direct analysis of secondary organic aerosol using the

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Martin Brüggemann 1,2 , Thorsten Hoffmann 1 1 Institute of Inorganic and Analytical Chemistry, Johannes Gutenberg Universität, Mainz, Germany 2 Max Planck Graduate Center with the Johannes Gutenberg Universität, Mainz, Germany ( [email protected]) A B E F Direct analysis of secondary organic aerosol using the flowing atmospheric-pressure afterglow (FAPA) ambient mass spectrometry source Overview Introduction Method C Source Characterization D the FAPA ion source consists of a ceramic discharge cell in which a Helium DC glow discharge plasma is maintained between a tip electrode and a capillary electrode exited Helium atoms and primary reagent ions can exit the discharge through the capillary electrode and enter the afterglow region where the desorption/ionization of the aerosol compounds takes place the ion source is held in place by a slightly redesigned Thermo® ESI flange; aerosol is introduced through a ¼” stainless steel tubing during operation a negative potential is applied to the inner electrode through a 5 k ballast resistor and the discharge is maintained in current controlled mode; the Helium flow is adjusted to 1 L/min with a rotameter laboratory SOA is produced by -pinene ozonolysis in a 100 L smog chamber SOA gas phase compounds are removed prior to analysis by passing the aerosol stream through an activated charcoal denuder background mass spectra Conclusions and Outlook the chemical analysis of atmospheric aerosols is still a major challenge and bound to big uncertainties in atmospheric research [1] online techniques, such as the Aerosol Mass Spectrometer (AMS, Aerodyne ® ), offer highly time- and size-resolved information but lack in chemical analysis of single organic compounds due to electron impact ionization [2] offline techniques, such as filter-sampling and subsequent analysis by LC-MS, offer almost complete chemical analysis of organic aerosols but have a very low time resolution and additional sample preparation is needed [1] here we present a new online technique for the chemical analysis of secondary organic aerosols (SOA) which uses the flowing atmospheric-pressure afterglow (FAPA) technique, offering highly time-resolved chemical information of sub-micrometer aerosol particles without additional sample preparation [3] secondary organic aerosol (SOA) accounts for a major fraction of atmospheric aerosol and has big implications for earth’s climate and human health it is formed when low volatile organic compounds (LVOCs), formed by oxidation of volatile organic compounds (VOCs), undergo gas-to-particle conversion to understand the impacts of SOA detailed knowledge about formation, properties and chemical evolution is needed [1] A B Figure 2: A) photograph of the FAPA ion source mounted on a LCQ Deca XP Plus (Thermo ® ) ion trap MS; B) Cross sectional view of the FAPA assembly. The aerosol inlet is arranged orthogonal to the MS inlet and the FAPA exit. While the original Thermo ® ESI flange was used the ESI manifold was replaced by a home-built FAPA manifold. Analysis of laboratory generated SOA Figure 1: Formation of secondary organic aerosol (SOA) by oxidation of volatile organic compounds (VOCs) and subsequent gas-to-particle conversion. temperature of the afterglow region Figure 3: A) maximum temperature of the afterglow region versus time for different current modes; B) maximum equilibrium temperature at a chosen current. temperature of the gas stream in the afterglow region was measured using a thermocouple (type K) which was placed directly in front of the exit capillary of the ion source correlation between the applied current, the time and the maximum equilibrium temperature in the afterglow region temperature shows a logarithmic behavior with time linear correlation between applied current and equilibrium temperature (3.3 °C/mA) covering approximately the range between 100 °C and 200 °C VOCs LVOCs natural and anthropogenic emissions oxidation by O 3 , OH, NO 3 e.g. carboxylic acids, esters, peroxides nucleation or condensation e.g. isoprene, terpenes, SO 2 SOA Acknowledgements m/z 62 m/z 125 m/z 149 m/z 167 m/z 279 m/z 391 Figure 4: background mass spectrum in positive ion mode: the four major signals correspond to plasticisers from the laboratory air which are known as common MS contaminants (m/z 149 = phtalic anhydride (MH + ), m/z 167 = dimethyl phtalate (MH + ), m/z 279 = dibutyl phtalate (MH + ), m/z 391 = dioctyl phtalate (MH + )). Figure 5: background mass spectrum in the negative ion mode: the signals at m/z 62 and m/z 125 correspond to the formation of NO 3 - ions in the afterglow from ambient air. The signals at m/z ratios above 400 are probably caused by polymeric compounds from built-in plastics in the ion source assembly. This work was supported by the Max Planck Graduate Center with the Johannes Gutenberg-Universität Mainz (MPGC). The background mass spectra are similar to other common atmospheric-pressure ionization techniques, such as electro spray ionization (ESI) or atmospheric-pressure chemical ionization (APCI). However, much higher signal intensities are achieved due to the higher reagent ion flux. SOA was generated in the laboratory from -pinene ozonolysis under dark and dry conditions SOA was introduced into the afterglow region of the FAPA through PTFE tubing with a flow rate of 2 L/min signals for typical -pinene oxidation products are observed in the range between m/z 150 and m/z 200, such as pinic acid (m/z 185, [M-H] - ), pinonic acid (m/z 183, [M-H] - ) and 10-hydroxypinonic acid (m/z 199, [M-H] - ) many unidentified signals at higher m/z ratios which are possibly dimeric oxidation products of -pinene 10-hydroxypinonic acid pinonic acid pinic acid Figure 6: mass spectrum in the negative ion mode (background subtracted) of laboratory-generated SOA. a new ion source for the online analysis of secondary organic aerosols based on the flowing atmospheric- pressure afterglow technique was developed and characterized first measurements with laboratory-generated aerosol were conducted further experiments are needed to improve the analysis of higher molecular weight compounds intercomparison studies with other aerosol instruments to evaluate the obtained data experiments for calibration of the ion source and measurement of detection limits for different substances application of the instrument in field measurements References: [1] T. Hoffmann, R.-J. Huang, M. Kalberer, Anal. Chem. 2011, 83, 4649-4664. [2] V. A. Lanz et al., Atmos. Chem. Phys. 2010, 10, 10453-10471. [3] J. T. Shelley, J. S. Wiley, G. M. Hieftje, Anal. Chem. 2011, 83, 5741-5748. 183 171 185 199 157

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Page 1: Direct analysis of secondary organic aerosol using the

Martin Brüggemann1,2 , Thorsten Hoffmann11 Institute of Inorganic and Analytical Chemistry, Johannes Gutenberg Universität, Mainz, Germany2 Max Planck Graduate Center with the Johannes Gutenberg Universität, Mainz, Germany( [email protected])

A

B

E

F

Direct analysis of secondary organic aerosol using the flowing atmospheric-pressure afterglow (FAPA) ambient mass spectrometry source

Overview

Introduction

MethodC Source CharacterizationD• the FAPA ion source consists of a ceramic discharge cell in

which a Helium DC glow discharge plasma is maintainedbetween a tip electrode and a capillary electrode

• exited Helium atoms and primary reagent ions can exit thedischarge through the capillary electrode and enter theafterglow region where the desorption/ionization of theaerosol compounds takes place

• the ion source is held in place by a slightly redesignedThermo® ESI flange; aerosol is introduced through a ¼”stainless steel tubing

• during operation a negative potential is applied to the innerelectrode through a 5 k ballast resistor and the discharge ismaintained in current controlled mode; the Helium flow isadjusted to 1 L/min with a rotameter

• laboratory SOA is produced by -pinene ozonolysis in a100 L smog chamber

• SOA gas phase compounds are removed prior to analysisby passing the aerosol stream through an activated charcoaldenuder

background mass spectra

Conclusions and Outlook

• the chemical analysis of atmospheric aerosols is still amajor challenge and bound to big uncertainties inatmospheric research [1]

• online techniques, such as the Aerosol MassSpectrometer (AMS, Aerodyne®), offer highly time- andsize-resolved information but lack in chemical analysisof single organic compounds due to electron impactionization [2]

• offline techniques, such as filter-sampling andsubsequent analysis by LC-MS, offer almost completechemical analysis of organic aerosols but have a verylow time resolution and additional sample preparationis needed [1]

• here we present a new online technique for thechemical analysis of secondary organic aerosols (SOA)which uses the flowing atmospheric-pressure afterglow(FAPA) technique, offering highly time-resolvedchemical information of sub-micrometer aerosolparticles without additional sample preparation [3]

• secondary organic aerosol (SOA) accounts for a majorfraction of atmospheric aerosol and has bigimplications for earth’s climate and human health

• it is formed when low volatile organic compounds(LVOCs), formed by oxidation of volatile organiccompounds (VOCs), undergo gas-to-particleconversion

• to understand the impacts of SOA detailed knowledgeabout formation, properties and chemical evolution isneeded [1]

A

B

Figure 2: A) photograph of the FAPA ion source mounted on a LCQ Deca XPPlus (Thermo®) ion trap MS; B) Cross sectional view of the FAPA assembly.The aerosol inlet is arranged orthogonal to the MS inlet and the FAPA exit.While the original Thermo® ESI flange was used the ESI manifold wasreplaced by a home-built FAPA manifold.

Analysis of laboratory generated SOA

Figure 1: Formation of secondary organic aerosol (SOA) by oxidation ofvolatile organic compounds (VOCs) and subsequent gas-to-particleconversion.

temperature of the afterglow region

Figure 3: A) maximum temperature of the afterglow region versus time fordifferent current modes; B) maximum equilibrium temperature at a chosencurrent.

• temperature of the gas stream in the afterglow region wasmeasured using a thermocouple (type K) which was placeddirectly in front of the exit capillary of the ion source

• correlation between the applied current, the time and themaximum equilibrium temperature in the afterglow region

• temperature shows a logarithmic behavior with time

• linear correlation between applied current and equilibriumtemperature (3.3 °C/mA) covering approximately the rangebetween 100 °C and 200 °C

VOCs LVOCs

natural and anthropogenic

emissions

oxidation byO3, OH, NO3

e.g. carboxylic acids, esters, peroxides

nucleation or condensation

e.g. isoprene, terpenes, SO2

SOA

Acknowledgements

m/z 62

m/z 125

m/z 149

m/z 167m/z 279

m/z 391

Figure 4: background massspectrum in positive ion mode:the four major signalscorrespond to plasticisers fromthe laboratory air which areknown as common MScontaminants (m/z 149 =phtalic anhydride (MH+),m/z 167 = dimethyl phtalate(MH+), m/z 279 = dibutylphtalate (MH+), m/z 391 =dioctyl phtalate (MH+)).

Figure 5: background massspectrum in the negative ionmode: the signals at m/z 62 andm/z 125 correspond to theformation of NO3

- ions in theafterglow from ambient air. Thesignals at m/z ratios above 400are probably caused bypolymeric compounds frombuilt-in plastics in the ion sourceassembly.

This work was supported by the Max Planck Graduate Centerwith the Johannes Gutenberg-Universität Mainz (MPGC).

The background massspectra are similar to

other common atmospheric-pressure ionization techniques, suchas electro spray ionization (ESI) or atmospheric-pressurechemical ionization (APCI). However, much higher signalintensities are achieved due to the higher reagent ion flux.

• SOA was generated in the laboratory from -pineneozonolysis under dark and dry conditions

• SOA was introduced into the afterglow region of the FAPAthrough PTFE tubing with a flow rate of 2 L/min

• signals for typical -pinene oxidation products areobserved in the range between m/z 150 and m/z 200,such as pinic acid (m/z 185, [M-H]-), pinonic acid (m/z183, [M-H]-) and 10-hydroxypinonic acid (m/z 199, [M-H]-)

• many unidentified signals at higher m/z ratios which arepossibly dimeric oxidation products of -pinene

10-hydroxypinonic acid pinonic acid pinic acid

Figure 6: mass spectrum in the negative ion mode (backgroundsubtracted) of laboratory-generated SOA.

a new ion source for the online analysis of secondaryorganic aerosols based on the flowing atmospheric-pressure afterglow technique was developed andcharacterized

first measurements with laboratory-generated aerosolwere conducted

further experiments are needed to improve the analysis ofhigher molecular weight compounds

intercomparison studies with other aerosol instruments toevaluate the obtained data

experiments for calibration of the ion source andmeasurement of detection limits for different substances

application of the instrument in field measurements

References: [1] T. Hoffmann, R.-J. Huang, M. Kalberer, Anal. Chem. 2011, 83, 4649-4664. [2] V. A. Lanz et al., Atmos. Chem. Phys. 2010, 10, 10453-10471. [3] J. T. Shelley, J. S. Wiley, G. M. Hieftje, Anal. Chem. 2011, 83, 5741-5748.

183

171 185

199

157