rewritten in the following form
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( 5.1B.8 )
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Substituting the space-time charge density distribution (5.1B.3) to
(5.1B.8) and approxiomating the partial differentiation of the current with
respect to variable z by the center difference, the continuity equation
(5.1B.8), after the swap of the derivation and integration, can be written
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( 5.1B.9 )
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Since the constant basis functions
are used for the space approximation of the current (5.1B.3), the partial
derivative with respect to variable z in (5.1B.9) could not be computed
straightforwardly (the derivative of the constant function is equal to zero),
but the center difference has to be used. To be the differentiating correct,
the integral of currents with respect to time at the ends of the wire were
included in (5.1B.9), although they are equal to zero. In the last step in (5.1B.9)
the basis functions were swaped: from the
spacious approximation of the current by the basis functions fn(z) we got toward the approximation
of the charge density by the basis functions fn+(z).
Substituting the continuity equation (5.1B.9)
to (5.1A.2) the scalar potential at the point zm+
and the instant tk can be evaluated
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( 5.1B.10 )
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where
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( 5.1B.11 )
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( 5.1B.12a )
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( 5.1B.12b )
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( 5.1B.13 )
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Here, as in case of the evaluating of the vector potential, it is possible to use for the evaluation of the distance
in (5.1B.11) either the accurate relation (5.1B.12a), or the approximate relation (5.1B.12b).
The reasons and the condition are the same as in case of the evaluation of the
vector potential.
Similarly the scalar potential at the point zm and the time instant tk
can be evaluated zm-
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( 5.1B.14 )
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To evaluate the relations (5.1B.10) and (5.1B.14),
it is necessary to compute the integral of the current with respect to time.
The integral can be evaluated according to different numerical integration
rules. We choose the trapezoid rule because its implementation is easy and
offers sufficient accuracy. By this rule, the integral of the current in the
interval from 0 to tk,, in case of the equidistant
division of the interval, can be computed
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( 5.1B.15 )
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Now, let’s go back to (5.1B.1) and discretize
it. Let’s approximate the first derivative of the vector potential with respect
to time by the center difference of the first order. By this step the partial
derivative of the vector potential is evaluated
at the point zm and the time instant tk-1/2.
To be the calculation sufficiently accurate, the partial derivative of the scalar potential with respect to variable z has
to be evaluated at the same point and the time instant. This can be reached by
using the center differentiation for the scalar potential at the points zm+ and zm-
at two instants tk and tk-1. The average of
these central differences is actually numerically evaluated the derivative of
the scalar potential at the point zmand the time instant tk-1/2. Of course, the excitation
pulse has to be evaluated at the same point and the instant as the vector and scalar potentials.
After this steps the equation (5.1B.1) can be rewritten into the following form
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( 5.1B.16 )
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Rearranging terms in (5.1B.16) we obtain
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( 5.1B.17 )
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The vector potential on
the left-side of the equation (5.1B.17), computed according to (5.1B.4), can be
transcribed
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( 5.1B.18 )
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where
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( 5.1B.19a )
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( 5.1B.19b )
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For evaluating A1(zm, tk),
only the contributions of currents at delayed time instants tRk(m, n)>tk-1 are considered (the unknowns currents). In case of the evaluating
of A2(zm, tk), only the contributions of currents at delayed instants tRk(m, n)≤tk-1 are considered
(the known currents). The unknown current at the time instant tRk(m, n) in the interval from tk-1 to tk can be evaluated
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( 5.1B.20 )
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Substituting (5.1B.20) to (5.1B.19a), A1(zm,
tk) can be expressed by the unknown and known currents at the
instants tk and tk-1
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( 5.1B.21 )
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where
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( 5.1B.22a )
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( 5.1B.22b )
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The
term A11(zm, tk) contains only
the unknown currents at the instant tk.
Now, let’s focus our attention on the rest of the right-side of the
equation (5.1B.17). The scalar potential (5.1B.10) at
the point zm+ can be evaluated
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( 5.1B.23 )
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where the terms on the right-side (5.1B.23) can
be expressed as the vector potential (5.1B.18).
Let’s focus our attention on the first term
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( 5.1B.24 )
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where
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( 5.1B.25a )
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( 5.1B.25b )
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The situation is analogical as for the vector potential, however more complicated, because of
the integral of the current with respect to time in (5.1B.25). Since the term φ1(zm++, tk) contains
the unknown current at the time instant tk, let’s express the
integral of the current over the interval from 0 to tRk(m+,
n+) in (5.1B.25a) as the sum of two integrals
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( 5.1B.26 )
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where
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( 5.1B.27a )
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( 5.1B.27b )
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The term φ13(zm++, tk) in (5.1B.27b)
can be easily evaluated, since it contains only the known values of the
currents. However, the term φ1’(zm++, tk)
contains the unknown current at the time instant tk.
Therefore we express φ1’(zm++, tk)
by the trapezoid rule for the numerical evaluation of the integral in the
interval from tk-1 to tRk(m+, n+),
and the relations (5.1B.18) and (5.1B.20)
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( 5.1B.28 )
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where
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( 5.1B.29a )
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( 5.1B.29b )
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Now only the term φ11(zm++, tk) contains
the unknown current at the time instant tk. This one can be
easily expressed by (5.1B.29a). The relation (5.1B.24) can be expressed, considering (5.1B.25)
to (5.1B.29), as follow
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( 5.1B.30 )
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Analogically
we can proceed with the evaluation of the term φ (zm+-,
tk)
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( 5.1B.31 )
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or
the scalar potential at the point zm-
and the time instant tk φ(zm-,
tk).
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( 5.1B.14 )
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where
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( 5.1B.32a )
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( 5.1B.32b )
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The terms on the right-sides of the relations
(5.1B.31) and (5.1B.32) can be expressed similarly as the terms on the right-sides of
relations (5.1B.24) to (5.1B.29) by changing the corresponding superscripts + and -,
or vice versa.
Substituting (5.1B.10), (5.1B.14), (5.1B.18) to (5.1B.21)
and (5.1B.24) to (5.1B.32) into the left-side of the relation (5.1B.17) and by
rearranging the terms in this equation we obtain
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( 5.1B.33 )
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where
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( 5.1B.34a )
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( 5.1B.34b )
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( 5.1B.34c )
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( 5.1B.34d )
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The system of N equations (5.1B.33) is
possible, with considering (5.1B.18) to (5.1B.21) and (5.1B.23) to (5.1B.32), to rewrite
into the following matrix equation
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( 5.1B.35 )
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where
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( 5.1B.36a )
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( 5.1B.36b )
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( 5.1B.36c )
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( 5.1B.36d )
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In (5.1B.35) we denote the matrix of the size NxN
and Nx1 by square and brace brackets, respectively. It is apparent that
the left side of the equation (5.1B.35) contains only the unknown currents at the
time instants t=tk, however, the right-side contains
the known currents at time instants t±tk-1. The algorithm can start with the
assumption {I(m, t0)}={0} and computing {I(m,
t1)}. When the current are computed {I(m,t1)},
then it is possible to compute {I(m,t2)} and so
on. Further, it should be noted, that it is necessary to solve the inverse
matrix. However, this one does not depend on time and it is spare. Thus, the
inverse matrix is computed only once.
Using the implicit algorithm is demonstrated in the layer A on the analysis of
the wire dipole.
Numerical model of antenna excitation
Let’s go back to the excitation of our wire antenna, and discus the appropriate numerical
model of the excitation. Let’s suppose that the feeding ports of our antenna
are located in the position of the current cells z1, z2,
…, zN of our discretized wire antenna (fig. 5.1B.1); denote this
place by zf. The length of the feeding port is equal to the
length of the discretization segment. An antenna can generally work in a
receiving or transmitting mode.
If the antenna works in the receiving mode,
the plane wave electromagnetic wave incidents on antenna’s surface, and its
transient dependence can be arbitrary (in our case it is defined by a Gaussian
pulse modulated by a harmonic signal (5.1A.7)). Depending on the direction of the
incident wave with the respect to antenna axis, the transient dependence of the
incident wave at the current cells z1, z2,
…, zN is delayed. The incident wave induces in the wire
antenna a current. The current response at the location of the feeding port zf
can be recorded.
If the antenna works in the transmitting
mode, the situation is analogical to the one described in chapter 4.1. In the
transmitting mode the voltage source is connected to the feeding port of the
antenna at zf. This source evokes the intensity of the electric
field at the feeding port (in our case the time dependence is described by the
Gaussian pulse modulated by a harmonic signal). Since the excitation source is
connected only at the location of the feeding port zf, at the
other current cells the intensity of the excitation field is equal to zero.
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