文章编号 :100425929 (2008) 0120091206
1 . 5μm激光雷达相干探测 CO2 与风场系统
设计
领导形象设计圆作业设计ao工艺污水处理厂设计附属工程施工组织设计清扫机器人结构设计
与仿真
陶小红 , 胡以华 , 赵楠翔 , 雷武虎
(电子工程学院 , 合肥 230037)
摘 要 : 探测低空大气 CO2 浓度的同时可以探测大气风场。采用相干探测较非相干探测具有更高的信噪
比 ,而目前 1. 5μm 波长由于在人眼安全、系统设计简单廉价等方面存在一定优势 ,使 1. 5μm 可能成为未
来探测气溶胶激光雷达的主流波长。本文阐述了激光雷达相干探测大气 CO2 与风场的原理 ,设计了 1. 5
μm 相干探测激光雷达系统 ,并对系统的信噪比进行了估算 ,得出结论 :1. 5μm 相干探测风场与 CO2 是可
行的 ,经过 3 分钟的脉冲积累 ,在 3km 处仍具有高于 10 的信噪比值。
关键词 : 相干探测 ;激光雷达 ;风场 ;CO2 浓度
中图法分类号 : TN958 文献标识码 : A
Design and Simulation of Coherent Lidar System
for Measurements of CO2 and wind
f ield with 1. 5 Microns
TAO Xiao - hong , HU Yi - hua , ZHAO Nan - xiang , L EI Wu - hu
( Elect ronic Engineering Instit ute , Hef ei 230037 , China)
Abstract : Concentration of CO2 and wind field in low altitude can be measured by coherent li2
dar simultaneously , with better signal - to - noise ratio ( SNR) than incoherent detection. At
present the 1. 5 microns laser is both eye - safe and low - cost for building a lidar system . The
1. 5 microns wavelength will also be the best candidate for the future aerosol lidar. In this pa2
per , the principles of detecting concentration of CO2 and wind field with coherent lidar are de2
scribed and the design details of coherent lidar with 1. 5 microns are given. From the simulated
SNR , it can be concluded that heterodyne detection of wind field and concentration of CO2 with
1. 5 microns is feasible and the estimated SNR at 3km distance in daylight can be better than 10
for 3 minutes integraton.
Key words : Heterodyne detection ; Coherent lidar ; Wind field ; Concentration of CO2
收稿日期 : 2007207231 ; 收修改稿日期 : 2007210218
作者简介 : 陶小红 ,男 ,汉族 ,1980 - ,电子工程学院博士研究生 ,研究方向为空间信息处理. 通信地址 :安徽省合肥市电子工程学
院 506 室 邮编 :230037. E2mail : txheei @163. com1 IntroductionConcentration of CO2 in atmosphere is closelylinked with our living environment and has be2come a concern to scientists because of its“Green2 house Effect”. Many characteristics of atmospher2ic CO2 are still not well known , thus it is neces2sary to continue to carry out measurements of CO2concentration profiles using lidar technology. . Thewind field’s detection is also important to avia2
第 20 卷 第 1 期 光 散 射 学 报 Vol120 No11
2008 年 3 月 THE JOURNAL OF L IGHT SCATTERIN G Mar1 2008
© 1994-2008 China Academic Journal Electronic Publishing House. All rights reserved. http://www.cnki.net
tions , in application areas such as atmospheric
turbulence and wind shear warning to aircrafts. It
has been shown previously that coherent lidar can
be used to detect concentration of CO2 and wind
field simultaneously[1 ] . The use of laser wave2
length at 1. 5 microns has merits of high eye safe2
ty threshold of 1 J / cm2 , no photochemistry dam2
age and low sky radiance interference. Based on
1. 5 microns fiber laser , the lidar system is simple
and stable. So 1. 5 microns will be a popular
wavelength of aerosol lidar in the future[2 ] .
2 Heterodyne detection of wind f ield and con2
centration of CO2
Heterodyne detection can provide better
SNR than direct detection and its noise - equiva2
lent - power (N EP) is close to the theoretical de2
tection limit . Intermediate f requency ( IF) signal
of heterodyne detection can shorten the receiver
bandwidth so that f requency detection is easy[3 ] .
Heterodyne detection of wind field is based
on laser Doppler theory[4 ] . When the transmitted
laser signal is backscattered by the atmosphere ,
the backscattered photons will have frequency
shift. The frequency shift is in direct proportion
to the wind radial velocity , i. e.
Δv = 2 V
c
v (1)
Where , v is the laser f requency , V is wind radial
velocity , c is light velocity andΔv is Doppler f re2
quency shift . The return signal will be mixed
with local oscillator (LO) laser beam at the detec2
tor. After f requency differentiation , the wind ve2
locity can be obtained. With the 1. 5 microns fiber
laser , the transmitted signal power can be ampli2
fied by an erbium doped fiber amplifiers ( EDFA) .
Detection of the concentration of CO2 is
based on differential absorption lidar ( DIAL ) .
After the laser pulses are transmitted and scat2
tered by aerosol , the return signal and LO laser
beam are mixed and detected. After the mixed
signals are processed , the concentration of CO2
can be obtained. The principle of DIAL consists
of using two different wavelengths with the first
one in resonance with the peak of an absorption
line (λon) of CO2 and the second one at the line
wing (λof f ) . The two wavelengths must be care2
fully chosen to prevent interference from other at2
mospheric molecule absorption lines , minimize
temperature dependence , and optimize optical
depth. The absorption curve of CO2 near 1. 5 mi2
crons is shown in Fig. 1. In this paper the wave2
lengths are chosen to be 1571. 276 nm (λon ) at
the peak of absorption curve and 1571. 434 nm
(λof f ) at the nearest line wing.
Fig. 1 Absorption curve of CO2 near 1. 5 microns
The lidar return signals can be written as[5 ] :
P( R) on =
P0 (λon)ηβ(λon , R)ΔR ( A / R2) ·
exp [ - 2∫R0 [ N w ( z )σw (λon) +α(λon , z ) ]d z ]
(2)
P ( R) of f =
P0 (λof f )ηβ(λof f , R)ΔR ( A / R2) ·
exp [ - 2∫R0 [ N w ( z )σw (λof f ) +α(λof f , z ) ]d z ]
(3)
Where , ΔR is the spatial resolution , N w is the
concentration of CO2 , R is the detection
distance , P( R) x ( x denotes on or of f ) is the
return power from R to R +ΔR , P0 (λ) is the
transmitted laser power , η is the optical
efficiency , A is the effective receiver area , and
β(λ, R) is the backscattering coefficient . The
29 光 散 射 学 报 第 20 卷
© 1994-2008 China Academic Journal Electronic Publishing House. All rights reserved. http://www.cnki.net
atmospheric extinction of the laser includes
atmospheric scattering and absorption extinction ,
i. e. N w ( z )σw (λ, z ) + α(λ, z ) ·σw (λ) is the
absorption cross section of CO2 , α(λ, z ) is the
atmospheric absorption coefficient besides CO2 .
Because λon is very close to λof f , it can be shown
that :
β(λon , R) = β(λof f , R) ,
α(λon , z ) = α(λof f , z )
After division of Eq. 2 by Eq. 3 , and taking
the logarithmic and differential operation , the
concentration of CO2 will be obtained from
equation 4 below [6 ] .
N w ( R) = 12[σw (λon) - σw (λof f ) ] ·
d
d R ln
p ( R) of f
p ( R) on (4)
3 System design of coherent measurements of
wind and CO2
Shown in Fig. 2 is the coherent lidar system
for detection of wind field and concentration of
CO2 . In the transmission portion , an external
cavity diode laser ( ECDL) is used as the master
oscillator of λon , with wavelength at 1571. 276
nm. The ECDL is composed of a diode laser , a
collimation lens , a diff raction grating and a back
reflection mirror. One surface of the diode laser is
a full - reflecting film is coated while the other
surface a half - reflecting. The full - reflecting
film and the back reflection mirror formed a reso2
nance cavity. The diff raction grating is used not
only for selecting the frequency but also to give a
feedback to compress the line - width of laser. In
order to stabilize the λon , a portion of light is
t ransmitted from the coupler to the wavelength -
meter to monitor the changes of the laser wave2
length. Actually the wavelength - meter is a stan2
dard absorption cell filled with atmospheric CO2 ,
and the feedback signal can be used to adjust the
wavelength of ECDL so that the laser can be
locked at the center of absorption peak of CO2 . A
dist ributed feedback laser (DFB) is used as the
master oscillator of λof f , whose wavelength is
1571. 434nm. DFB is a complicated servo device
in a feedback frequency - locking configuration
and composed of an etalon and a photodiode , and
a cooler with heat - sensitive resistance. The
spectral width of DFB is wider than ECDL , but
much lower price.
Fig. 2 Schematic diagram of coherent detection system
39第 1 期 陶小红 : 1. 5μm 激光雷达相干探测 CO2 与风场系统设计与仿真
© 1994-2008 China Academic Journal Electronic Publishing House. All rights reserved. http://www.cnki.net
In this system the output of DFB and ECDL
are continuous wave ( CW) laser. The two CW
lasers are turned into a pulse lasers by using a2
cousto - optic modulators ( AOM) . The control
f requency of the two AOMs are set to 10 KHz and
their pulses are alternanting. In order to avoid
disturbances among echo pulses , the pulses should
not be very close together , so the repetition fre2
quency is set below 20 KHz. The switches are
controlled to alternate between the λon and λof f
pulses. Narrow - band filter is also used to filter
out the sky background noise. As LO signal , a
portion of the laser light f rom the master oscillator
is t ransmitted by a long fiber and mixed with the
return signal at the detector. After the signal am2
plification , and digitization , the acquired data are
processed , the concentration of CO2 are calculated
from the mixed signal. After f requency differenti2
ation , wind velocity can also be obtained. In GaAs
PIN photodiode is used as the detector. The
length of the long fiber should be chosen to be
about the same as the detection distance for better
coherence.
4 Simulation of system
Heterodyne detection needs two balance de2
tectors. That is to say the two photodiodes should
be identical. When LO signal power is higher
than background noise power , the noise of hetero2
dyne detection mainly comes from shot noise. As2
suming that the responsivity is χ, the bandwidth
of detector is B , LO signal power is Pl , echo sig2
nal power is Ps , background radiance power is
Pb , the number of pulses accumulation is M ,
work temperature is T and resistance is R , the
SNR of heterodyne detection can be written as[7 ]
S M R = M ·
(2χ Ps Pl ) 2
2 B [χe ( Ps + Pl + Pb) + 2 K T/ R) ] (5)
Where e is electronic charge , K is Boltzman con2
stant . The echo signal power can be written as ,
Ps ( R) = P0 cτ2 η′β( R) ( A / R
2) ·
exp [ - 2∫R0 [ N w ( z )σw (λ) +α(λ, z ) ]d z ]
(6)
Where η′is optical efficiency (quantum efficiency
not included) , c is the speed of light , τ is pulse
duration.
Atmospheric extinction at 1. 5 microns can
be deduced from that of 532 nm. As has studied ,
atmospheric molecular backscattering coefficient
of 532 nm can be written asβm ( z ) = 1 . 54 ×10 - 3
exp ( - z / 7) and aerosol backscattering coefficient
can be described as βa ( z ) = 2 . 47 ×10 - 3 exp ( -
z / 2) + 5. 13 ×10 - 6exp ( - ( - z - 20) 2/ 36) . At2
mospheric molecular extinction coefficient can be
expressed asαm ( z ) =βm ( z ) ×8π/ 3 and aerosol
extinction coefficient can be given by αa ( z ) =βa
( z ) ×50 [8 ] . The relationship among molecular
backscattering coefficient , aerosol backscattering
coefficient and wavelength can be shown as[9 ]
βa (λ1 , z )
βa (λ2 , z ) =
λ1
λ2
- 1
(7)
βm (λ1 , z )
βm (λ2 , z ) =
λ1
λ2
- 4
(8)
And the relationship between backscattering
coefficient of 1571 nm and that of 532 nm is given
by
βa (1571 , z ) = 0 . 34 ×βa (532 , z ) ,
βm (1571 , z ) = 0 . 0131 ×βm (532 , z )
From the above equations , the atmospheric
backscattering coefficient and absorption
coefficient of 1571 nm can be written as ,
β( R) = 0 . 8398 ×10 - 3exp ( - R/ 2) +
1 . 74 ×10 - 6exp ( - ( R - 20) 2/ 36) +
2 ×10 - 5exp ( - R/ 7) (9)
α( z ) = 4 . 2 ×10 - 2exp ( - z / 2) +
8 . 7 ×10 - 5exp ( - ( z - 20) 2/ 36) +
1 . 67 ×10 - 4exp ( - z / 7) (10)
In order to simulate the echo signal ,
concentration of atmospheric CO2 at low altitude
can be given by ,
N w ( z ) = N 0exp ( - z / 7) (9)
Where , N 0 is 1. 048 × 1016 (cm - 3) [10 ] . The
absorption cross sections of CO2 at the wavelength
49 光 散 射 学 报 第 20 卷
© 1994-2008 China Academic Journal Electronic Publishing House. All rights reserved. http://www.cnki.net
of λon andλof f are 6. 36 ×10 - 23 (cm2) and 4. 56 ×
10 - 24 (cm2) respectively[11 ] . The background
radiance power can be expressed as ,
Pb = A
π
4θ
2η′S b (λ)Δλ (10)
Where ,θ is the field of view ( FOV) , S b (λ) is
background spectrum radiance and Δλ is the
bandwidth of narrow - band filter. With the typi2
cal parameters given by IPG Company , the SNR
of this lidar system is estimated. System parame2
ters are given in Table 1.
Table 1 Parameters of lidar system
Parameter Value Parameter Value
Output power of EDFA 5w LO power 2. 5mw
Pulse duration 100ns Repetition rate 10 KHz
Diameter of telescope 350mm Optic efficiency 0. 5
FOV 0. 5mrad Detection responsivity 0. 95A/ w
Bandwidth of filter 1nm Detection bandwidth 50MHz
Background spectrum radiance 1w/ m2srum Pulse accumulation time 3min
Temperature 273 K Resistance 50Ω
The simulated SNR of heterodyne detection
as a function of distance are shown in Fig. 3. The
solid curve corresponds to the SNR of λon and the
dashed curve is that ofλon . From Fig. 3 , it can be
seen that the SNR at 3 km distance in daylight is
still better than 10 after 3 minutes of pulses accu2
mulation. The SNR will be improved for longer
integation , measurement taken at night or detec2
tors with better sensitivities are used.
Fig. 3 Variation of SNR with distance
after 3 min pulse accumulation
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