DOAJ Open Access 2020

An intercomparison of CH<sub>3</sub>O<sub>2</sub> measurements by fluorescence assay by gas expansion and cavity ring-down spectroscopy within HIRAC (Highly Instrumented Reactor for Atmospheric Chemistry)

L. Onel A. Brennan M. Gianella J. Hooper N. Ng +6 lainnya

Abstrak

<p>Simultaneous measurements of <span class="inline-formula">CH<sub>3</sub>O<sub>2</sub></span> radical concentrations have been performed using two different methods in the Leeds HIRAC (Highly Instrumented Reactor for Atmospheric Chemistry) chamber at 295&thinsp;K and in 80&thinsp;mbar of a mixture of <span class="inline-formula">3:1</span> <span class="inline-formula">He∕O<sub>2</sub></span> and 100 or 1000&thinsp;mbar of synthetic air. The first detection method consisted of the indirect detection of <span class="inline-formula">CH<sub>3</sub>O<sub>2</sub></span> using the conversion of <span class="inline-formula">CH<sub>3</sub>O<sub>2</sub></span> into <span class="inline-formula">CH<sub>3</sub>O</span> by excess NO with subsequent detection of <span class="inline-formula">CH<sub>3</sub>O</span> by fluorescence assay by gas expansion (FAGE). The FAGE instrument was calibrated for <span class="inline-formula">CH<sub>3</sub>O<sub>2</sub></span> in two ways. In the first method, a known concentration of <span class="inline-formula">CH<sub>3</sub>O<sub>2</sub></span> was generated using the 185&thinsp;nm photolysis of water vapour in synthetic air at atmospheric pressure followed by the conversion of the generated OH radicals to <span class="inline-formula">CH<sub>3</sub>O<sub>2</sub></span> by reaction with <span class="inline-formula">CH<sub>4</sub>∕O<sub>2</sub></span>. This calibration can be used for experiments performed in HIRAC at 1000&thinsp;mbar in air. In the second method, calibration was achieved by generating a near steady state of <span class="inline-formula">CH<sub>3</sub>O<sub>2</sub></span> and then switching off the photolysis lamps within HIRAC and monitoring the subsequent decay of <span class="inline-formula">CH<sub>3</sub>O<sub>2</sub></span>, which was controlled via its self-reaction, and analysing the decay using second-order kinetics. This calibration could be used for experiments performed at all pressures. In the second detection method, <span class="inline-formula">CH<sub>3</sub>O<sub>2</sub></span> was measured directly using cavity ring-down spectroscopy (CRDS) using the absorption at 7487.98&thinsp;cm<span class="inline-formula"><sup>−1</sup></span> in the <span class="inline-formula"><i>A</i>←<i>X</i></span> (<span class="inline-formula"><i>ν</i><sub>12</sub></span>) band with the optical path along the <span class="inline-formula">∼1.4</span>&thinsp;m chamber diameter. Analysis of the second-order kinetic decays of <span class="inline-formula">CH<sub>3</sub>O<sub>2</sub></span> by self-reaction monitored by CRDS has been used for the determination of the <span class="inline-formula">CH<sub>3</sub>O<sub>2</sub></span> absorption cross section at 7487.98&thinsp;cm<span class="inline-formula"><sup>−1</sup></span>, both at 100&thinsp;mbar of air and at 80&thinsp;mbar of a <span class="inline-formula">3:1</span> <span class="inline-formula">He∕O<sub>2</sub></span> mixture, from which <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M26" display="inline" overflow="scroll" dspmath="mathml"><mrow><msub><mi mathvariant="italic">σ</mi><mrow class="chem"><msub><mi mathvariant="normal">CH</mi><mn mathvariant="normal">3</mn></msub><msub><mi mathvariant="normal">O</mi><mn mathvariant="normal">2</mn></msub></mrow></msub><mo>=</mo><mo>(</mo><mn mathvariant="normal">1.49</mn><mo>±</mo><mn mathvariant="normal">0.19</mn><mo>)</mo><mo>×</mo><msup><mn mathvariant="normal">10</mn><mrow><mo>-</mo><mn mathvariant="normal">20</mn></mrow></msup></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="146pt" height="18pt" class="svg-formula" dspmath="mathimg" md5hash="a0de3b239060922dec1332333490d350"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="amt-13-2441-2020-ie00001.svg" width="146pt" height="18pt" src="amt-13-2441-2020-ie00001.png"/></svg:svg></span></span>&thinsp;cm<span class="inline-formula"><sup>2</sup></span>&thinsp;molecule<span class="inline-formula"><sup>−1</sup></span> was determined for both pressures. The absorption spectrum of <span class="inline-formula">CH<sub>3</sub>O<sub>2</sub></span> between 7486 and 7491&thinsp;cm<span class="inline-formula"><sup>−1</sup></span> did not change shape when the total pressure was increased to 1000&thinsp;mbar, from which we determined that <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M31" display="inline" overflow="scroll" dspmath="mathml"><mrow><msub><mi mathvariant="italic">σ</mi><mrow class="chem"><msub><mi mathvariant="normal">CH</mi><mn mathvariant="normal">3</mn></msub><msub><mi mathvariant="normal">O</mi><mn mathvariant="normal">2</mn></msub></mrow></msub></mrow></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="34pt" height="12pt" class="svg-formula" dspmath="mathimg" md5hash="91f987b38bd7263d5c8018a9bd5e863c"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="amt-13-2441-2020-ie00002.svg" width="34pt" height="12pt" src="amt-13-2441-2020-ie00002.png"/></svg:svg></span></span> is independent of pressure over the pressure range 100–1000&thinsp;mbar in air. <span class="inline-formula">CH<sub>3</sub>O<sub>2</sub></span> was generated in HIRAC using either the photolysis of <span class="inline-formula">Cl<sub>2</sub></span> with UV black lamps in the presence of <span class="inline-formula">CH<sub>4</sub></span> and <span class="inline-formula">O<sub>2</sub></span> or the photolysis of acetone at 254&thinsp;nm in the presence of <span class="inline-formula">O<sub>2</sub></span>. At 1000&thinsp;mbar of synthetic air the correlation plot of [<span class="inline-formula">CH<sub>3</sub>O<sub>2</sub></span>]<span class="inline-formula"><sub>FAGE</sub></span> against [<span class="inline-formula">CH<sub>3</sub>O<sub>2</sub></span>]<span class="inline-formula"><sub>CRDS</sub></span> gave a gradient of <span class="inline-formula">1.09±0.06</span>. At 100&thinsp;mbar of synthetic air the FAGE–CRDS correlation plot had a gradient of <span class="inline-formula">0.95±0.024</span>, and at 80&thinsp;mbar of <span class="inline-formula">3:1</span> <span class="inline-formula">He∕O<sub>2</sub></span> mixture the correlation plot gradient was <span class="inline-formula">1.03±0.05</span>. These results provide a validation of the FAGE method to determine concentrations of <span class="inline-formula">CH<sub>3</sub>O<sub>2</sub></span>.</p>

Penulis (11)

L

L. Onel

A

A. Brennan

M

M. Gianella

J

J. Hooper

N

N. Ng

G

G. Hancock

L

L. Whalley

L

L. Whalley

P

P. W. Seakins

G

G. A. D. Ritchie

D

D. E. Heard

Format Sitasi

Onel, L., Brennan, A., Gianella, M., Hooper, J., Ng, N., Hancock, G. et al. (2020). An intercomparison of CH<sub>3</sub>O<sub>2</sub> measurements by fluorescence assay by gas expansion and cavity ring-down spectroscopy within HIRAC (Highly Instrumented Reactor for Atmospheric Chemistry). https://doi.org/10.5194/amt-13-2441-2020

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Informasi Jurnal
Tahun Terbit
2020
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DOAJ
DOI
10.5194/amt-13-2441-2020
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Open Access ✓