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when computing the algebra.
Friis’ formula also can be converted to EIN and T by
using the definitions in equation 12 and equation 13 on
page 9:
equation 21,
EINTOTAL, mW/Hz =
EIN2 mW/Hz – KTO
EIN1, mW/Hz + .
. ------------------------------------------------..
G1, RATIO
equation 22,
T1+ T2
TTOTAL = ------------------------
G1, RATIO
Unconverted Noise and SNR
The noise phenomena described in the previous section
all occur independent of the presence of an RF signal;
however, there is another class of noise
phenomena that occur only when a signal is present.
Such noise is present at low frequencies even without
a signal, but is translated to the neighborhood of the
signal when the light is modulated, as shown in Figure
11. This upconverted noise may reduce the signal to
noise ratio (SNR, C/N, or CNR) below what would be
calculated if only the EIN was considered. Fabry-Perot
lasers are especially susceptible to this noise and this
is reflected in their SNR specification.
For a Fabry-Perot laser, this low-frequency noise
results largely from mode partition noise, which
increases with fiber length and modulation frequency.
For DFB lasers there is only one optical mode (or
wavelength) so these effects are absent. The remaining
low-frequency noise for DFBs primarily results from
Rayleigh scattering in the fiber, which only becomes
apparent for links on the order of 20 km or more and for
high SNRs. These upconverted noise sources are
described in more detail in the sections on Reflections
and Interferometric Noise, page 24, and Distributed-
Feedback (DFB) vs. Fabry-Perot (FP) Lasers, page 25.
POWER
SIGNAL
LOW-FREQUENCY
SIDEBOARD
NOISE
NOISE
1 GHz 10 GHz
FREQUENCY
1-1222F
Figure 11. Effects of Unconverted Low-Frequency Noise on SNR
Agere Systems Inc.
Application NoteApril 2001 RF and Microwave Fiber-Optic Design Guide
Link Design Calculation (continued)
Noise-Equivalent Bandwidth
The SNR of the link depends not only on the RF signal
level outlined above, but also on the noise-equivalent
bandwidth. Wider channel widths will include more
noise power and thus reduce the SNR. Although the
link may be passing many channels over a wide band,
the receiver can be tuned to a single channel within this
band. This single-channel bandwidth is important in
determining the SNR and, in the next section, the
dynamic range.
equation 23,
NoiseCHANNEL = EINdBm/Hz + BWdB, Hz
Dynamic Range and Distortion
While the noise floor determines the minimum RF signal
detectable for a given link, non-linearizes in the
laser and amplifiers tend to limit the maximum RF signal
that can be transmitted. For links transmitting a single
tone where there is little concern for it interfering
with other signals, the 1 dB compression point is generally
used to specify the dynamic range. For links transmitting
a larger number of signals, the third-order
intercept point is frequently used to calculate the spur-
free dynamic range. Both definitions are discussed
below.
1 dB Compression Point
The most straightforward limitation on the power of an
input signal is the 1 dB compression point, P1dB. At this
RF input power, the output signal is 1 dB less than
what would be predicted by the small signal gain of the
link. Returning to the L-I curve of the transmitter, Figure
2 on page 4, it can be seen that once the magnitude of
the signal approaches that of the bias current, the signal
will clip at the lower level of the curve. This limit
defines the 1 dB dynamic range, DR1dB, as follows:
equation 24,
DR1dB = P1dB – NoiseCHANNEL
DR1dB = P1dB – EINdBm/Hz – 10 log (BWHz)
Third-Order Intercept and Spur-Free Dynamic
Range
A more precise treatment for a large number of carriers
uses the third-order intercept. Even in the middle of the
linear portion of a laser’s L-I curve, non-idealities distort
the output and cause higher order, intermodulation
signals. In particular, if two equilevel sinusoidal tones
at f1 and f2 modulate the fiber-optic link, third-order distortion
products are generated at 2f1– f2 and at 2f2 – f1,
as shown in Figure 12. The magnitude of these distortion
products expressed in dBm has a slope of three
when plotted against the input or output power level, as
shown in Figure 13 on page 14.
2f1 – f2 f1 f2 2f2 – f1
f2 – f1
INTERMODS
CARRIER
SIGNALS
C/IRF POWER (dB)
FREQUENCY
1-1223F
Figure 12.Third-Order Intermodulation Distortion Spectrum
Agere Systems Inc.
Application Note
RF and Microwave Fiber-Optic Design Guide April 2001
Link Design Calculation (continued)
NOISE LEVEL
THIRD-ORDER
DISTORTION
THIRD-ORDER
INTERCEPT
1 dB COMPRESSION
FUNDAMENTAL
SDFR
–104 dBm 35 dBm
(INPUT TOI OR IIP3)
–144 dBm
–5 dBm (OUTPUT TOI)
1-1224F
Figure 13. Third-Order Intercept and Spur-Free Dynamic Range
To quantify this effect, the slopes of the output signal
and distortion terms are extrapolated to higher power
until they intercept. The input power corresponding to
this intersection is defined as the input third-order intercept
point (IIP3 or input TOI), which can be calculated
by:
equation 25,
, ----------
IIP3dBm = SIN dBm + .
. -------C --------.
. /2
I2 TONE, dB
SIN, dBm is the input power of one of the carriers and
C/IdB is the ratio of the output power of the carrier to
that of one of the intermodulation distortion signals.
(For Agere Systems’ components, the input TOI rather
than the output TOI is usually specified because the
input TOI will be independent of the link gain. To find
the output TOI, simply add the input TOI to the link gain
in dB.) Equation 25 also can be used to approximate
the worst-case distortion terms for a given input power.
For example, if the IIP3 of a transmitter is 35 dBm and
a pair of signals is input with –5 dBm in each, then the
third-order terms will be 80 dB below these at
–85 dBm.
equation 26,
C/I2 TONE, dB = 2 (IIP3dBm –SIN, dBm)
C/I2 TONE, dB = 2 (35 dBm – (–5 dBm))
C/I2 TONE, dB = 80 dB
An important note to make is that this IIP3 power level
is never measured directly because it is strictly a small
signal linearity measurement. The IIP3 of a laser also
does not follow the traditional relationship observed in
amplifiers because it is roughly 10 dB above the 1 dB
compression point. For lasers, the difference between
these two powers is very dependent on both the frequency
and the dc bias current. Additionally, some
transmitters include predistorters, which specifically
improve the IIP3 without necessarily affecting the 1 dB
compression point.
Once the IIP3 is determined, the spur-free dynamic
range (SFDR) can be calculated. The SFDR corresponds
to the case of a link transmitting two input signals
of equal power. The SFDR is defined as the range
of the two input signals in which the signals are above
the noise floor and the third-order products are below
the noise floor. Graphically, this is shown in Figure 13.
If the noise floor is lowered either by using a quieter
laser or by operating over a narrower frequency band
then the SFDR will increase at a 2/3 rate, which is the
difference between the slope of the output signal and
distortion curves. In dB this gives:
equation 27,
SFDR = 2/3 (IIP3dBm – NoiseCHANNEL) (dB – BW)2/3
SFDR = 2/3 (IIP3dBm – EINdBm/Hz – 10 log BW) (dBHz2/
3)
For example, a link with an IIP3 of 35 dBm and an EIN
of –130 dBm/Hz would have a SFDR of 110 dB-Hz2/3
over a 1 Hz bandwidth. If the same link had a bandwidth
of 1 kHz, then its SFDR would be 90 dB-kHz2/3.
The SFDR value that results from these calculations
can be applied to either the input or output.
Agere Systems Inc.
Application NoteApril 2001 RF and Microwave Fiber-Optic Design Guide
Link Design Calculation (continued)
Large Number of Carriers
If a large number of carriers (or channels) are transmitted
through a link, then, in certain situations, the distortion
products can be higher than those predicted by the
two-tone IIP3 and SFDR. In particular, when the input
channels are evenly spaced, several different inter-
modulation tones may add together at the same frequency,
creating a stronger third-order term than what
would be produced by only two carriers. To approximate
the increase in the C/I, the following equation is
commonly used:
equation 28,
C/ITOTAL, dB = C/I2 TONE, dB – [6dB + 10 log (x)]
where x is a counting term that accounts for the overlap
of intermods, and the 6 dB term normalizes the result
to the two-tone case. This equation assumes that all of
the input carriers are equally spaced, add in power (not
voltage), and have equal powers. If they are not
equally spaced, then the two-tone calculations of the
section on Third-Order Intercept and Spur-Free
Dynamic Range, page 13, will be more appropriate.
Table 1. Carrier and Counting Term Calculations
Carriers x 6 dB + 10 log (x)
2 0.25 0 dB
3 1 6 dB
4 2.3 9.6 dB
5 4.5 12.5 dB
6 7.5 14.8 dB
7 11.5 16.6 dB
8 15.5 17.9 dB
9 20 19.0 dB
10 26 20.1 dB
11 33 21.2 dB
12 40 22.0 dB
13 48 22.8 dB
14 57 23.6 dB
15 67 24.3 dB
16 77 24.9 dB
n > 16 ~ (3/8) n2 6 dB + 10 log ((3/8) n2)
Placement of Amplifiers
For optical links that incorporate amplifiers, the amount
of distortion produced will be affected by where the
amplifiers are placed. Specifically, a trade-off must be
made between the noise and distortion performance of
the link. Placing an amplifier before the transmitter
raises the signal above the noise floor and, therefore,
lessens the noise figure of the link. However, if the
amplification is too large, then the transmitter or the
amplifier itself may begin to distort the signal. To avoid
such distortion some intermediate level pre-amp is
chosen appropriate to the given application. If necessary,
another amp after the receiver can then be used
to provide any additional gain.
Example
With all of the critical quantities defined, the perfor-
mance for a typical link can now be predicted. As an
example, consider an X-band antenna that needs to be
remotely operated 5 km from the receiver electronics
and has the following RF requirements:
Frequency range: 7.9 GHz to 8.4 GHz,
Five channels,
Channel width = 35 MHz,
SCHANNEL, RF(MIN) = –60 dBm,
SCHANNEL, RF(MAX) = –35 dBm,
SNR = 12 dB,
Total link gain = 0 dB,
Input and output impedances = 50 Ω.
Transmitter and Receiver Choice
Several transmitter/receiver pairs cover the range of
interest. For this example, the minimum data sheet
specifications for a typical DFB transmitter are used.
(Because performance varies for different products,
other values can be appropriate, depending on the
specific transmitter chosen.)
EINLASER < –120 dBm/Hz
PLASER > 2.4 mW
IIP3 > +25 dBm
P1 dB > +13 dBm
dc modulation gain > 0.06 mW/mA
For the receiver, consider one that is resistively
matched to 50 Ω and has no built-in amplifiers:
RPD > 0.75 mA/mW
ηRx, RF > 0.375 mA/mW
Throughout the example, these minimum specification
values will be used with the understanding that the
actual link would be expected to perform better than
the final answers.
Agere Systems Inc.
Application Note
RF and Microwave Fiber-Optic Design Guide April 2001
Link Design Calculation (continued)
Gain
The first thing to consider is the gain. Since the transmitter
is resistively matched for broadband operation,
its RF efficiency will be approximately equal to the
modulation gain of 0.06 mW/mA. The optical losses
can be determined with:
equation 29,
LOPT, dB = (fiber length) . (fiber attenuation) +
(# connectors) . (connector loss)
0.4 dB (OPT)
, --
LOPT dB = (5 km )..
. ------------------------------..
+ ()2 .(0.5 dB max )
km
LOPT, dB = 3 dB.
Substituting these values into equation 4 on page 6
gives for the gain of the optical transmitter, receiver,
and fiber:
equation 30,
GOPTICAL LINK = 20 log(ηTx, RF(ηRx, RF) – 2 LOPT, dB +
10 log(ROUT/RIN)
GOPTICAL LINK = 20 log [(0.06 mW/mA)
(0.375 mA/mW)] – 2 x 3 dB + 0
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