IBBCAES

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INCOHERENT BROADBAND CAVITY ENHANCEMENT ABSORPTION SPECTROSCOPY FOR TRACE GAS DETECTION

Transcript of IBBCAES

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INCOHERENT BROADBAND CAVITY ENHANCEMENT ABSORPTION SPECTROSCOPY

FOR TRACE GAS DETECTION

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Contents

Nitrate – some factsConventional vs Cavity enhanced

absorption spectroscopyIBBCEASExperiment

- Instrumental setup- Calibration

Results from lab measurementsConclusion

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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.

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The chemistry of the night-time atmosphere

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• 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

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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.

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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

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Cavity – Enhanced Absorption Spectroscopy

Sample

High reflectivity plano-concave dielectric mirrors

(typically R > 99.95% in the wavelength of interest)

Detector

Length = b

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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)

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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)

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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

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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)

+++

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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

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EXPERIMENTAL SETUP

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Lab Setup: Transmitter Unit

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Lab Setup: Intermediate Unit

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Lab Setup: Receiver Unit

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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:

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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)

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Wavelength Calibration585.249

585.103

703.137

703.241

Neon lamp lines (NIST, USA) Measured Neon lamp lines using AvaSpec 3648

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Results: NO3 Measurement

Intensity of cavity signal with N2 gas inside the cavity

Intensity of cavity signal with NO3 gas inside the cavity

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Results: NO3 Measurement

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α' and least squares fit for α’

Results: NO3 Measurement

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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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THANK YOU