IEC 61290-1-3:2015

IEC 61290-1-3 ®
Edition 3.0 2015-02
INTERNATIONAL
STANDARD
NORME
INTERNATIONALE
Optical amplifiers – Test methods –
Part 1-3: Power and gain parameters – Optical power meter method

Amplificateurs optiques – Méthodes d'essai –
Partie 1-3: Paramètres de puissance et de gain – Méthode par appareil de
mesure de la puissance optique

IEC 61290-1-3:2015-02(en-fr)
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IEC 61290-1-3 ®
Edition 3.0 2015-02
INTERNATIONAL
STANDARD
NORME
INTERNATIONALE
Optical amplifiers – Test methods –

Part 1-3: Power and gain parameters – Optical power meter method

Amplificateurs optiques – Méthodes d'essai –

Partie 1-3: Paramètres de puissance et de gain – Méthode par appareil de

mesure de la puissance optique

INTERNATIONAL
ELECTROTECHNICAL
COMMISSION
COMMISSION
ELECTROTECHNIQUE
INTERNATIONALE
ICS 33.180.30 ISBN 978-2-8322-2279-9

– 2 – IEC 61290-1-3:2015 © IEC 2015
CONTENTS
FOREWORD . 3
1 Scope . 5
2 Normative references . 5
3 Terms, definitions and abbreviations . 5
3.1 Terms and definitions . 5
3.2 Abbreviations . 6
4 Apparatus . 6
5 Test sample . 9
6 Procedure . 9
7 Calculation . 12
8 Test results . 13
Annex A (informative) Optimization of optical bandpass filter spectral width . 15
Bibliography . 16

Figure 1 – Typical arrangement of optical power meter test apparatus for
measurement . 7

INTERNATIONAL ELECTROTECHNICAL COMMISSION
____________
OPTICAL AMPLIFIERS – TEST METHODS –

Part 1-3: Power and gain parameters –
Optical power meter method
FOREWORD
1) The International Electrotechnical Commission (IEC) is a worldwide organization for standardization comprising
all national electrotechnical committees (IEC National Committees). The object of IEC is to promote
international co-operation on all questions concerning standardization in the electrical and electronic fields. To
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with the International Organization for Standardization (ISO) in accordance with conditions determined by
agreement between the two organizations.
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between any IEC Publication and the corresponding national or regional publication shall be clearly indicated in
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5) IEC itself does not provide any attestation of conformity. Independent certification bodies provide conformity
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services carried out by independent certification bodies.
6) All users should ensure that they have the latest edition of this publication.
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8) Attention is drawn to the Normative references cited in this publication. Use of the referenced publications is
indispensable for the correct application of this publication.
9) Attention is drawn to the possibility that some of the elements of this IEC Publication may be the subject of
patent rights. IEC shall not be held responsible for identifying any or all such patent rights.
International Standard IEC 61290-1-3 has been prepared by subcommittee 86C: Fibre optic
systems and active devices, of IEC technical committee 86: Fibre optics.
This third edition cancels and replaces the second edition published in 2005. This edition
constitutes a technical revision.
This edition includes the following significant technical changes with respect to the previous
edition:
a) Detail description of most parameters has been described in IEC 61290-1 and removed
from this part;
b) Description of maximum output signal power and maximum total output power are added.

– 4 – IEC 61290-1-3:2015 © IEC 2015
The text of this standard is based on the following documents:
CDV Report on voting
86C/1255/CDV 86C/1292/RVC
Full information on the voting for the approval of this standard can be found in the report on
voting indicated in the above table.
This publication has been drafted in accordance with the ISO/IEC Directives, Part 2.
A list of all parts in the IEC 61290 series, published under the general title Optical amplifiers –
1)
Test methods can be found on the IEC website.
This International Standard is to be used in conjunction with IEC-61290-1.
The committee has decided that the contents of this publication will remain unchanged until
the stability date indicated on the IEC web site under "http://webstore.iec.ch" in the data
related to the specific publication. At this date, the publication will be
• reconfirmed,
• withdrawn,
• replaced by a revised edition, or
• amended.
___________
1)
The first editions of some of these parts were published under the general title Optical fibre amplifiers – Basic
specification or Optical amplifier test methods.

OPTICAL AMPLIFIERS – TEST METHODS –

Part 1-3: Power and gain parameters –
Optical power meter method
1 Scope
This part of IEC 61290-1 applies to all commercially available optical amplifiers (OA) and
optically amplified subsystems. It applies to OA using optically pumped fibres (OFA based on
either rare-earth doped fibres or on the Raman effect), semiconductors (SOA), and
waveguides (POWA).
NOTE The applicability of the test methods described in the present standard to distributed Raman amplifiers is
for further study.
The object of this part of IEC 61290-1 is to establish uniform requirements for accurate and
reliable measurements, by means of the optical power meter test method, of the following OA
parameters, as defined in IEC 61291-1:
a) nominal output signal power;
b) gain;
c) polarization-dependent gain;
d) maximum output signal power;
e) maximum total output power.
All numerical values followed by (‡) are suggested values for which the measurement is
assured. Other values may be acceptable but should be verified.
This part of IEC 61290-1 applies to single-channel amplifiers. For multichannel amplifiers, the
IEC 61290-10 series applies.
2 Normative references
The following documents, in whole or in part, are normatively referenced in this document and
are indispensable for its application. For dated references, only the edition cited applies. For
undated references, the latest edition of the referenced document (including any
amendments) applies.
IEC 60793-1-40, Optical fibres – Part 1-40: Measurement methods and test procedures –
Attenuation
IEC 61290-1, Optical amplifiers – Test methods – Part 1: Power and gain parameters
IEC 61291-1, Optical amplifiers – Part 1: Generic specification
3 Terms, definitions and abbreviations
3.1 Terms and definitions
For the purposes of this document, the terms and definitions given in IEC 61291-1 apply.

– 6 – IEC 61290-1-3:2015 © IEC 2015
3.2 Abbreviations
ASE amplified spontaneous emission
DBR distributed Bragg reflector (laser diode)
DFB distributed feedback (laser diode)
ECL external cavity laser (diode)
FWHM full width at half maximum
LED light emitting diode
OA optical amplifier
OFA optical fibre amplifier
OSA optical spectrum analyzer
PDL polarization dependent loss
POWA planar optical waveguide amplifier
SOA semiconductor optical amplifier
4 Apparatus
A diagram of the measurement set-up is given in Figure 1.

Optical
coupler
Optical
Polarization
J1
Optical 1
dB power
controller
source
meter
(option)
Variable
optical
attenuator
Optical
power
meter
IEC
Figure 1a) Measurement of input signal power
Optical
coupler
Optical
Polarization
Optical
J1 J2
dB controller power
source
meter
(option)
Variable Optical
optical bandpass
filter
attenuator
Optical
power
meter
IEC
Figure 1b) Measurement of optical bandpass filter loss and jumper loss
Optical
coupler
Polarization
Optical
Optical J1
1 J2
controller OA power
dB
source
(option)
meter
Optical
Variable
OA
bandpass
optical
under test
filter
Optical
attenuator
power
meter
IEC
Figure 1c) Measurement of output signal power and gain
Optical
coupler
Polarization
Optical
Optical J1 J2
controller
dB OA power
source
(option) meter
Variable
OA
optical
under test
Optical
attenuator
power
meter
IEC
Figure 1d) Measurement of total output power
Figure 1 – Typical arrangement of optical power
meter test apparatus for measurement
The test equipment listed below, with the required characteristics, is needed.
a) optical source: The optical source shall be either at fixed wavelength or wavelength-
tuneable.
– 8 – IEC 61290-1-3:2015 © IEC 2015
– fixed-wavelength optical source: This optical source shall generate a light with a
wavelength and optical power specified in the relevant detail specification. Unless
otherwise specified, the optical source shall emit a continuous wave with FWHM of the
spectrum narrower than 1 nm (‡). A distributed feedback (DFB) laser, a distributed
Bragg reflector (DBR) laser, an external cavity laser (ECL) diode, a light emitting diode
(LED) with a narrow-band filter and a single line laser are applicable, for example.
The suppression ratio for the side modes for the DFB laser, the DBR laser or the ECL
shall be higher than 30 dB (‡). The output power fluctuation shall be less than 0,05 dB
(‡), which may be better attainable with an optical isolator at the output port of the
optical source. Spectral broadening at the foot of the lasing spectrum shall be minimal
for laser sources, and the ratio of the source power to total spontaneous emission
power of the laser shall be more than 30 dB.
– wavelength-tuneable optical source: This optical source shall be able to generate a
wavelength-tuneable light within the range specified in the relevant detail specification.
Its optical power shall be specified in the relevant detail specification. Unless
otherwise specified, the optical source shall emit a continuous wave with the full width
at half maximum (FWHM) of the spectrum narrower than 1 nm (‡). An ECL or an LED
with a narrow bandpass optical filter is applicable, for example. The suppression ratio
of side modes for the ECL shall be higher than 30 dB (‡). The output power fluctuation
shall be less than 0,05 dB, which may be better attainable with an optical isolator at
the output port of the optical source. Spectral broadening at the foot of the lasing
spectrum shall be minimal for laser sources and the ratio of the source power to total
spontaneous emission power of the laser shall be more than 30 dB.
b) optical power meter: It shall have a measurement accuracy better than ±0,2 dB,
irrespective of the state of polarization, within the operational wavelength bandwidth of the
OA. A maximum optical input power shall be large enough [e.g. +20 dBm (‡)]. Sensitivity
shall be high enough [e.g. –40 dBm (‡)]. A dynamic range exceeding the measured gain is
required (e.g. 40 dB).
c) optical isolator: Optical isolators may be used to bracket the OA. The polarization-
dependent loss (PDL) of the isolator shall be better than 0,2 dB (‡). Optical isolation shall
be better than 40 dB (‡). The reflectance from this device shall be smaller than –40 dB (‡)
at each port.
d) variable optical attenuator: The attenuation range and stability shall be over 40 dB (‡) and
better than  ± 0,1 dB (‡), respectively. The reflectance from this device shall be smaller
than –40 dB (‡) at each port.
e) polarization controller: This device shall be able to provide as input signal light all possible
states of polarization (e.g. linear, elliptical and circular). For example, the polarization
controller may consist of a linear polarizer followed by an all-fibre-type polarization
controller, or by a linear polarizer followed by a quarter-wave plate rotatable by minimum
of 90 ° and a half wave plate rotatable by minimum of 180 °. The loss variation of the
polarization controller shall be less than 0,2 dB (‡). The reflectance from this device shall
be smaller than –40 dB (‡) at each port. The use of a polarization controller is considered
optional, except for the measurement of polarization dependent gain, but may be
necessary to achieve the desired accuracy for OA devices exhibiting significant
polarization dependent gain.
f) optical fibre jumpers: The mode field diameter of the optical fibre jumpers used should be
as close as possible to that of fibres used as input and output ports of the OA. The
reflectance from this device shall be smaller than –40 dB (‡) at each port, and the length
of the jumper shall be shorter than 2 m.
Standard optical fibres defined in IEC 60793-2-50, B1 are recommended. However, other
fiber type may be used as input/output fiber. In this case, the type of fibre will be
considered.
g) optical connectors: The connection loss repeatability shall be better than ± 0,2 dB. The
reflectance from this device shall be smaller than –40 dB (‡).
h) optical bandpass filter: The optical bandwidth (FWHM) of this device shall be less than
3 nm (‡). It shall be either wavelength-tuneable or an appropriate set of fixed bandpass
filters. During measurement, the difference between the centre wavelength of this

bandwidth and the optical source centre wavelength shall be no more than 1,5 nm (‡). The
PDL of the bandpass filter shall be less than 0,2 dB (‡). The reflectance from this device
shall be smaller than –40 dB (‡).
NOTE 1 Optimization of optical band pass filter spectral width is discussed in Annex A.
i) optical coupler: The polarization dependence of the branching ratio of the coupler shall be
less than 0,1 dB (‡).Any unconnected port of the coupler shall be properly terminated, in
such a way as to decrease the reflectance below –40 dB (‡).
NOTE 2 The change of the state of polarization of the input light is typically negligible.
j) wavelength meter: It shall have a wavelength measurement accuracy better than 0,1 nm (‡).
If the optical source is so calibrated that the accuracy of the wavelength is better than
0,1 nm (‡), the wavelength meter is not necessary.
5 Test sample
The OA shall operate at nominal operating conditions. If the OA is likely to cause laser
oscillations due to unwanted reflections, use of optical isolators is recommended to bracket
the OA under test. This will minimize the signal instability and the measurement uncertainty.
For all parameter measurements except polarization-dependent gain, care shall be taken to
maintain the state of polarization of the input light during the measurement. Changes in the
polarization state of the input light may result in input optical power changes because of the
slight polarization dependency expected from all the optical components used, thus leading to
measurement errors.
6 Procedure
a) Nominal output signal power: The nominal output signal power is given by the minimum
output signal optical power, for an input signal optical power specified in the relevant
detail specification, and under nominal operating conditions, given in the relevant detail
specification. To find this minimum value, input and output signal power levels shall be
continuously monitored for a given duration of time and in presence of changes in the
state of polarization and other instabilities, as specified in the relevant detail specification.
The measurement procedures described below shall be followed, with reference to
Figure 1.
In order to minimize the amplified spontaneous emission (ASE) power contribution to the
signal power output from the OA, several methods may be used. The optical bandpass
filter method is given below.
1) Set the optical source at the test wavelength specified in the relevant detail
specification, measuring the input signal wavelength (e.g. with a wavelength meter).
2) Measure the branching ratio of the optical coupler through the signal power levels
exiting the two output ports with an optical power meter.
3) Measure the loss L of the optical bandpass filter and the optical fibre jumper between
bj
the OA and the optical power meter (see Figure 1(b)) by the insertion loss technique
(see Method B in IEC 60793-1-40).
4) Activate the OA under test and evaluate the ASE power level passed through the
optical filter, PASE, by measuring the optical output power from the OA, as shown in
Figure 1(c), without input signal.
NOTE 1 In large-signal conditions, the measurement of the ASE power is sometimes omitted.
NOTE 2 For consideration of measurement uncertainty, refer to the last paragraph of Annex A, which
concerns the optimization of the optical band pass filter spectral width.
5) Set the optical source and the variable optical attenuator in such a way as to provide,
at the input port of the OA, the input optical signal power (P ) specified in the relevant
in
detail specification. Record the optical power (P ) measured with an optical power
o
meter at the other (second) output port of the optical coupler, as shown in Figure 1(a).

– 10 – IEC 61290-1-3:2015 © IEC 2015
Instantly applying signal light into the active OA can cause the generation of an optical
surge which may damage the optical components. The input signal shall have
sufficiently small power to prevent the optical surge, when it is launched to the OA
initially. The input power shall be gradually increased to the specified level.
6) Keep the optical signal power at the OA input constant (Pin) during the following
measurements, by monitoring the second output port of the coupler and, if necessary,
setting the variable optical attenuator in such a way that the optical power (P ) exiting
o
the second output port of the optical coupler remains constant.
7) Connect the fibre jumpers to the input and output port of the OA under test, as shown
in Figure 1(c) and evaluate the optical output power (P ) with input signal.
out
In the case using the polarization controller, the following procedure shall be adapted.
8) Set the polarization controller at a given state of polarization as specified in the
relevant detail specification; activate the OA, and monitor, by means of the optical
power meter, the optical signal power at the output of the OA, for the specified period
of time, recording the minimum value.
9) Change the state of polarization of the input signal by means of the polarization
controller, trying to measure maximum and minimum output optical signal powers with
the optical power meter, and repeat procedure 8).
10) Repeat procedure 9) for the different states of polarization indicated in the relevant
detail specification and, finally, take the absolute minimum and maximum output
optical signal powers recorded in the various conditions: P and P .
out-min out-max
Optical connectors J1 and J2 shall not be removed during the measurement to avoid
measurement errors due to reconnection.
The measurement error shall be reduced by eliminating the effect of the ASE
simultaneously detected with the signal. This is better attainable by placing an optical
bandpass filter having the narrower passband at the output of the OA under test, as it
has been discussed in the main text. For large optical signal power levels, the optical
bandpass filter may not be necessary to achieve an accurate measurement. The use of
the optical bandpass filter is important, especially when the input signal to the OA is
small. This is because the ASE power increases as the input signal decreases.
However, if this kind of optical filter is already built in the OA, the external optical filter
is not needed. The effectiveness of the optical band pass filter is further discussed in
Annex A.
b) Gain and polarization dependent gain: As from procedures 1) to 7) in a), but this method
permits determination of the gain through the measurements of the OA input signal power
P and the OA output power P , taking into account the OA amplified spontaneous
in out
emission (ASE) power P at the signal wavelength.
ASE
11) Repeat procedures 5) to 7), with increasing input signal power gradually to the
maximum input signal power given in the relevant detail specification. Maintain the
pump power or pump current with the firstly set point. Polarization-dependent gain: as
in a), but this parameter is determined through the measurements of the OA input
signal power, P , the OA output power, P and P , taking into account the
in out-min out-max
OA amplified spontaneous emission (ASE) power, P at the signal wavelength, by
ASE
repeating all procedures at different states of polarization as specified in the relevant
detail specification.
The state of polarization of the input signal shall be changed after each measurement of
P , P and P by means of the polarization controller, so that substantially all the
in out ASE
states of polarization, in principle, are successively launched into the input port of the OA
under test.
The polarization controller shall be operated as specified in the relevant detail
specification. A possible way, when using a linear polarizer followed by a quarter-wave
rotatable plate, is the following: the linear polarizer is adjusted so that the OA output
power is maximized; the quarter-wave plate is then rotated by a minimum of 90 ° step-by-
step. At each step, the half-wave plate is rotated by a minimum of 180 ° step-by-step.

A short optical jumper at the OA input, kept as straight as possible, shall be used, in order
to minimize the change of the state of polarization induced in it by possible stress and
anisotropy.
The polarization-dependent loss of the optical connector shall be less than 0,2 dB (‡).
c) Maximum output signal power: As in a), but this parameter is determined by repeating all
procedures at different wavelengths specified in the detailed specification, and replace
procedures 1), 4), 5) with the following.
1) Set the wavelength-tuneable optical source at a test wavelength within the specified
wavelength range, measuring the input signal wavelength (e.g. with a wavelength
meter).
4) Activate OA and adjust the maximum pump power or maximum pump current of OA to
the nominal condition as specified in the relevant detail specification. When the OA
under test is integrated with control circuitry, the OA shall be tested with constant
pump power mode or constant pump current mode.
5) Set the optical source and the variable optical attenuator in such a way as to provide,
at the input port of the OA, the maximum input optical signal power P specified in
in-max
the relevant detail specification. Record the optical power P measured with an optical
o
power meter at the other (second) output port of the optical coupler, as shown in
Figure 1(a).
Instantly applying signal light into the active OA can cause the generation of an optical
surge which may damage the optical components. The input signal shall have sufficiently
small power to prevent the optical surge, when it is launched into the OA initially. The
input power shall be gradually increased to the specified level.
d) Maximum total output power: The maximum total output power is given by the highest
optical power level at the output port of the OA operating within the absolute maximum
ratings. To find this maximum value, input and output signal power levels shall be
continuously monitored for a given duration of time and in presence of changes in the
state of polarization and other instabilities, as specified in the relevant detail specification.
The measurement procedures described below shall be followed, with reference to
Figure 1.
12) Measure the branching ratio of the optical coupler through the signal power levels
exiting the two output ports with an optical power meter.
13) Set the optical source and the variable optical attenuator in such a way as to provide,
at the input port of the OA, the maximum input optical signal power P specified in
in-max
the relevant detail specification. Record the optical power P measured with an optical
o
power meter at the other (second) output port of the optical coupler, as shown in
Figure 1(a).
Putting signal light into the active OA can cause the generation of optical surge which may
damage the optical components. Input signal shall have sufficiently small power to prevent
the optical surge, when it is launched to the OA in the beginning. And the input power
shall be gradually increased to a certain level.
14) Keep the optical signal power at the OA input constant (P ) during the following
in-max
measurements by monitoring the second output port of the coupler and, if necessary,
setting the variable optical attenuator in such a way that the optical power (P ) exiting
o
the second output port of the optical coupler remains constant.
15) Connect the fibre jumpers to the input and output port of the OA under test, as shown
in Figure 1(d) and activate OA and adjust the maximum pump power or maximum
pump current of OA to the absolute maximum ratings, given in the relevant detail
specification. When the OA under test is integrated with control circuitry, the OA shall
be tested with constant pump power mode or constant pump current mode, and
evaluate the optical output power (P ) with input signal.
total-out
If the polarization controller is used, procedures 5), 6), 7) shall be followed.
16) Set the polarization controller at a given state of polarization as specified in the
relevant detail specification; activate the OA, and monitor, by means of the optical
power meter, the optical signal power at the output of the OA, for the specified period
of time, recording the minimum value.

– 12 – IEC 61290-1-3:2015 © IEC 2015
17) Change the state of polarization of the input signal by means of the polarization
controller, trying to measure maximum and minimum output optical powers with the
optical power meter, and repeat procedure 5).
18) Repeat procedure 6) for the different states of polarization indicated in the relevant
detail specification, and finally take the absolute minimum and maximum output optical
powers recorded in the various conditions: P and P .
total-out-min total-out-max
Optical connectors J1 and J2 shall not be removed during the measurement to avoid
measurement errors due to reconnection.
The measurement error shall be reduced by eliminating the effect of the ASE
simultaneously detected with the signal. This is better attainable by placing an optical
bandpass filter having the narrower passband at the output of the OA under test, as it has
been discussed in the main text. For large optical signal power levels, the optical
bandpass filter may not be necessary to achieve an accurate measurement. The use of
the optical bandpass filter is important, especially when the input signal to the OA is small.
This is because the ASE power increases as the input signal decreases. However, if this
kind of optical filter is already built in the OA, the external optical filter is not needed. The
effectiveness of the optical band pass filter is further discussed in Annex A.
7 Calculation
a) Nominal output signal power: The nominal output signal power P (in dBm) shall
sig-out-nom
be calculated as
P = 10 log (P – P ) + L (dBm) (1)

sig-out-nom 10 out ASE bj
where
P is the recorded absolute value of output optical signal power (in mW);
out
P is the recorded absolute value of output ASE power through the optical bandpass

ASE
filter (in mW);
L is the insertion loss of the optical bandpass filter and fibre jumper placed between
bj
the OA and the optical power meter (in dB).
NOTE 1 If optical bandpass filter is already built in the OA, the external optical filter is not needed. In this
case, the insertion loss L is equal to that of the fibre jumper.
bj
NOTE 2 A comparison of the measured values obtained with OSA, with the calculated values with optical
power meter using various band pass filters, is referred to in Annex A.
b) Gain: The gain G at the signal wavelength shall be calculated as
G = (P – P )/P (linear units) (2)

out ASE in
or as
G = 10 log [(P – P )/P ] (dB) (3)
10 out ASE in
If the FWHM of the filter is very narrow so that the detected P is sufficiently small, P
ASE ASE
could be omitted in the above calculation. In large-signal regime, if P is sufficiently
out
larger than P , P could be negligible with respect to P . A comparison of the

ASE ASE out
measured values obtained with OSA, with the calculated values with optical power meter
using various band pass filters, is referred to in Annex A.
NOTE 3 The small-signal regime is when the OA under test operates in the linear regime, while the large-
signal regime is in the saturated regime. The distinction between small-signal and large-signal regimes can be
confirmed by plotting G versus the input signal power. The linear regime demands the time-averaged input
signal power to be in the range in which the gain is quite independent from it (see IEC 61290-1). An input
signal power ranging from –30 dBm to –40 dBm is generally well within this range. In the saturated regime, the
signal power is large enough to well suppress the ASE.
NOTE 4 The measurement error can be better than ±0,2 dB (‡), depending mainly on the uncertainty of the
optical power meter.
c) Polarization-dependent gain: Calculate the gain values at the different states of
polarization as described in b). Calculations are processed using the following procedure.
1) Calculate the gain values at the different states of polarization, as in b).
2) Identify the maximum G and the minimum G gain as the highest and the
max-pol min-pol
lowest of all these gain values, respectively.
3) The polarization-dependent gain ∆G shall be calculated as follows
pol
∆G = G – G (dB) (4)
pol max-pol min-pol
NOTE 5 G is defined as the same as G in b). G is defined as G in which P is replaced by
min-pol max-pol out-min
P .
out-max
NOTE 6 ∆G does not necessarily indicate the possible maximum variation of the polarization
pol
dependency. This is because the attenuation through the OA under test is maximum only when each input
state of polarization simultaneously yields maximum attenuation for each component in the OA under test.
NOTE 7 The measurement error can be better than  ± 0,5 dB (‡), depending mainly on the optical power
meter polarization dependency.
The input signal power at which the parameter is specified and measured should be stated.
Larger input power is recommended considering the ASE factor contained in the output
power.
d) Maximum output signal power: Calculate the maximum output signal power P
sig-out-max
(in dBm) as in a).
e) Maximum total output power: The maximum total output power P (in dBm) shall be
out-max
calculated as
P = 10 log (P ) (dBm) (5)
out-max 10 out-max
where
P is the recorded absolute maximum value of output optical power (in mW).
out-max
8 Test results
a) Nominal optical signal power
The following details shall be presented:
1) arrangement of the test set-up
2) spectral linewidth (FWHM) of the optical source
3) indication of the optical pump power and possibly driving current of pump lasers for
OFAs, and injection current for SOAs (if applicable)
4) operating temperature (if required)
5) input signal optical power P
in
6) FWHM of the optical bandpass filter
7) central wavelength of the optical bandpass filter
8) wavelength of the measurement
9) nominal optical signal power levels P
sig-out-nom
10) change in the state of polarization given to the input signal light
b) Gain: The details 1) to 8), previously listed for the nominal optical signal power levels,
shall be presented and, in addition
11) gain
Parameters 5) and 9) may be replaced with the gain versus input optical signal power
curve.
– 14 – IEC 61290-1-3:2015 © IEC 2015
Parameters 8) and 10) may be replaced with the gain versus input signal wavelength
curve.
c) Polarization-dependent gain: The details 1) to 8), previously listed for the gain, shall be
presented and, in addition
12) polarization dependency of the optical power meter uncertainty
13) the maximum and minimum gain, G and G
max-pol min-pol
14) polarization-dependent gain
15) change in the state of polarization given to the input signal light
d) Maximum output signal power: The details 1) to 8), previously listed for the gain, shall be
presented and, in addition
16) maximum output signal power P
sig-out-max
e) Maximum total output power: The details 1) to 8), previously listed for the gain, shall be
presented and, in addition
17) maximum total output power P
out-max
Annex A
(informative)
Optimization of optical bandpass filter spectral width
The measurement uncertainty of this method depends on the choice of the band pass filter,
e.g. in terms of the spectral width (FWHM). In fact, as mentioned, the purpose of this filter is
to cancel the ASE contribution from the measurement. As such, it is intuitive that the smaller
the filter FWHM is chosen the greater is the ASE cancellation and hence the measurement
uncertainty. However, if the filter spectral width is excessively narrow, problems of alignment
between the filter central frequency and the signal frequency can arise, leading to stability
problems which can be detrimental to measurement uncertainty. These considerations
indicate that an optimal spectral width of the filter should be chosen to minimize the
measurement uncertainty.
A possible procedure to determine such an optimal filter is to calibrate this optical power
meter (OPM) method with the OSA technique (see IEC 61290-1-1), intrinsically more accurate.
For a given OA typology, OPM measurements using successively different filters (with FWHM
e.g. from 1 nm to 5 nm) can be compared with an OSA measurement. The optimal band pass
filter to be chosen will be the one which minimizes the difference between the results from the
two measurement methods.
For example, applying this calibration procedure in a numerically simulated case, the use of a
band pass filter of Lorentzian type with FWHM of 2 nm demonstrated to sufficiently cancel the
effect of ASE and achieve a difference with respect to OSA measurements result less than
only 0,05 dB. This difference increased to approximately 0,15 dB for a filter with FWHM of
5 nm. It should be noted that, while the effect of ASE can be accurately evaluated in small-
signal regime, even in large-signal regime, notwithstanding less accurate evaluation of ASE
power, the portion of ASE power becomes less significant with respect to the signal power. As
a result, an accurate OPM measurement can be maintained over entire input signal levels by
choosing an optimally narrow FWHM of band pass filter.

– 16 – IEC 61290-1-3:2015 © IEC 2015
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