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Grant: Discovery Grants Program - Individual

St. Francis Xavier University

$28,000.00

Atmospheric trace gas detection using the properties of whispering-gallery mode micro-resonators

EF 2009-10

Résumé
Climate change and its consequences are one of the most important issues humanity will have to face in the coming decades. Reliable modeling can only come from an accurate knowledge of the composition of the atmosphere. This program is aimed at the development of a powerful in-situ instrument to detect pollutants in the atmosphere using a variant of tunable diode laser absorption spectroscopy. The miniature dimension of the instrument will allow an easy deployment on small balloon payloads or aircrafts for atmospheric measurement campaigns. Additionally, this new instrument will find many applications in industry (e.g., leak detection, process control systems, etc), in agriculture (e.g., emission from soils, livestock, etc) and in forensic science (e.g., detection of explosives, narcotics and other chemical substances, etc). Standard in-situ technique consists of a set of tunable diode lasers, an absorbing medium and a detector. When the laser frequency is tuned over the absorption lines of a gas, a part of the laser intensity is lost when the laser beam passes through the gas. The remaining intensity is measured by the detector at the exit of the absorbing medium and analyzed to obtain the concentration, temperature and velocity of the gaz. Despite its great sensitivity, the deployment of this technique for atmospheric measurements has been limited because it requires a long path length through heavy multi-pass cell. My plan is to use a new spectroscopic technique based on the whispering-gallery modes (WGMs) of silica micro-resonators to develop a portable sensitive infrared spectrometer for in-situ detection of trace gases. The WGMs are resonance modes in which light is confined, by internal reflection, at the surface of a circular micro-resonator. When the resonator is set inside a gas vapour and its WGM tuned over an absorption frequency of the gas, an energy loss occurs by a non-radiative transfer between the resonator and the neighbouring molecules. As this non-radiative transfer rate is considerably higher than the radiative absorption rate, we can obtain, by analyzing the energy loss, a sensitivity equivalent to those obtained by a bulk device.
Programme
Discovery Grants Program - Individual
Emplacement
Nova Scotia, Canada
Type de bénéficiaire
Academia
Type
Grant
Source
NSERC's Awards Data

Tel que publié

Application id
371442-2009
Name nom
LeBris, Karine
Department département
Physics
Organization id
83
Institution établissement
St. Francis Xavier University
Province en
Nova Scotia
Province fr
Nouvelle-Écosse
Country en
CANADA
Country fr
CANADA
Fiscal year exercice financier
2009
Competition year année de concours
2009
Award amount
28000
Program id
RGPIN
Program nane en
Discovery Grants Program - Individual
Program name fr
Programme de subventions à la découverte - individuelles
Group en
Discovery grants programs
Group fr
Programmes de subventions à la découverte
Committee code
29
Committee name en
General Physics
Committee name fr
Physique générale
Area of application code
401
Area of application group en
Environment
Area of application group fr
Environnement
Area of application en
Climate and atmosphere
Area of application fr
Climat et atmosphère
Research subject code
3101
Research subject group en
Physics
Research subject group fr
Physique
Research subject en
Atomic and molecular studies
Research subject fr
Études atomiques et moléculaires
Partie
1
Nb partie
1
Application title
Atmospheric trace gas detection using the properties of whispering-gallery mode micro-resonators
Keyword
NA
Application summary
Climate change and its consequences are one of the most important issues humanity will have to face in the coming decades. Reliable modeling can only come from an accurate knowledge of the composition of the atmosphere. This program is aimed at the development of a powerful in-situ instrument to detect pollutants in the atmosphere using a variant of tunable diode laser absorption spectroscopy. The miniature dimension of the instrument will allow an easy deployment on small balloon payloads or aircrafts for atmospheric measurement campaigns. Additionally, this new instrument will find many applications in industry (e.g., leak detection, process control systems, etc), in agriculture (e.g., emission from soils, livestock, etc) and in forensic science (e.g., detection of explosives, narcotics and other chemical substances, etc). Standard in-situ technique consists of a set of tunable diode lasers, an absorbing medium and a detector. When the laser frequency is tuned over the absorption lines of a gas, a part of the laser intensity is lost when the laser beam passes through the gas. The remaining intensity is measured by the detector at the exit of the absorbing medium and analyzed to obtain the concentration, temperature and velocity of the gaz. Despite its great sensitivity, the deployment of this technique for atmospheric measurements has been limited because it requires a long path length through heavy multi-pass cell. My plan is to use a new spectroscopic technique based on the whispering-gallery modes (WGMs) of silica micro-resonators to develop a portable sensitive infrared spectrometer for in-situ detection of trace gases. The WGMs are resonance modes in which light is confined, by internal reflection, at the surface of a circular micro-resonator. When the resonator is set inside a gas vapour and its WGM tuned over an absorption frequency of the gas, an energy loss occurs by a non-radiative transfer between the resonator and the neighbouring molecules. As this non-radiative transfer rate is considerably higher than the radiative absorption rate, we can obtain, by analyzing the energy loss, a sensitivity equivalent to those obtained by a bulk device.