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For the CF-Multipoll, the external STAs in the overlapping BSS will have their TXOPs overlap the ones allocated to the internal STAs. We assume that the interference from external STAs has been included in the parameter BER. Hence, Dn,m = (n m) (1 ) frame num/2 ldata

where no is the number of spheres per unit volume. Putting (10.2.8), (10.2.9), and (10.2.10) together gives

(10.2.11)

Putting (10.2.12) in (10.2.13) gives noaE D = EE + noa = 1-1+-2noa] 3E noa E [ 1--

(10.2.13)

(10.2.14)

frame )

(10.2.15)

[ 1--

(10.2.16)

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Next we determine the polarizability 0: of a sphere of radius a and permittive ity E , consider E = Ee Z to be the exciting field upon the sphere. Let <Pout p and <Pin be the scalar potentials outside and inside the sphere, respectively. Solving Laplace's equation by letting

(10.2.17) (10.2.18)

Also, each successive TXOP starts an SIFS period after the predecessor s TXOP limit expires in the CF-Multipoll. Note that the time spent by a polled STA is xed regardless of the number of pending data frames. Hence, Tn,m = tn poll + n SIFS + n frame num (tdata

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The boundary conditions are the continuity of the potential and the continuity of the normal component of the displacement. At r = a

(10.2.19) (10.2.20)

(10.2.21) (10.2.22)

(10.2.23)

(10.2.24)

+ SIFS)

15 =

(10.2.25)

I also like to tail the log file so that I can see how things are progressing:

(10.2.26)

Using (10.2.24)-(10.2.26)

(10.2.27)

(21.8)

(10.2.28)

Putting a from (10.2.28) in (10.2.16) gives the effective permittivity of a medium consisting of particles of permittivity Ep embedded in a background medium of permittivity E. 1 + 2 fy ) Eeff = E ( 1 - fy where

(10.2.29)

(10.2.30)

In the CP-Multipoll, there are two processing phases: one is for the normal multipoll and the other is for the error recovery. In the normal phase, there are (n m) STAs successfully receiving the multipolling frame under the state m : fail. Among these STAs, (1 )(n m) STAs are behaved STAs and (n m) STAs are nonbehaved ones. Each nonbehaved STA is assumed to destroy one data frame transmitted by a behaved one. In the recovery phase, m STAs failed to receive the multipolling frame and (n m) nonbehaved STAs will be served individually using the CP-Multipoll with poll size one. The analysis of this phase is similar to the one in the single poll. Hence, Dn,m has the following value:

(10.2.31)

Equation (10.2.16) is known as the Clausius-Mossoti formula or the LorentzLorenz formula. On the other hand, (10.2.29) is known as the MaxwellGarnett mixing formula. The Maxwell-Garnett mixing formula can be put in the following symmetric form

After a while we should see our log file spit out the following:

(10.2.32)

which is also known as the Rayleigh mixing formula. Given the effective permittivity, we can also calculate the effective propagation constant K with

k 21

normal recovery Dn,m = Dn,m + Dn,m normal Dn,m = [(1 ) (n m) frame num/2 (n m)] (1 ) ldata frame (1 ERRdata frame ) recovery Dn,m = [m + (n m)] (1 ) frame num/2 ldata frame (1 ERRdata frame ) (1 ERR1 poll )

(10.2.33) (10.2.34)

However the imaginary part of the effective propagation constant K in (10.2.33) only accounts for absorption. To include the attenuation due to scattering, we have to take into account incoherent scattering which we will study in the next section.

In this section, the coherent propagation constant is calculated by including the attenuation due to scattering. The scattered intensity can be attributed to the radiation of the induced dipole that is induced by the exciting field.

From (10.2.8) and (10.2.12)

=---

(21.9)

(10.2.35)

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(10.2.36)

Since the electric field E is in the medium that has effective wavenumber K. Let K r = Re(K). Thus we can write (10.2.37) where e is the polarization of the electric field and K r is the wavevector with IKrl = K r . At the position Ti of the ith particle, we have induced dipole moment

(10.2.38)

_ _ Esi(r)

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