interferometric signals in fiber optic methane sensors with wavelength modulation of the dfb laser...
TRANSCRIPT
lnterferometric noise in fibre optic methane sensor with wavelength modulation of the
DFB laser source.
G Stewart, A Mencaglia, W Philp and W Jinr
Department of Electronic and Electrical Engineering
University of Strathclyde
Glasgow Gl lXW
Tel: +44 (0)141 552 4400 ext. 2887
Fax: +44(0) 141 553 1955
e-mail : g. stewart@eee. strath.ac.uk
Abstract
We examine the perfornance limitations of a fibre optic methane sensor using micro-
optic GRIN lens cells in either transmission or reflective mode. We derive the worst
case values of sensitivity due to interference effects caused by reflections within the
cell as a function of the cell parameters. We also show both theoretically and
experimentally how the interference noise may be minimised by suitable choice of the
amplitude of the frequency modulation. Although, theoretically, reflective cells could
match the performance of transmission cells, in practice, transmission cells are
superior in terms of interferometric noise levels.
I Department of Electrical EngineeringThe Hong Kong Polytechnic UniversityHung Hom, Kowloon, Hong Kong.
INTRODUCTION
Recently a number of distributed feedback (DFB) lasers have been developed in the
1.2-2.0pm region specifically for trace gas monitoring [1,2]. A number of important
gases, including methane, carbon dioxide, carbon monoxide, hydrogen sulphide,
ammonia, etc., possess overtone or combination absorption lines in the near-IR and
although these lines are weak, high sensitivity detection can be obtained with the DFB
laser systems. Detection of HzS l2l, CO2l2l, Cru [3] and simultaneous detection of
CH+ and CzH2 l4l have been experimentally demonstrated. The key features of the
DFB lasers are (i) their very narrow linewidth, typically < 50MHz and hence much
less than the linewidth of a single rotational gas absorption line and (ii) the ability to
modulate the wavelenglh of the laser output through the injection current. High
sensitivity detection is obtained by wavelength or frequency modulation spectroscopy
and by monitoring first, second or higher order harmonics of the modulation
frequency in the detected output signal [1,5-9].
Currently we are developing a fibre optic multi-point sensor system for methane
detection, using several micro-optic cells with GRIN lenses, as illustrated in Figure 1.
Because of the very long coherence length of the DFB laser, multi-reflections
occurring within the cells and from fibre joints/connectors give rise to interference
signals which produce harmonics in the output indistinguishable from the gas signal.
This is a serious problem which must be dealt with for successful operation of the
sensor [10]. The effect may be reduced by the use of high quality anti-reflection
coatings and angled connectors, but the interference may still be the limiting factor in
the system performance. Additionally the cost of a multi-point system is greatly
increased if high quality GRIN lenses are specified for satisfactory operation. The
same problem has been reported by a number of other authors in optical gas sensors
employing bulk or multi-pass cells [11-15]. In these cases, special steps have been
devised to reduce the etalon fringes such as (i) the introduction of a second low-
frequency jitter [11] and low pass frltering [12], (ii) frequency modulation combined
with wavelength modulation using a triangular waveform [13,14] and more recently
(iii) the development of digital signal processing algorithms 116,17l. Similar methods
may be applied to the fibre optic system.
ln earlier work [18,19] we reported some theoretical calculations for the limitations
imposed by interferometric noise in fibre optic gas sensors using differential
absorption spectroscopy, that is, where the output is an intensity ratio at two distinct
wavelengths, one at the centre of the absorption line, the other displaced to a point
where the absorption is negligible. Here we report both ow theoretical and
experimental investigation into the interference noise specifically for the fibre optic
methane sensor using wavelength modulation of the DFB laser source. We determine
the limitations imposed on the sensitivity and demonstrate how the interference
signals depend on the operating parameters.
II SIGNAL OUTPUT FROM THE MICRO-OPTIC CELL
For the fibre optic system we assume that the dominant source of interferometric noise
will be from the micro-optic cell which may be used in either transmission or
reflectance mode, Figure 2(a) and (b). The cell length, i, is typically 5 - 25cm and is
very much less than the coherence length of the DFB laser source. The surfaces of the
GRIN lenses have reflection coefficients rt and 12 and we assume that, with anti-
reflection coatings, tt , 12 <<1 and transmission coefficient, t -1. For the reflective
cell we assume a back-reflection of tr at the inner surface of the GRIN lens and a
reflection coefficient ,,eiL- at the reflector. Additionally, the collimation/focusing
action of the GRIN lenses will not be perfect, so we should allow for a cell
(amplitude) attenuation factor ry Qt < l). The attenuation will depend on cell length
and has a typical experimental value of - 2dB power loss (ry2 - 0.6) for a transmission
cell of length 5cm with the GRIN lenses mounted in a v-groove.
Under the above conditions (low finesse Fabry-Perot cavity) we need only consider
first order reflections and the field output for the transmission cell may be written as
(see Figure 2):
Er = l,{Eo exp(-a "Cl)cos(at)+
rTlr,rrEoexp(-3a,Cl)cos[a\t- ")]] (l
4
and for the reflective cell as:
E * x r7r,Eo exp(-2a "C/)
cos[ar(r - ,) * 0,]
- rtE o cos(a;/) + rrrT'rj E o exp(-4a "Cli
cos[a{r - 2c) + 2Q -f
Note that for the reflective cell, ? coresponds to the round trip (amplitude)
attenuation factor. From equation (2) we can combine the effects of ry and r-to form
an effective cell reflectivity factor, 4, = rlt,. We denote rl? as an (intensity)
efficiency factor for light passing through a transmission cell arrd rtl the effrciency
factor for the return of light from a reflectance cell.
In th. ^bor. equations, a, is the (amplitude) attenuation coefficient for methane in the
cell, C is the methane concentration and z is the round-trip delay time of the cell,
r =2llc.
The output intensity is the time averag e < E2 > and with the assumptions that rr, rz
<< 1 and aoCl <<.1, we obtain:
* - | - o C tl+ 2ql r,rrcos(arz)
(2
and:
(3
(4h " lr - z a c 4-'; t, - n?) co4r, - O,)-2r,2 cos2(ot, - 0,)
where a: 2ao is the methane absorption coefficient and Io = Ei lZ.
In equations (3) and (4), the first term represents the methane signal while the
remaining term(s) represents the interferometric noise. We consider each term in tum
in the following two sections.
m METHANE SIGNAL
The absorption spectrum of methane in the near infrared contains a number of
individual rotational lines centred around 1660nm and labelled as P, Q and R lines.
(These correspond to the second harmonic of the fundamental methane absorption
spectrum at 3.3pm). For trace gas monitoring at atmospheric pressure, the individual
lines can be described as a Lorcntzian function (pressure-broadened line) [20] so we
may write the methane absorption coefficient as a function of wavelength or
wavenumbat, v : lf )", as:
where a. is the absorption at the line centre, vo is the wavenumber at the line centre
and 7,is the half-linewidth.
(s
6
with wavelength modulation of the DFB raser source (through moduration of theinjection current) we can write the raser output wavenum ber, vr as:
v t = (vo + Av) + dvsin(at ;)
where av is the offset of the raser output from the absorptionamplitude of the modulation and a^the modulation frequency.
Combining equations (5) anO (6) we obtain:
a(v)=ffiwhere A = A vfy and F, = 6r/y .
In order to obtain the harmonic content of theFourier series:
methane signal we expand a into the
where o0, at, o2, .....-..onare the Fourier coefficients and depen d, on / and. F, .
(6
Iine centre, dy is the
(7
(8
o - dn{r,.ir, sinlrr^, * e,)}
The magnitude of the n-th
equation(3) and (4):
harmonic of the methane signal is therefore from
(e
for the transmission and reflective cells, respectively.
The coefficients a, may easily be calculated by numerical integration and Figure 3
shows at, a2 and a3 as a function of A for F* : 1.5. To gain an idea into the
magnitude of the signals involved, consider the case where the DFB laser output is
locked to the absorption line centre (A : 0) and the second harmonic component is
used to monitor the methane concentration. From Figure 3 we see that a2: 0.32.
(Actually, the maximum value of az:0.35 is obtained when F. is increased to 2.2).
The absorption coefficient at the line centre, a*has been reported as - O.4cm-latm-l
for the Q6 line at 1665.5nm [3] and - 0.14cm-ratm-r for the R4 line at 165lnm [1].
Our measurements on the Q6 line yielded a value of - 0.25cm-latm-1. Hence if we
take a typical value of a* = 0.2cm-latm-l we obtain a second harmonic in terms of the
methane concentration in ppm.metre as:
for the transmission cell.
!,-l =6.4xppm'me*elni t,l, to6
(10
IV INTERFEROMETRIC SIGNAL
We now consider the terms in equations (3) and (4) which describe the interference
effects. Writing equation (6) for the laser output in terms of angular frequency ar
gives:
ar=@+Sossin(at,t)
where o :2rc(vo + Lv) and 5a = 2rc5v
Hence the interference term for the transmission cell from equation (3) is:
(11
h = 2172,rrrrcos {ar +lSarlsin(ar,r)} (r2
For the reflective cell, from equation (4) there are two terms contributing to the
interference effects. If the cell efficiency factor approaches IOO% (rt? -+ 1), the
second term -+ 0 and the remaining term gives interference similar to a transmission
cell (exceptthat r is replaced by 2r). Specifically, comparison of the magnitude of
the two terms shows that this is true if ,tl >>(l-r,rt,) = (1-4). nor example if the
GRIN lens has a surface reflectance of -30dB, (rr' = l0'), then the efficiency factor
of the cell, rTlneeds to be >> 97o/o. This is unlikely to be true in practice for a GRIN
lens cell; for example, with a round trip loss in the cell of 4dB and mirror reflectance
of 80%, r7l has value of only - 0.3. Hence the main contribution to interference will
be from the second term in equation (4), namely:
* - -|tt- n1)crs{.t +[6an]sin(a.r,r) - O,\ (13
We can expand equation (12) or (13) into its harmonic components using:
cos{or+fda;r]sin(at ^t)\ = Jo(5an)cos(or) -iO,sin(na *t + Q) 04n=l
where An =2J,(6an)sin(ot - 0) and 0n = 0 for n: t, 3, 5, ....., 0n = nl2 for n =
2, 4, 6,....(converts from sine to cosine).
Hence the magnitude of the rz-th harmonic of the interference is
l*1,=2qtr,r,A.
for the transmission cell and similarly for the reflective cell.
Note that ll,l=lJ,l^^*. Consider the second harmonic component from the
interference. The maximum value of Jz is - 0.5 so we have ltr l ry? trla qlr,r, for the
transmission cell and lr, I ,tlt rl= \r, I q,\(, - ,',) ror the reflective cell.
(1s
10
V SENSITIVITY LIMIT FROM INTERFERENCE
We can determine the limitations imposed on the sensitivity from interference effects
by comparing the methane signal, equation (9) and the interference signal, equation
(15). By equating the methane and the interference signals we obtain a noise
equivalent methane concentration (the minimum detectable methane concentration)
for detection at the n-th harmonic as:
2r7lr,rrA,
d -an(16
(t7
[c/]-," =
for the transmission cell and
[c/].,, =,,(t- r7i),1,
?'l ,d ran
for the reflective cell. Q.{ote the absence of the factor of 2 in equation ( 1 7) compared
with equation(16) because of the double pass in a reflective cell).
We can estimate the worst case values of [C/].in for second harmonic detection using
the typical values quoted earlier. If the surface reflectance is -30dB 1r2 :lO-3 ) then
[C/]*i" < l00ppm.metre for a transmission cell with ,i - 0.6, and < 30O0ppm.metre
for a reflective cell with r7l - 0.3. The reflectance cell is clearly much poorer in
performance. The value obtained here for the transmission cell is similar to that
derived in our earlier analysis of a system using differential absorption spectroscopy
[18, 19] where a value of 200ppm.metre was obtained for a transmission cell with
l1
4? = l. Our experiments on a fibre optic methane system employing micro-optic
transmission cells with standard GRN lenses (- -30dB reflectivity) and second
harmonic detection have indicated a resolution around 20Oppm.metre [10]. The above
results imply that to achieve a resolution of lppm.metre in a transmission cell, high
quality GRIN lenses are required with surface reflections < -50dB. This makes for
much greater expense, especially in a multipoint system and other means of dealing
with the interference noise is required.
VI REDUCTION OF INTERI'ERENCE EFFECTS
Examination of equation (14) shows that the magnitude of the interference signals
depends on the Bessel function .I,. Hence it should be possible in principle to
eliminate the interference effects for a particular harmonic by choosing an appropriate
value of the frequency modulation amplitude dar so that J,(6an) = g.
In practice the interference from a single cell cannot be totally eliminated because the
frequency modulation of the DFB laser also produces a degree of amplitude
modulation. We can take this into account as follows.
With simultaneous frequency and amplitude modulation equation (12) becomes:
1,,= 2 r7l r,rrfl + m sin(a S))cos {or + [dar] sin (ar,t)\
ry? ro
t2
(18
where rz is the amplitude modulation index, m = k6o where ,t is a constant.
(Experimentally for our DFB laser, fr - -1 .6x 10-t MH, -';
Expansion of equation (18) into its harmonics gives:
where:
I-. { @ I
;t=2r7lr,rr\Aocos(or + V)-\,l,sin(na,t * O)l (19
A, = @.r(dan) - J,-r@aflf'z sin(or + v/, - O,) eo
(21
2J,(6at)*{J,,,(6an) - J,_t@an) rl (22
vo=tan-'\1ryffi] o,
and Q,= 0 for h: 1,3,5, ....., d, = ol2 for n:2,4,6,.....'..as before.
A similar result may be obtained for the reflective cell.
13
From equation (20) it can be seen that the amplitude of the n-th harmonic may be
minimised, but not necessarily reduced to zero, by suitable choice of 6at
The above analysis has dealt with interference arising from a single cavity only. In
practice, reflections from other surfaces and fibre connections in the system will give
rise to multiple cavities as illustrated in Figure 4. This may be taken into account by
adding additional reflection terms on to equation (1) and under the assumption of
small reflectivities, t1, ri 11 1 equation (18) takes the form:
+ :2ll + *srn(, -l)>n?, r r, "or{., ,
+filar ,fsin(a ,t1\4'lo ' ,.,
which also may be expanded into harmonic components.
Vil EXPERIMENTAL OBSERVATION OF INTERFERENCE
Interference signals at first and second harmonic frequencies were experimentally
measured as a function of the frequency modulation amplitude \ot for both
transmission and reflective cells (with no methane present) in order to compare with
equation (20). For different data sets we expect the cell length to fluctuate over a few
wavelengths giving random fluctuations in r. The fluctuations in or will cause the
sine term in equation (20) to drift over a few cycles but the effect on 6atr will be
(24
t4
insignificant. Hence for each cell, four sets of measurements were taken for the full
range of 5o and the standard deviation computed. Results are shown in Figures 5-9.
Each figure shows the first and second harmonic signals experimentally measured
compared with a theoretical fit (in bold) from equation (20) for Figures 5-7 and using
equation (24) for Figures 8 and 9. (The vertical scale is arbitrary, adjusted to give best
fit between experimental and theoretical curves.)
Experimentally, the frequency modulation amplitude was varied by the application of
a sinusoidal voltage (through a 10dB attenuator) to the current driver of the laser
diode and so the horizontal scale of Figures 5-9 is given in units of millivolts (rms).
This may be related to the FM amplitude 6a as follows:
*=lT)*=lT)ff)(il* (2s
where [4] tr the current tuning rate of the DFB laser and\ r,/
i-V charucteristic.
e is the slope of its
We estimated these parameters experimentally by scanning through the Q6 line of
methane (a 3V ramp produced - 56mA current change, scanning through - 0.14nm1.
rhe values obtained *, (q) - 0.002snm/mA and (#) - lemA/v. Bearing in
mind that the voltage shown in the graphs is in millivolts (rms), applied through a
1OdB attenuator, the conversion factor is:
t5
# =[o.s ' ro'] to.oozsl ee x J) x0.32x 10-3) = 0.0r 5 GHz I mv,,,
This conversion factor was used in plotting the theoretical curves. Clearly there is
excellent agreement both in the general shape of the curves as Bessel functions and in
the positions of the minima.
As noted earlier the amplitude modulation index, m = k6a. The value of t is
obtained using the fact that the experimental slope of the power/current curve of the
DFB is 4- o.oornwmA ar an output power of 1.5mw *d f+l - 0.0025nm/rnA,5i \ r,/
giving k- -L6x10-s MHz-r.
Examination of Figures 6 and 7 for the reflective cell show that while the general
shape is well predicted by the theoretical cruves based on equation (20) for a single
cavity, there is a secondary high frequency ripple in the experimental curves. This
suggests the presence of a much longer second cavity also contributing to the
interference signal. On this basis, Figure 8 and 9 show the same experimental curves
as Figures 6 and 7, respectively, but here the theoretical curve is based on two cavities
using equation (24), as illustrated in Figure 4, the second cavity having a additional
(physical) length of 5metres (optical length 5x1.456m). This model appears to
provide a good description of the experimental data and suggests there is a secondary
reflection from a fibre connector within our experimental fibre system (FC/PC
connectors were used which introduce a back reflection of - -40dB). It is to be noted
(26
16
that while the results
evidence of a slight
reflective cells.
for the transmission cell, Figures 5 and 6, also show some
ripple, the effect is clearly much more pronounced in the
VM CONCLUSION
In this paper we have examined the limitations imposed on the sensitivity of a fibre
optic methane sensor due to interference effects. We have shown both theoretically
and experimentally how the interference signals can be reduced by choice of the
amplitude of the frequency modulation. Our experimental results indicate that
reflective-t1pe cells give poorer performance and tend to enhance interference effects
from connectors and joints within the fibre system and this is consistent with the
theoretical results. Theoretically, a reflective cell with a very high reflectance
efficiency ( ry]) could provide similar performance to a transmission cell but this
would be difficult to achieve in practice with GRIN lens systems. In a future paper we
will show how the results presented here can be used along with digital signal
processing methods to obtain accurate measurements of methane concentrations in the
f,rbre optic system.
t7
ACKNOWLEDGMENT
This work was supported by the EPSRC/DTI LINK Photonics Programme in the UK
(OMEGA Project). The authors thank Chris Tandy of Gas Measurements Instruments
(GMD and the other industrial partners, British Gas and OptoSci for helpful co-
operation.
18
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22
FIGURE CAPTIONS
l. Fibre optic multi-point methane sensor system employing micro-optic cells.
2. Micro-optic cells using GRIN lenses showing reflected beams that contribute
to interference effects in the system output
(a) transmission cell (b) reflective cell.
3. Fourier coeffrcients for first, second and third harmonics of the laser
wavelength modulation frequency as a function of fractional offset from line
centre. (Lorentzian lineshape and normalised modulation amplitude, F*: 1.5)
Reflective cell with secondary reflection from a fibre corurector.
Experimental and theoretical results for the first and second harmonic
components of interference noise as a function of the amplitude of the
frequency modulation.
5-9
23
(
l.-modulation
micro-optic cells
detector reference cell
single mode
fibre
methane concentration
at each micro-optic cell
ELECTRONICSlaser controllock-in amplifierscomputer interface
Chartl
OFFSET FROM LINE CENTRE AS MULTIPLE OF HALF-LINEWIDTH
zIIJ
Il!lJ.r.lJ
ootrllJe=-aol!l!otrJf
040
a1 .,\020
\,p\.
a3
00 0
-0.10
-0.20
-0.30
-0.40
m. 1.
.\/. \--l
4
]Ir^
(,
Page 1
5
350
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lst harmonic: 25cm transmission cellSingle cavity model
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Amplitude of frequency modulation (mV)
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