IBBCAES
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Transcript of IBBCAES
INCOHERENT BROADBAND CAVITY ENHANCEMENT ABSORPTION SPECTROSCOPY
FOR TRACE GAS DETECTION
Contents
Nitrate – some factsConventional vs Cavity enhanced
absorption spectroscopyIBBCEASExperiment
- Instrumental setup- Calibration
Results from lab measurementsConclusion
Nitrate (NO3-)
Atmospheric NO3- (NO3
-atm) is a mixture of gas
phase nitric acid, produced by the oxidation of NOx, and NO3
- salts formed by heterogeneous reactions involving NOy on aerosol surfaces
NO3- is not present in the sunlit atmosphere,
because it is rapidly destroyed by photolysis.
The chemistry of the night-time atmosphere
• A substantial portion of nitrate found in the soil, stream and ground water is of atmospheric origin
• The global nitrogen cycle has been altered by human activities:– human N2-fixation > 2 x natural fixation (annually)
• NO3- is a substantial source of new N
• The negative impacts of excess N and NO3-
input includes – shifts in biodiversity,– soil acidification and forest decline,– eutrophication of coastal waters and estuaries and – degradation of ground and surface waters
Tracing of atmospheric nitrate deposition in a
complex semiarid ecosystem by University
of California
CONVENTIONAL ABSORPTION SPECTROSCOPY
A laboratory technique used to determine the structure and concentration of a sample based on the amount and wavelengths of light that it absorbs.
It derives concentrations of absorbing species in the atmosphere by using a form of the Beer-Bouguer-Lambert Law.
Beer - Bouguer - Lambert Law
Transmittance, T is calculated as
where I0 – initial light intensity (power P0) I – transmitted intensity (power P) α’ - absorption coefficient of the sample b – path length of light through the
sample
Cavity – Enhanced Absorption Spectroscopy
Sample
High reflectivity plano-concave dielectric mirrors
(typically R > 99.95% in the wavelength of interest)
Detector
Length = b
Advantage of Cavity – Enhanced Absorption Spectroscopy
• The cavity having a length of 1m approximately could create an effective path length of 10km
This increases the sensitivity of the instrument
Iin (1-R)2(1-L) (0th pass)
Iin (1-R)2(1-L)3 R2 (1st pass)
Iin (1-R)2(1-L)2n+1 R2n (nth pass)
Types of Cavity Enhanced Absorption Spectroscopy
1. Cavity Ring Down Spectroscopy (CRDS)2. Integrated Cavity Output Spectroscopy (ICOS)3. Incoherent Broadband Cavity Enhanced
Absorption Spectroscopy (IBBCEAS)
IBBCEAS
Simple, Robust & Economic
High temporal resolution
Portable & Compact
Easy integration into
spectrometers
Applicable to fluids
Applicable over a wide spectral range
Theoretical application to
solids
Theory of IBBCEAS
Iin (1-R)2(1-L) (0)
Iin (1-R)2(1-L)3 R2 (1)
Iin (1-R)2(1-L)2n+1 R2n (n)
+++
Since R<1 and L<1
For an empty resonator with L = 0, Io = Iin (1-R) (1+R)-1
Therefore,
Assuming the losses per pass to be solely due to Beer absorption,
Theory of IBBCEAS
EXPERIMENTAL SETUP
Lab Setup: Transmitter Unit
Lab Setup: Intermediate Unit
Lab Setup: Receiver Unit
Preparation of NO3 In The Laboratory
4 HNO3(aq) + Cu (s) → Cu(NO3)2(aq) + 2 H2O(l) + 2 NO2(g)
NO2 + O3 → NO3 +O2
Using ozoniser, NO2 inside the chamber is made to undergo the following reaction:
Calibration of Mirror Reflectivity ‘R’
Low-loss optic [L(λ) < 0.001, Layertec]
500 550 600 650 700 750
0
2000
4000
6000
8000
10000
Cou
nt
Wavelengh
LLO I0
Transmission without optic (I0)
Transmission with optic (LLO)
Wavelength Calibration585.249
585.103
703.137
703.241
Neon lamp lines (NIST, USA) Measured Neon lamp lines using AvaSpec 3648
Results: NO3 Measurement
Intensity of cavity signal with N2 gas inside the cavity
Intensity of cavity signal with NO3 gas inside the cavity
Results: NO3 Measurement
α' and least squares fit for α’
Results: NO3 Measurement
CONCLUSION A simple IBBCEAS setup to detect trace gases
like NO3 is designed for the In-situ measurement.
The instrument was able to detect NO3 concentration at ppb levels.
The calculated error was about 7% - 9%. Further optimizations are required to improve
sensitive. When the instrument is used in humid
conditions, H2O absorption lines in the spectral range of interest will increase the amount of error.
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