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13
Notes:
1. This is the maximum voltage that can be applied across the Di eren-
tial Transmitter Data Inputs to prevent damage to the input ESD pro-
tection circuit.
2. The outputs are terminated with 50 connected to VCC -2 V.
3. The power supply current needed to operate the transmitter is pro-
vided to di erential ECL circuitry. This circuitry maintains a nearly
con stant current ow from the power supply. Constant current op-
eration helps to prevent unwanted electrical noise from being gen-
erated and conducted or emitted to neighboring circuitry.
4. This value is measured with the out puts terminated into 50
W connected to VCC - 2 V and an Input Optical Power level of
-14 dBm average.
5. The power dissipation value is the power dissipated in the receiver
itself. Power dissipation is calcu lated as the sum of the products of
supply voltage and currents, minus the sum of the products of the
output voltages and currents.
6. This value is measured with respect to VCC with the output termi-
nated into 50 connected to VCC - 2 V.
7. The output rise and fall times are measured between 20% and 80%
levels with the output connected to VCC -2 V through 50 .
8. These optical power values are measured with the following condi-
tions:
• The Beginning of Life (BOL) to the End of Life (EOL) optical
power degradation is typically 1.5 dB per the industry con-
vention for long wavelength LEDs. The actual degradation
observed in Avago Technologies’ 1300 nm LED products is
< 1 dB, as speci ed in this data sheet.
• Over the speci ed operating voltage and temperature ranges.
• With 25 MBd (12.5 MHz square-wave), input signal.
• At the end of one meter of noted optical ber with cladding
modes removed.
The average power value can be converted to a peak power value by
adding 3 dB.
9. The Extinction Ratio is a measure of the modulation depth of
the optical signal. The data “1” output optical power is com-
pared to the data “0” peak output optical power and expressed
in decibels. With the transmitter driven by a 25 MBd (12.5 MHz
square-wave) input signal, the average optical power is mea-
sured. The data “1” peak power is then calculated by adding
3 dB to the measured average optical power. The data “0” output
optical power is found by measuring the optical power when the
transmitter is driven by a logic “0” input. The extinc tion ratio is the
ratio of the optical power at the “1” level compared to the optical
power at the “0” level expressed in decibels.
10. The transmitter will provide this low level of Output Optical Power
when driven by a logic “0” input. This can be useful in link trouble-
shooting.
11. The relationship between Full Width Half Maximum and RMS values
for Spectral Width is derived from the assumption of a Gaussian
shaped spectrum which results in a 2.35 X RMS = FWHM relation-
ship. The optical rise and fall times are measured from 10% to 90%
when the transmitter is driven by a 25 MBd (12.5 MHz square-wave)
input signal. The ANSI T1E1.2 committee has designated the pos-
sibility of de ning an eye pattern mask for the transmitter optical
output as an item for further study. Avago Technologies will incor-
porate this requirement into the speci cations for these products if
it is de ned. The AFBR-5805 products typically comply with the tem-
plate require ments of CCITT (now ITU-T) G.957 Section 3.2.5, Figure
2 for the STM-1 rate, excluding the optical receiver lter normally
associated with single mode ber measurements which is the likely
source for the ANSI T1E1.2 committee to follow in this matter.
12. Systematic Jitter contributed by the transmitter is de ned as the
com bination of Duty Cycle Distortion and Data Dependent Jitter.
Systematic Jitter is measured at 50% threshold using a 155.52 MBd
(77.5 MHz square-wave), 27 -1 psuedo random data pattern input
signal.
13. Random Jitter contributed by the transmitter is speci ed with a
155.52 MBd (77.5 MHz square-wave) input signal.
14. This speci cation is intended to indicate the performance of the
receiver section of the transceiver when Input Optical Power signal
characteristics are present per the following de nitions. The Input
Optical Power dynamic range from the minimum level (with a
window time-width) to the maximum level is the range over which
the receiver is guaranteed to provide output data with a Bit Error
Ratio (BER) better than or equal to 1 x 10-10.
• At the Beginning of Life (BOL)
• Over the speci ed operating temperature and voltage ranges
• Input is a 155.52 MBd, 223 - 1 PRBS data pattern with 72 “1”s and
72 “0”s inserted per the CCITT (now ITU-T) recommenda tion G.958
Appendix I.
• Receiver data window time-width is 1.23 ns or greater for the
clock recovery circuit to operate in. The actual test data window
time-width is set to simulate the e ect of worst case optical input
jitter based on the transmitter jitter values from the speci cation
tables. The test window time-width is AFBR-5805 3.32 ns.
• Transmitter operating with a 155.52 MBd, 77.5 MHz square-wave,
input signal to simulate any cross-talk present between the trans-
mitter and receiver sections of the transceiver.
15. All conditions of Note 14 apply except that the measurement is
made at the center of the symbol with no window time-width.
16. Systematic Jitter contributed by the receiver is de ned as the
combina tion of Duty Cycle Distortion and Data Dependent Jitter.
Systematic Jitter is measured at 50% threshold using a 155.52 MBd
(77.5 MHz square-wave), 27 - 1 psuedo random data pattern input
signal.
17. Random Jitter contributed by the receiver is speci ed with a 155.52
MBd (77.5 MHz square-wave) input signal.
18. This value is measured during the transition from low to high levels
of input optical power.
19. This value is measured during the transition from high to low levels
of input optical power.
20. The Signal Detect output shall be asserted within 100 μs after a step
increase of the Input Optical Power.
21. Signal detect output shall be de-asserted within 350 μs after a step
decrease in the Input Optical Power.
22. The AFBR-5805 transceiver complies with the requirements for the
trade-o s between center wavelength, spectral width, and rise/fall
times shown in Figure 9. This gure is derived from the FDDI PMD
standard (ISO/IEC 9314-3 : 1990 and ANSI X3.166 - 1990) per the de-
scription in ANSI T1E1.2 Revision 3. The interpretation of this gure is
that values of Center Wavelength and Spectral Width must lie along
the appropriate Optical Rise/Fall Time curve.