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Lecture 5 Log Normal Shadowing

- Shadowing, also called slow fading, accounts for random variations in received power over distances comparable to building widths, requiring extra transmit power (fading margin) to compensate. - Local average power measurements are taken at antenna positions spaced half a wavelength or more, then averaged, and repeated for multiple distances to characterize shadowing effects. - The likelihood of coverage at a given distance can be expressed as the probability that the local average received power is above a required threshold, accounting for path loss and random shadowing effects modeled as a Gaussian random variable.
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0% found this document useful (0 votes)
374 views24 pages

Lecture 5 Log Normal Shadowing

- Shadowing, also called slow fading, accounts for random variations in received power over distances comparable to building widths, requiring extra transmit power (fading margin) to compensate. - Local average power measurements are taken at antenna positions spaced half a wavelength or more, then averaged, and repeated for multiple distances to characterize shadowing effects. - The likelihood of coverage at a given distance can be expressed as the probability that the local average received power is above a required threshold, accounting for path loss and random shadowing effects modeled as a Gaussian random variable.
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© © All Rights Reserved
We take content rights seriously. If you suspect this is your content, claim it here.
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Download as PDF, TXT or read online on Scribd
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LOG-NORMAL

SHADOWING
Shadowing
•  Also called slow-fading
•  Accounts for random variations in received power
observed over distances comparable to the widths of
buildings
•  Extra transmit power (a fading margin) must be provided
to compensate for these fades
Local Average Power Measurements
•  Take power measurements in Watts as the antenna is moved in a on
the order of a few wavelengths
•  Average these measurements to give a local average power
measurement

> λ/2

Velocity of antenna

Points where power measurements are made


Same-Distance Measurements

•  Local averages are made for many different locations,


keeping the same transmitter-receiver distance
•  These local averages will vary randomly with location

Example Tx-Rx
locations within
a floor of a building
Repeat for Multiple Distances
•  Similar collections of average powers are made for other
Tx-Rx distances
Likelihood of Coverage
•  At a certain distance, d, what is the probability that the
local average received power is below a certain threshold
γ?

P( Pr (d ) < γ )

Pt Gt Gr
Pr (d ) =
Lt L(d ) X σ Lr
Path Loss Shadowing
Likelihood of Coverage, cont’d
•  Since only Xσ is random, the probability can be expressed
as a probability involving it:

P( Pr (d ) > γ ) = P( X σ > β )

Chosen to give a desired quality of service


Typical Macrocell Characteristics
[not real data]
-60 .
. ... ..
... ... . . .
..
-70
.. ... ..

.
. .. . .. .
. . . .. .. . .... ... . . . .. . ...

..
Total Path Loss [-dB]

. .. . . .. . .
. . ..
. . . . . . ... .. .
.
.
-80
. ..... . ... . . . .
. . .
.
. . . . . The set of average
. .. ... ..... . . . . .
.
... ... .
. .. . . .
. . ... . .
... . . . . losses measured
..

. .
. . .... .. . . .
-90
. . . . .
.
.
. . ..
.... ... . ... ... ...... . . . at about 4km

. . . ........ . .

. . . . .. ..
[10log10(4)=6]

.
.
-100
.. ... .. . .
..

.
. . .. .. . . .. ..
.. . . .
.. . .
.
.. . ... .. . . . ..
.
. . .
.... . ... . .
.
-110
.

-120
0 1 2 3 4 5 6 7 9 10

10log10(Distance from Base Station [km])


Path Loss Assumptions
•  The mean loss in dB follows the power law :

⎛ d ⎞
L(d ) = L(d o ) + 10n log10 ⎜⎜ ⎟⎟
⎝ d o ⎠
•  The measured loss in dB varies about this mean
according to a zero-mean Gaussian RV, Xσ, with
standard deviation σ

⎛ d ⎞
L(d ) = L(d o ) + 10n log10 ⎜⎜ ⎟⎟ + X σ
⎝ d o ⎠
Typical Data Characteristics
[not real data]
-60 .
. ... ..
... ... . . .
..
-70
.. ... ..

.
. .. . .. . Best Fit
. . . .. .. . .... ... . . . .. . ...

..
Total Path Loss [-dB]

. .. . . .. . .
Path Loss
. . ..
. . . . . . ... .. .
.
.
-80
. ..... . ... . . . .
. . .
. Exponent:
. . . . . n=4
. .. ... ..... . . . . .
.
... ... .
. .. . . .
. . ... . .
... . . . .
..

. .
. . .... .. . . .
-90
. . . . .
.
.
. . ..
.... ... . ... ... ...... . . .
. . . ........ . .

. . . . .. ..
.
.
-100
.. ... .. . . σ is usually
..

.
. . .. .. . . .. ..
.. . . . 5-12 dB for
.. . .
.
.. . ... .. . . . ..
. mobile comm
. . .
.... . ... . .
.
-110
.

-120
0 1 2 3 4 5 6 7 9 10

10log10(Distance from Base Station [km])


Probability Calculation
•  Since Xσ is Gaussian, we need to know how to calculate
probability involving Gaussian RVs

P( X σ > β )
Q Function
•  If X is a Gaussian RV with mean α and standard deviation
σ, then
⎛ b − α ⎞
P( X > b) = Q⎜ ⎟
⎝ σ ⎠
where Q is a function defined as

1
+∞
⎛ x 2 ⎞
Q( z ) = ∫z exp⎜⎜⎝ − 2 ⎟⎟⎠dx

The Problem with Q
•  The integrand of Q has no antiderivative
•  Q is found tabulated in books
•  Q can be calculated using numerical integration
What is Log-normal Shadowing?
•  If Y is a Gaussian RV and Z is defined such that Y=logZ,
then Z is a log-normal RV
•  Shadowing is log-normal shadowing when the path loss in
dB is Gaussian; this means that the path loss expressed
as a ratio is log-normal
Inverse Q Problems

•  Sometimes, the probability is specified and we


must find one of the parameters in the
argument of Q
⎛ b − α ⎞
P( X > b) = Q⎜ ⎟
⎝ σ ⎠
•  Suppose the value of P ( X
> b)is given, along
with values of b and α. Solve for σ

•  Must look up the argument of Q that gives the
specified value.
Example Inverse Q Problem
•  Suppose the mean of the local average received powers at a certain
distance is -30dBm, that the standard deviation of shadow fading is 9
dB, and that the observed received power is above the threshold 95%
of the time. What is the threshold power?

•  Q is usually tabulated for arguments of 0.5 and less, so we must use


the fact that ⎛ b − (−30) ⎞
P( Pr > b) = Q⎜ ⎟ = 0.95
⎝ 9 ⎠
•  The argument of Q that yields 0.05 is about 1.65

Q(z ) = 1 − Q(− z)
b + 30
− = 1.65, and b = −44.85 dBm
9
Boundary Coverage
•  Suppose that a cell has radius R and γ is the
minimum acceptable received power level
•  Then P( Pr ( R) > γ ) is the “likelihood of coverage”
at the boundary of the cell
•  P( Pr ( R) > γ ) is also the “fraction of time” that a
mobile’s signal is acceptable at a distance R from
the transmitter, assuming the car moves around
that circle
Percentage of Useful Service Area
•  By integrating these probabilities over all the circles within
a disk, one can compute the fraction of the area within the
cell that will have acceptable power levels

2π R
1
U (γ ) = 2 ∫ ∫ P( P (r ) > γ ) rdrdθ
r
πR 0 0
Integral Evaluated
•  Assuming log-normal shadowing and the power
path loss model, the fraction of useful service
area is

1 ⎛ ⎛ 1 − 2ab ⎞⎡ ⎛ 1 − ab ⎞⎤ ⎞


U (γ ) = ⎜⎜1 − erf (a) + exp⎜ 2 ⎟⎢1 − erf ⎜ ⎟⎥ ⎟⎟
where 2 ⎝ ⎝ b ⎠⎣ ⎝ b ⎠⎦ ⎠

γ − Pr ( R) 10n log10 e
a= and b=
σ 2 σ 2
The Error Function
•  erf(x) is another form of the Gaussian integral (like
Q(x))
•  erf(x) has odd symmetry, with extreme values ±1.

erf1(x)
1
x
2 −t 2
erf ( x) = ∫e dt x
π 0
-1

•  Note that some authors may define erf differently


erf and Q
•  The erf function and Q are related:

( )
erf ( z ) = 1 − 2Q 2 z
When the Average Boundary Power is
Acceptable

•  Suppose
Pr (R) =. γThen
we may use this
graph from
[Rappaport ’96]
to figure the
percent useful
service area
Summary
•  The logs of local averages of received power (or
path loss) tend to be Gaussian when the
ensemble is all Tx-Rx locations with the same
distance in the same type of environment
•  The mean local average path loss follows the
standard power model (proportional to 10logdn)
•  Can use Q or erf to calculate the likelihood of
boundary coverage or the percent of useful
service area
References
•  [Rapp, ’96] T.S. Rappaport, Wireless Communications,
Prentice Hall,
•  [Saunders,`99] Simon R. Saunders, Antennas and
Propagation for Wireless Communication Systems, John
Wiley and Sons, LTD, 1999.

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