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<article xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:oasis="http://docs.oasis-open.org/ns/oasis-exchange/table" dtd-version="3.0"><?xmltex \makeatother\@nolinetrue\makeatletter?>
  <front>
    <journal-meta>
<journal-id journal-id-type="publisher">AMT</journal-id>
<journal-title-group>
<journal-title>Atmospheric Measurement Techniques</journal-title>
<abbrev-journal-title abbrev-type="publisher">AMT</abbrev-journal-title>
<abbrev-journal-title abbrev-type="nlm-ta">Atmos. Meas. Tech.</abbrev-journal-title>
</journal-title-group>
<issn pub-type="epub">1867-8548</issn>
<publisher><publisher-name>Copernicus Publications</publisher-name>
<publisher-loc>Göttingen, Germany</publisher-loc>
</publisher>
</journal-meta>

    <article-meta>
      <article-id pub-id-type="doi">10.5194/amt-9-3851-2016</article-id><title-group><article-title>A new technique for the direct detection of HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> radicals using bromide
chemical ionization mass spectrometry (Br-CIMS):<?xmltex \hack{\break}?> initial characterization</article-title>
      </title-group><?xmltex \runningtitle{A new technique for the direct detection of HO${}_{{2}}$ radicals}?><?xmltex \runningauthor{J.~Sanchez et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Sanchez</surname><given-names>Javier</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Tanner</surname><given-names>David J.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Chen</surname><given-names>Dexian</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-6963-5205</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Huey</surname><given-names>L. Gregory</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-0518-7690</ext-link></contrib>
        <contrib contrib-type="author" corresp="yes" rid="aff1 aff2">
          <name><surname>Ng</surname><given-names>Nga L.</given-names></name>
          <email>ng@chbe.gatech.edu</email>
        <ext-link>https://orcid.org/0000-0001-8460-4765</ext-link></contrib>
        <aff id="aff1"><label>1</label><institution>School of Chemical and Biomolecular Engineering, Georgia Institute of
Technology, Atlanta, GA 30332, USA</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>School of Earth and Atmospheric Sciences, Georgia Institute of
Technology, Atlanta, GA 30332, USA</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Nga L. Ng (ng@chbe.gatech.edu)</corresp></author-notes><pub-date><day>19</day><month>August</month><year>2016</year></pub-date>
      
      <volume>9</volume>
      <issue>8</issue>
      <fpage>3851</fpage><lpage>3861</lpage>
      <history>
        <date date-type="received"><day>4</day><month>April</month><year>2016</year></date>
           <date date-type="rev-request"><day>6</day><month>April</month><year>2016</year></date>
           <date date-type="rev-recd"><day>21</day><month>July</month><year>2016</year></date>
           <date date-type="accepted"><day>22</day><month>July</month><year>2016</year></date>
      </history>
      <permissions>
<license license-type="open-access">
<license-p>This work is licensed under a Creative Commons Attribution 3.0 Unported License. To view a copy of this license, visit <ext-link ext-link-type="uri" xlink:href="http://creativecommons.org/licenses/by/3.0/">http://creativecommons.org/licenses/by/3.0/</ext-link></license-p>
</license>
</permissions><self-uri xlink:href="https://amt.copernicus.org/articles/9/3851/2016/amt-9-3851-2016.html">This article is available from https://amt.copernicus.org/articles/9/3851/2016/amt-9-3851-2016.html</self-uri>
<self-uri xlink:href="https://amt.copernicus.org/articles/9/3851/2016/amt-9-3851-2016.pdf">The full text article is available as a PDF file from https://amt.copernicus.org/articles/9/3851/2016/amt-9-3851-2016.pdf</self-uri>


      <abstract>
    <p>Hydroperoxy radicals (HO<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> play an important part in tropospheric
photochemistry, yet photochemical models do not capture ambient HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
mixing ratios consistently. This is likely due to a combination of
uncharacterized chemical pathways and measurement limitations. The indirect
nature of current HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> measurements introduces challenges in accurately
measuring HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>; therefore a direct technique would help constrain
HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> chemistry in the atmosphere. In this work we evaluate the
feasibility of using chemical ionization mass spectrometry (CIMS) and
propose a direct HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> detection scheme using bromide as a reagent ion.
Ambient observations were made with a high-resolution time-of-flight
chemical ionization mass spectrometer (HR-ToF-CIMS) in Atlanta over the
month of June 2015 to demonstrate the capability of this direct measurement
technique. Observations displayed expected diurnal profiles, reaching
daytime median values of <inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 5 ppt between 2 and 3 p.m.
local time. The HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> diurnal profile was found to be influenced by
morning-time vehicular NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions and shows a slow decrease into the
evening, likely from non-photolytic production, among other factors.
Measurement sensitivities of approximately 5.1 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 1.0 cps ppt<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> for a
bromide ion (<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>79</mml:mn></mml:msup></mml:math></inline-formula>Br<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> count rate of 10<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msup></mml:math></inline-formula> cps were observed. The
relatively low instrument background allowed for a 3<inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula> lower detection
limit of 0.7 ppt for a 1 min integration time. Mass spectra of ambient
measurements showed the <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>79</mml:mn></mml:msup></mml:math></inline-formula>BrHO<inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> peak was the major component
of the signal at nominal mass-to-charge 112, suggesting high selectivity for
HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> at this mass-to-charge. More importantly, this demonstrates that
these measurements can be achieved using instruments with only unit mass
resolution capability.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <title>Introduction</title>
      <p>Hydroperoxy radicals (HO<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> play an important role in the photochemistry
of the troposphere. They are primarily formed from the OH initiated oxidation
of CO and other volatile organic compounds (VOCs), with contributions from
ozonolysis of alkenes, nitrate radical oxidation of VOCs, and photolysis of
aldehydes (e.g., HCHO) (Geyer et al., 2003; Cooke et al., 2010; Volkamer et
al., 2010; Alam et al., 2013; Stone et al., 2014). HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> is a reservoir
species for OH, the primary daytime oxidant, and facilitates the
photochemical production of ozone via its reaction with NO. Additionally, the
relative abundance of HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> to NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> plays a critical role in the fate
of peroxy radicals (RO<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> and the production of low-volatility products
in secondary organic aerosol (SOA) formation (Orlando and Tyndall,
2012; Ziemann and Atkinson, 2012). For instance, reactions of HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> with
RO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> serve as the main source of atmospheric organic hydroperoxides,
which are important constituents of SOA (Docherty et al., 2005).</p>
      <p>HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> is also critical for the evaluation of model photochemical schemes.
Because HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> is short lived (Heard and Pilling, 2003), HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
measurements allow for evaluation of model photochemistry with the exclusion
of confounding phenomena, such as atmospheric transport. However, accurate
measurements have proven difficult due to the naturally low abundance of
HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>. HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> also possess weak spectral lines, which has posed
challenges for spectroscopic techniques. Nevertheless, some spectroscopic
measurements have been made, primarily in the laboratory.
Radford et al. (1974) employed laser magnetic resonance (LMR)
spectroscopy in the laboratory to measure HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> while Mihelcic et
al. (1985, 2003) used matrix isolation electron spin resonance (MIESR). The
latter requires HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> to be collected for a period of 30 min on a
D<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O matrix at 77 K before detection. Both techniques directly measure
HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> but their applicability to atmospheric observations is limited, due
to either instrumentation needs or low time resolution.</p>
      <p>More recent methods such as peroxy radical chemical amplification (PERCA)
(Cantrell and Stedman, 1982; Cantrell et al., 1984; Liu et al.,
2009; Horstjann et al., 2014), chemical ionization mass spectrometry (CIMS)
(Hanke et al., 2002; Edwards et al., 2003; Hornbrook et al., 2011; Kim et
al., 2013; Wolfe et al., 2014), and laser induced fluorescence (LIF)
(Stevens et al., 1994; Brune et al., 1995; Griffith et al., 2013; Walker et
al., 2015) provide lower detection limits at high temporal resolution.
However, these techniques do not measure HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> directly. Instead, the
aforementioned techniques require that HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> be titrated with NO, which
may introduce additional complexity, primarily from reactions of NO with
RO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>. The PERCA technique, for example, exploits the radical chain
reactions of HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> with NO and OH with CO to produce multiple NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
molecules from each HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> present in the sample. The production of
NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> molecules is proportional to the contact time between the added
reagents and the sample gas. Because multiple NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> molecules are
produced from each HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, the signal is effectively amplified. The
NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> has then traditionally been detected using luminol, though some
recent measurements employ cavity ring-down spectroscopy (Liu et al.,
2009; Horstjann et al., 2014). If organic peroxy radicals are present, the
addition of NO to the sample gas results in additional production of
HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>; therefore the technique allows for the measurement of
HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> RO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>. As of yet, speciation of HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> from other peroxy
radicals has not been successful, though previous attempts have been made
(Miyazaki et al., 2010).</p>
      <p>Chemical ionization techniques such as RO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> Chemical Conversion/CIMS (ROxMAS)
(Hanke et al., 2002) and Peroxy radical CIMS (PerCIMS) (Edwards et
al., 2003; Hornbrook et al., 2011; Kim et al., 2013; Wolfe et al., 2014) also
rely on addition of NO to the sample gas. The OH produced from HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
titration subsequently reacts with SO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> which is added to the inlet to
produce H<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>SO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>. The H<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>SO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> is then ionized by nitrate ions
(NO<inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> to produce a stable HSO<inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> product ion for
detection. Because NO is added, PerCIMS suffers from positive artifacts from
the contribution of the RO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> NO reaction to the measured HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
concentration. Previous attempts to limit the contribution of the
RO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> NO reaction have been made. For example, Hornbrook et al. (2011)
successfully speciated HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> RO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> measurements by
modulating the relative NO and O<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations in the reaction
region, suppressing the conversion of some peroxy radicals to
<inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 15 %. However, the effectiveness of the oxygen dilution
modulation scheme depends largely on the chemical structure of the
hydrocarbons in the sample. Unsaturated hydrocarbons, such as isoprene, have
additional pathways to the formation of HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> which are not suppressed by
the oxygen dilution modulation scheme.</p>
      <p>Unlike CIMS techniques and chemical amplification, the laser induced
fluorescence technique does not require multiple conversion steps. It only
requires the titration of HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> to OH, which is subsequently detected
using laser excitation at 308 nm. The relative simplicity of the technique
allows for more effective control of reaction time, which can be used to
minimize RO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> NO reactions. Nevertheless, LIF instruments have
previously been shown to be susceptible to similar artifacts, with
magnitudes dependent on the effective reaction time allowed after NO
addition before detection and on peroxy radical precursor composition of the
sample gas (Fuchs et al., 2011; Whalley et al., 2013).</p>
      <p>Given the uncertainties associated with indirect methods of HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
measurement and the time resolution required for atmospheric measurements, a
direct fast time resolution measurement of HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> would benefit efforts
aiming to measure and model HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> in order to understand atmospheric
photochemistry. The exclusion of measurement artifacts would aid in
evaluating the gap between measured and modeled HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations in
forested regions, where measured to modeled HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> ratios are highly
variable (Stone et al., 2012). In this work, we evaluated the
potential of various chemical ionization schemes and propose the Br<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula>
ionization of HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> to form a Br<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula>(HO<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> adduct as a direct
method for measuring HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> using chemical ionization mass spectrometry.
This technique provides selective, fast time resolution measurements of
HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>. Ambient measurements were conducted in Atlanta in June 2015 to
demonstrate instrument performance. Important measurement considerations and
future improvements are also discussed.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1" specific-use="star"><caption><p>Schematic diagram of the high-resolution time-of-flight chemical
ionization mass spectrometer (HR-ToF-CIMS). Sample air enters the ion–molecule reaction
region through a 0.5 mm orifice where it is ionized at 100 mbar. The contents
of the ion–molecule reaction region are sub-sampled through a 0.3 mm orifice
into the small segmented quadrupole (SSQ) chamber held at 2.5 mbar.
Collisional dissociation occurs in the SSQ. Ion products are then collimated
by the big segmented quadrupole (BSQ) where they also dissipate energy by
collisions with background gas at reduced pressure. The subsequent ion lenses
then focus and accelerate the ion beam towards the ToF analyzer.</p></caption>
        <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/3851/2016/amt-9-3851-2016-f01.png"/>

      </fig>

<?xmltex \hack{\vspace{-3mm}}?>
</sec>
<sec id="Ch1.S2">
  <title>Instrument description</title>
      <p>A high-resolution time-of-flight chemical ionization mass spectrometer (HR-ToF-CIMS,
Aerodyne Research, Inc.) and a house-built quadrupole CIMS
were used for laboratory characterizations of reagent ions for the
measurement of HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>. Ambient data were collected using the HR-ToF-CIMS
exclusively. The HR-ToF-CIMS consists of an atmospheric pressure interface
with five differentially pumped stages, utilizing two scroll pumps and a
multi-stage turbomolecular pump. The instrument design has been described in
detail by Bertram et al. (2011). Figure 1
shows a schematic diagram of the HR-ToF-CIMS. HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> is measured by
introducing 2 standard L min<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> of sample into the ion–molecule reaction region through a
0.5 mm orifice and mixed with Br<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula> reagent produced by passing 10 sccm
of a 0.2 % CF<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>Br <inline-formula><mml:math display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> mixture carried by <inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 2 standard L min<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>
N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> gas (99.999 %, Airgas) through a cylindrical 10 mCi <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>210</mml:mn></mml:msup></mml:math></inline-formula>Po
alpha radiation source. The ion–molecule reaction region (IMR) has a
residence time of 0.07 s and is operated at a pressure of 100 mbar.
The contents of the IMR were sub-sampled through a 0.3 mm critical orifice
leading to the instrument's ion optics. HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> present in the sample
cluster with Br<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula> to form Br<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula>(HO<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> adducts which are
transmitted by a series of ion optics and speciated by the time-of-flight
spectrometer. The isotopic abundance of bromine is such that the adduct is
detected at two nominal mass-to-charge ratios, <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 112 and <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 114 corresponding
to the <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>79</mml:mn></mml:msup></mml:math></inline-formula>Br and <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>81</mml:mn></mml:msup></mml:math></inline-formula>Br isotopes, respectively. The adducts have
fractional mass-to-charge ratios of 111.9165 and 113.9144 Th. In order to
demonstrate the generalizability of the technique to instruments with unit
mass resolution, only the unit mass resolution data are used for ambient
measurements, though the high-resolution capabilities were exploited to
diagnose and address possible artifacts during the method development. The
high-resolution mass spectra are also used to unambiguously identify the
BrHO<inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> adducts. In contrast to the HR-ToF-CIMS, the quadrupole
CIMS was operated at an ion–molecule reaction region pressure of 15 torr.
The sample and N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> flow rates were both 2 standard L min<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>.</p>
</sec>
<sec id="Ch1.S3">
  <?xmltex \opttitle{HO${}_{{2}}$ generation and calibration procedure}?><title>HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> generation and calibration procedure</title>
      <p>HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> were generated for the evaluation of chemical ionization schemes
and instrument calibrations by water photolysis at 184.9 nm using a mercury
UV lamp as previously described by a number of studies e.g., (Tanner et
al., 1997; Holland et al., 2003; Smith et al., 2006; Dusanter et al. 2008). Air was
humidified by passing the gas stream through glass bubblers and diluted in
dry air from a pure air generator (AADCO 747-14) to vary the relative
humidity of the gas. The gas stream was then introduced into a black
anodized aluminum square flow tube (15.6 mm <inline-formula><mml:math display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 15.6 mm <inline-formula><mml:math display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 520 mm) and exposed to UV radiation through a small slit. HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
concentrations were calculated using Eq. (<xref ref-type="disp-formula" rid="Ch1.E1"/>),
          <disp-formula id="Ch1.E1" content-type="numbered"><mml:math display="block"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mrow class="chem"><mml:mo>[</mml:mo><mml:mi mathvariant="normal">HO</mml:mi></mml:mrow><mml:mrow class="chem"><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msub><mml:mrow class="chem"><mml:mo>]</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mo>=</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/></mml:mrow><mml:mi mathvariant="italic">ϕ</mml:mi><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>I</mml:mi><mml:msub><mml:mrow class="chem"><mml:mo>[</mml:mo><mml:mi mathvariant="normal">H</mml:mi></mml:mrow><mml:mrow class="chem"><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msub><mml:mrow class="chem"><mml:mi mathvariant="normal">O</mml:mi><mml:mo>]</mml:mo></mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>t</mml:mi><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
        <?xmltex \hack{\newpage}?><?xmltex \hack{\noindent}?>where <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">ϕ</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:mi>I</mml:mi></mml:math></inline-formula>, and <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>t</mml:mi></mml:mrow></mml:math></inline-formula> represent the quantum yield, water
absorption cross-section, UV lamp photon flux at 184.9 nm, and irradiation
time, respectively. The quantum yield was assumed to be unity and a value of
7.22 <inline-formula><mml:math display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn>20</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> cm<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> was used for the water absorption cross section
(Creasey et al., 2000). The lamp photon flux was measured
using a Hamamatsu Phototube (Hamamatsu Photonics), and found to be 2.6 <inline-formula><mml:math display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>13</mml:mn></mml:msup></mml:math></inline-formula> photons cm<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> s<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>. A bandpass filter (HORIBA Scientific)
was used to selectively transmit at 185 nm. The dew point of the gas was
measured using a LICOR LI-840A CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> H<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O gas analyzer. The
irradiation time was calculated based on the flow velocity which was
measured using a Dwyer pitot tube and a magnehelic pressure sensor. Flow
velocities varied between 400 and 800 cm s<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> (<italic>Re</italic> &gt; 4000) to promote
plug flow conditions. The slit allowing light into the tube was located such
that the distance before irradiation after entry into the tube was 10 times
the hydraulic diameter, allowing the flow profile to fully develop before exposure to UV light. Plug
flow conditions were confirmed by measuring the flow velocity both at the
center line and near the wall of the tube, showing no measurable
differences. The water vapor mixing ratios varied between 0.66 and 8.20 ppt. The time after irradiation before introduction into the
instrument was minimized (<inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">τ</mml:mi></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 60 ms) to avoid additional
HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> generation from OH oxidation of trace CO present in the N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
gas. It was calculated that less than 8 % of the OH formed would react
with CO to produce additional HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> assuming a CO concentration of 500 ppb. Addition of 40 ppm of C<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>F<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:math></inline-formula> as an OH scavenger had no effect
on the HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> signal intensity, confirming the lack of contribution from
OH oxidation to HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> production. The HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentration was kept low (2–45 ppt)
to calibrate for the HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> levels observed during ambient sampling and to
avoid non-linearity in the calibration curve due to depletion of HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
through HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> radical–radical recombination. At the HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> mixing
ratios employed, less than 1 % of HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> are estimated to be lost to
recombination. The overall calibration uncertainty is 18 % (1<inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="italic">σ</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>.
The contribution of the different parameters to the overall uncertainty is
given in Table S1 in the Supplement. A conservative estimate of 20 % is used in this work.
<?xmltex \hack{\vspace{-3mm}}?></p>
</sec>
<sec id="Ch1.S4">
  <title>Laboratory characterizations and reagent ion selection</title>
      <p>Prior to the selection of Br<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula> for our ionization scheme, a number of
negative reagent ions were evaluated for their ability to detect HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>.
HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> were generated using the procedure in Sect. 3. HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> mixing
ratios were typically in excess of 300 ppt for initial reagent ion
evaluation, and varied by varying the gas humidity and velocity. NO was
added in excess (2–4 ppm) to obtain the instrument background. NO was also
added in small concentrations and in increasing increments to roughly test
the kinetics suggested by the HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> signal response to additions of
varying concentrations of NO, as additional confirmation that the analyte
being observed corresponded to HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>. Tests were conducted primarily at
room temperature (293 K). The humidity of the gas stream was determined by
the amount of water vapor added to produce HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>. No additional sources
of water vapor were present, nor was water directly added to the IMR. The
reagent ions evaluated included O<inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>, SF<inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">6</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>, Cl<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula>, and
I<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula>. Because of their low electron affinities, O<inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> and
SF<inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">6</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> were utilized in an attempt to produce the HO<inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> ion
directly via charge exchange. However, HO<inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> was not observed in
laboratory characterization experiments. It is likely that the
HO<inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> ion formed but was not detected due to its low electron
affinity (Ramond et al., 2002), which results in high
reactivity. The SF<inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">6</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> ionization did yield a cluster at
mass-to-charge 52, which was assigned as HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>F<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula> in the high-resolution mass spectrum. However, the signal was not quantitatively
reproducible and did not remain constant for a given HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentration.
Additionally, the form of the cluster is more likely to be O<inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>(HF)
than F<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula>(HO<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> (Seeley et al., 1996), which may
compromise the selectivity of the measurement, as O<inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> ions are not
uniquely formed from the ionization of HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>.</p>
      <p>Chloride and iodide reagent ions were generated from HCl and CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>I
mixtures, respectively. Full mass spectra obtained using the quadrupole CIMS
identified Cl<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula>(HCl), Cl<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula>(HNO<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, and Cl<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula>(CF<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>COOH) as
prominent ions. However, the Cl<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula>(HO<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> cluster was not observed.
The characterizations involving chloride reagent ions in the laboratory were
conducted using the quadrupole CIMS. Unlike the other ions, which were
evaluated with the HR-ToF-CIMS as well as the quadrupole CIMS, Cl<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula> was
not revisited with the HR-ToF-CIMS instrument.</p>
      <p>The I<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula> reagent ion, which has been used extensively to measure both
organic and inorganic species (Huey et al., 1995; Slusher et al., 2004; Lee
et al., 2014; Woodward-Massey et al., 2014; Brophy and Farmer, 2015; Faxon et
al., 2015; Nah et al., 2016; Lee et al., 2016), was found to cluster with
HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, appearing at mass-to-charge 160, consistent with observations by
Veres et al. (2015). However, we
observed that addition of NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> (Scott-Marrin, 100 ppm <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>v</mml:mi><mml:mo>/</mml:mo><mml:mi>v</mml:mi></mml:mrow></mml:math></inline-formula> N<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> to a
clean N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> gas matrix resulted in an increase of 1 cps per ppb NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
per 10<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msup></mml:math></inline-formula> cps I<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula> in the <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 160 signal. A 20 ppb addition results in a
20 cps increase in the <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 160 signal, equivalent to <inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 4 ppt of
HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>. The addition of NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> showed an increase in a peak (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 159.9896)
not associated with HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> that we could not identify. The addition of
NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> did not affect the high-resolution I<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula>(HO<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> signal but is
expected to be a significant artifact for instruments of low resolving
power.</p>
      <p>Unlike the other reagent ions, the Br<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula> ionization scheme was found to
be sensitive to HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, the measurements were reproducible, and there were
no observed positive artifacts from NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> or O<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>, making this an
ideal scheme for measurements of HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>. To evaluate potential positive
artifacts as observed using iodide, NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> was added to the N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> gas
sample and measured using the bromide reagent, but no increase in the
Br<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula>(HO<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> (nominal <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 112 and <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 114) signals was observed. Parts per
million mixing ratios of ozone were also introduced into the inlet in a
clean N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> matrix but did not cause any changes in the Br<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula> (HO<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> cluster signal. While Br<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula> has the disadvantage of having a
<inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 50 % natural isotopic abundance with nominal <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 79 and 81,
HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> calibrations performed as described in Sect. 4 showed similar
absolute sensitivities for the I<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula>(HO<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> and
<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>79</mml:mn></mml:msup></mml:math></inline-formula>Br<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula>(HO<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> clusters using I<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula> and Br<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula> reagents,
respectively. A synthesized mixture containing primarily <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>79</mml:mn></mml:msup></mml:math></inline-formula>Br could
nearly double the sensitivity at the <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 112 cluster if necessary, giving
Br<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula> a potential advantage over I<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula> with respect to sensitivity. The
<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>79</mml:mn></mml:msup></mml:math></inline-formula>Br<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula>(HO<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> cluster was used preferentially over the
<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>81</mml:mn></mml:msup></mml:math></inline-formula>Br<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula>(HO<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> cluster for ambient data because <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 114 has a
contribution from the isotope of a large <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 113 CF<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>COO<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula> signal which
arises from impurities in PFA Teflon<sup>™</sup>. Iodide ionization was attempted
once more during ambient sampling, which will be discussed in Sect. 5.3.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2"><caption><p>Laboratory HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> calibration curves for the
<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>79</mml:mn></mml:msup></mml:math></inline-formula>Br<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula>(HO<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> cluster as observed at nominal <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 112. The slopes
represent the sensitivity in cps ppt<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>. HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> mixing ratios are calculated
using Eq. (1). Two calibrations conducted on separate occasions are shown to illustrate reproducibility. The
error associated with the individual sensitivities is 20 % which arises
from the combined uncertainty of the calibration parameters (Eq. 1).</p></caption>
        <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/3851/2016/amt-9-3851-2016-f02.pdf"/>

      </fig>

<sec id="Ch1.S4.SSx1" specific-use="unnumbered">
  <?xmltex \opttitle{Br${}^{{-}}$ ionization: sensitivity, selectivity, humidity, and temperature
dependence}?><title>Br<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula> ionization: sensitivity, selectivity, humidity, and temperature
dependence</title>
      <p>The instrument sensitivity using Br<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula> reagent was calibrated following
the procedure in Sect. 3. Figure 2 shows HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> calibration curves for
<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>79</mml:mn></mml:msup></mml:math></inline-formula>Br<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula>(HO<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> at <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 112. The figure shows two separate calibrations performed on two different occasions to
illustrate reproducibility. The curves are linear with slopes of 4.95 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 1.00 and 5.26 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 1.05 which represent the instrument sensitivity in
cps ppt<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> for a <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>79</mml:mn></mml:msup></mml:math></inline-formula>Br<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula> ion count of 10<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msup></mml:math></inline-formula> cps. Intercepts of
27 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 5 and 30 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 3 are observed for the calibration curves which
are not explained by errors in any of the parameters used to calculate the
expected HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations in Eq. (1). Instead, there appears to be a
constant HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> photolytic source independent of water photolysis. The
unidentified source requires the presence of water vapor but does not scale
with the absolute water vapor mixing ratio. Further, addition of 40 ppm
C<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>F<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:math></inline-formula> as OH scavenger did not have an effect on the observed
intercept, suggesting that the HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> production is unrelated to OH
oxidation. The magnitude of the HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> formation from this unknown source
scales linearly with the UV lamp flux. The intercept does not affect the
sensitivity and is not used to calculate the HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> mixing ratio. The
uncertainty in the sensitivity is derived from the combined uncertainties of
the parameters used in Eq. (1), as well as random error in the HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
signal, resulting in a 1<inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula> uncertainty of 20 %. Contributions to
the overall uncertainty for each parameter are listed in Table S1. The time
series of one HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> calibration at both <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 112 and 114 are shown in
Fig. S2 in the Supplement
to illustrate the rapid instrument response to varying levels of analyte.</p>
      <p>The Br<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula>(HO<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> measurement selectivity was explored further in the
laboratory. In addition to high concentration additions of NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and
O<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>, other common atmospheric constituents were sampled with the
instrument to assess the possibility of other potential artifacts. Large
concentrations (&gt; 10 ppm) of SO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> were added, which did not
elicit a response. Hydrogen peroxide and formaldehyde were sampled from the
Georgia Tech Environmental Chamber facility
(Boyd et al., 2015) at concentrations in excess
of several ppm, eliciting responses of 0.25 and 0.002 cps ppb<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> at
<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 112, respectively. It is not clear whether the observed signal response is
due to ion–molecule reaction with Br<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula> or unidentified wall reactions
within the experimental chamber. Regardless, these responses are
insignificant under most atmospheric and laboratory experimental conditions.
Furthermore, if the resulting signal increase is due to reactions inside the
IMR, the contribution of these species can be removed from the measurement
by obtaining appropriate instrument backgrounds, such as by using additions
of NO. Such additions would remove HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> in the sample, but not remove
H<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> or HCHO. The small contributions to the signal at <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 112 would
be present in the background and therefore removed from the measurement.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3"><caption><p>Instrument sensitivity as measured at <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 112
<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mo mathsize="1.1em">(</mml:mo><mml:mn>79</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>Br<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula>(HO<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo><mml:mo mathsize="1.1em">)</mml:mo></mml:mrow></mml:math></inline-formula> as a function of sample relative humidity. The
instrument sensitivity demonstrates no water vapor dependence beyond a
sample relative humidity of 10 %. The “Calibration 1” and “Calibration
2” labels refer to the curves in Fig. 2.</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/3851/2016/amt-9-3851-2016-f03.pdf"/>

        </fig>

      <p>Another important consideration for this technique is the effect of
temperature and humidity on cluster stability, which was explored during
laboratory characterizations. The effect of varying water vapor mixing
ratios in the sample gas on sensitivity is shown in Fig. 3. At relative
humidities in the sample below 10 %, the sensitivity appears to have a
strong, negative water dependence. However, when the humidity in the sample
gas is higher than 10 %, the sensitivity is invariant with increasing
relative humidity, which simplifies ambient sampling, as no
humidity-dependent correction is required. The temperature dependence was
also explored, where an IMR temperature increase from 20 to 40 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C
resulted in a 20 % decrease in instrument sensitivity. The relatively
strong negative temperature dependence suggests that Br<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula>(HO<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> is a
weak cluster. This highlights the importance of temperature control and
performing calibrations at the sampling temperature.
<?xmltex \hack{\vspace{-3mm}}?></p>
</sec>
</sec>
<sec id="Ch1.S5">
  <title>Ambient measurements</title>
      <p>To demonstrate the applicability of the Br<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula> ionization scheme to
ambient HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> measurements, a field study was conducted in June 2015
(9–25 June 2015) in Atlanta at an urban site located on the roof (30–40 m above ground) of the Ford Environmental Science &amp; Technology building
on the Georgia Tech campus, which has been used for previous ambient studies
(Hennigan et al., 2008; Xu et al., 2015a, b). The site is
about 840 m west of Interstate 75/85 and can therefore be affected by
traffic emissions. The instrument was located outside in an enclosure,
allowing for a short 1 cm inner diameter Teflon<sup>™</sup> inlet of
approximately 13 cm in length. The residence time of ambient sample in the
tube was short (0.3 s) which helps to minimize HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> surface losses
on the sample tubing. Data was collected at a 1 Hz frequency and averaged to
1 min. A solenoid valve was used to perform periodic additions of 10 sccm
of an NO <inline-formula><mml:math display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> mixture (Scott-Marrin, 810 ppm) into the sample stream
every 10 min on a 10 % duty cycle to obtain the measurement
background. The <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 112 signal was normalized to a <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>79</mml:mn></mml:msup></mml:math></inline-formula>Br<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula> count of
10<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msup></mml:math></inline-formula> cps to account for temporal changes in reagent ion abundance.</p>
      <p>Various co-located instruments were deployed for simultaneous measurements
of O<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>, NO, NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, and HNO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>. NO concentrations were
measured using a Teledyne 200EU chemiluminescence monitor while NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> was
measured by a Cavity Attenuated Phase Shift NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> monitor (Aerodyne
Research, Inc.). Ozone was measured using a Teledyne Model T400 UV
absorption analyzer. Pernitric acid (HNO<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, formed from the reaction of
HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> with NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> was also monitored using a house-built quadruple CIMS with an iodide-adduct
ionization scheme and observed at <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 206. A similar configuration of the
instrument has been described previously by Slusher et al. (2004). Previous measurements of HNO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> using I<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula> have been conducted
by Veres et al. (2015). Meteorological
data, including temperature and humidity, were recorded using a Vantage Pro2
weather station. An additional UV sensor was employed with the Vantage Pro2
weather station to obtain an UV index measurement between 280 and 360 nm.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4"><caption><p>Hourly median diurnal profiles of HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, NO, O<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> and UV
index in Atlanta. The sampling period was during 9 June 2015 21:14:00 to 11 June 2015
13:28:00, and 15 June 2015 01:52:00 to 25 June 2015 01:32:00 LT.</p></caption>
        <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/3851/2016/amt-9-3851-2016-f04.pdf"/>

      </fig>

<?xmltex \hack{\newpage}?>
<sec id="Ch1.S5.SS1">
  <?xmltex \opttitle{Bromide-CIMS measurements of HO${}_{{2}}$}?><title>Bromide-CIMS measurements of HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula></title>
      <p>Figure 4 shows the diurnal profiles of HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, as well as the diurnal profiles of
the UV radiation index, NO, and O<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> concentrations. The difference in
the time between peak actinic flux and peak HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentration is at
least partially due to the suppression of HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> by the presence of NO
from morning-time traffic emissions. The HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> rises once the NO
concentration is sufficiently low and peaks between 2 and 3 p.m. with a
mixing ratio of <inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 5 ppt, comparable to previous studies in
other urban regions (Emmerson et al., 2005; Kanaya et al., 2007; Dusanter
et al., 2009). The 3<inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula> limit of detection was calculated to be 0.7 ppt for a 1 min integration time based on laboratory calibrations and
baselines observed during ambient sampling, which is sufficiently low for
atmospherically important HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations. The slow decay of
HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> in early evening may partially be explained by non-photolytic
HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> production, e.g., from oxidation of biogenic volatile organic
compounds (BVOCs), which are abundant in the Southeast United States
(Geron et al., 2000; Guenther et al., 2006), as well as a decrease in
boundary layer height. However, additional measurements would be required to
constrain sources and sinks.</p>
      <p>The mass spectrum for a 24 h period of ambient observations is shown in
Fig. 5 and compared to a laboratory spectrum generated during HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
calibration. Few additional peaks are present in ambient spectrum,
suggesting that Br<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula> ionization is selective at the mass-to-charge
values shown in the figure. Further, the majority of the additional peaks
have signal intensities much lower than the intensity of the HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> signal
at <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 112, which makes it unlikely that the species at the additional peaks
and their respective isotopes will affect the signal at <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 112.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5"><caption><p>Comparison of laboratory generated and ambient mass spectra.
Laboratory data was collected during HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> calibration using the procedure
described in Sect. 3. Ambient data from a 24 h period during ambient
sampling is shown here. The ambient mass spectrum is reversed for clarity.
Few additional peaks are observed in the ambient spectrum, the majority of
which are of low signal intensity. Prominent known peaks are at <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 79 and
81 (Br<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 85 (CF<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>O<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 97
<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mo mathsize="1.1em">(</mml:mo><mml:mn>79</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>Br<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula>(H<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O)<inline-formula><mml:math display="inline"><mml:mo mathsize="1.1em">)</mml:mo></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 99 <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mo mathsize="1.1em">(</mml:mo><mml:mn>81</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>Br<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula>(H<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O) and
<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>79</mml:mn></mml:msup></mml:math></inline-formula>Br<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula>(HF)<inline-formula><mml:math display="inline"><mml:mo mathsize="1.1em">)</mml:mo></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 101 <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mo mathsize="1.1em">(</mml:mo><mml:mn>81</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>Br<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula>(HF)<inline-formula><mml:math display="inline"><mml:mo mathsize="1.1em">)</mml:mo></mml:math></inline-formula>, and <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 113
(CF<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>COO<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>.</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/3851/2016/amt-9-3851-2016-f05.pdf"/>

        </fig>

      <p>HNO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> and NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> measurements were used to infer HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
concentration for comparison with the measured HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations. The
HNO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> and HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> are assumed to be in thermal equilibrium for the
calculation. Details regarding the calculation are discussed in the
Supplement. Their respective diurnal profiles are
shown in Fig. S3. The profiles agree well temporally but not quantitatively,
differing by a factor of 5 during the afternoon. A more complete discussion
regarding the comparison is presented in the Supplement.</p>
</sec>
<sec id="Ch1.S5.SS2">
  <title>Instrument background determinations</title>
      <p>Measurement backgrounds were conducted by the addition of NO to the sample
gas, as mentioned previously. To evaluate the accuracy of the instrument
background, a metal wool scrubber was utilized for comparison to the NO
addition. The scrubber was first tested to ensure complete scrubbing of
sample HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> by generation of additional HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> in ambient air with a
mercury lamp. Though HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> was generated, none was observed when the
scrubber was placed before the instrument, demonstrating that the scrubber
was effectively removing all HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> in the sample gas.</p>
      <p>It was observed that the two methods of obtaining the instrument background
did not agree, with the NO addition providing a lower background signal than
the metal wool scrubber. Furthermore, additions of NO to the sample air
after physical scrubbing further decreased the HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> signal. This
suggests that there is internal HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> generation within the instrument.
Laboratory characterizations were conducted to explore the discrepancy. In
the laboratory, adding NO to a clean N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> sample matrix also decreased
the observed HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> background signal. The differences in HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
backgrounds observed between the different backgrounding methods and NO
additions to N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> gas were similar, representing <inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 4 ppt of
HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> generated inside the instrument. The similarity suggests that
HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> generation is independent of sample composition. The HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> is
likely produced from ion-molecule reactions of trace gases in the N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
used for ion generation. The HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> mixing ratios were corrected by
subtraction of an additional, constant 4 ppt contribution from internal
HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> generation.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6"><caption><p>Normalized high-resolution mass spectra of nominal <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 112 for the
Br<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula> ionization of HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> (top panel) and <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 160 for the I<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula> ionization of
HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> (bottom panel). The <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>79</mml:mn></mml:msup></mml:math></inline-formula>Br<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>81</mml:mn></mml:msup></mml:math></inline-formula>Br<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula> peak corresponds to Br<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
added directly to the sample flow from a permeation tube as an additional
calibrant.</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/3851/2016/amt-9-3851-2016-f06.pdf"/>

        </fig>

      <p>Based on the observations made in this work, future instrument backgrounds
can be conducted in alternative ways to eliminate the need for
post-correction. For example, a physical scrubber may be used as has been
done here to avoid removal of internally generated HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> from the
background signal. Alternatively, the NO addition concentration and contact
time can be optimized such that the HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> NO reaction is efficient in
the sample line before the instrument, where the pressure is approximately
atmospheric, but inefficient inside the IMR, where the pressure is at least
a factor of 10 lower. The addition of NO under optimal conditions would
then only titrate HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> efficiently in the sample line, but would not
allow significant NO reaction with internally generated HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>.</p>
</sec>
<sec id="Ch1.S5.SS3">
  <?xmltex \opttitle{Iodide-CIMS measurements of HO${}_{{2}}$}?><title>Iodide-CIMS measurements of HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula></title>
      <p>Despite artifacts observed in the measurements of laboratory-generated
HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, iodide ionization measurements were conducted during a short
ambient sampling period (25 July 2015 06:00 p.m. to 27 July 2015 10:00 a.m.) to
assess its viability in a real air matrix for the measurement of HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>.
We observed that the measured I<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula>(HO<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> signals were not consistent
with the expected behavior of HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>. The time series did not show a clear
diurnal pattern, nor was the signal effectively suppressed by NO additions.
Instead, NO additions caused <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 160 to increase. The high-resolution
capability of the HR-ToF-CIMS allowed for the peak assignment of
I<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula>(HO<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> with high accuracy but the time series of the high-resolution peak displayed a similar behavior to that of the low resolution
data. The resolving power of the instrument during the sampling period was
<inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 3000 and the high-resolution time series of the major peaks
at nominal <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 160 appear to be mostly independent of each other, which
suggests that resolution is not a limiting factor. Additionally, a peak
(<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 159.990 Th) which may pertain to the NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> related artifact observed
during earlier laboratory characterizations was present (Fig. 6). Because
the sampling period was short, the possibility of using iodide for HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
measurements may warrant further exploration. However, our laboratory and
ambient measurements suggest that for iodide to be viable, high-resolution
capability will be necessary for accurate measurements due to artifacts
caused by the presence of NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>. This is not the case for Br<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula>.
Figure 6 shows the mass spectra of Br<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula> and I<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula> at the
mass-to-charge ratios where the HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> clusters are observed. The Br<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula>
spectrum shows that the Br<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula>(HO<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> cluster is the dominant species
at <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 112. The minor peak observed is always present and does not vary
significantly over the course of the day. Furthermore, the peak does not
respond to NO additions, making NO backgrounds effective at eliminating any
contribution to the signal from this peak. Thus, the measurement of HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
with Br<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula> does not require high-resolution capability.</p><?xmltex \hack{\vspace{-3mm}}?>
</sec>
</sec>
<sec id="Ch1.S6" sec-type="conclusions">
  <title>Conclusions and future work</title>
      <p>HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> is an important contributor to photochemistry in the atmosphere. In
this work, we investigated the feasibility of a direct chemical ionization
measurement of HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>. We evaluated a number of negative reagent ions
(O<inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>, SF<inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">6</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>, Cl<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula>, I<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula>, and Br<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> using a
HR-ToF-CIMS and found that detection of HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> using charge exchange
ionization is not feasible in the real atmosphere. However, ionization of
HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> via clustering was found to be a promising mechanism for the direct
measurement of atmospheric HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>. Among the reagent ions evaluated,
Br<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula> was found to be the best candidate for the measurement of HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>,
providing improved selectivity over I<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula>. The HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> sensitivities as
measured at <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 160 and <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 112 using iodide and bromide, respectively, were found
to be similar, giving Br<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula> a potential advantage in sensitivity, as an
isotopically pure CF<inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mn>79</mml:mn></mml:msubsup></mml:mrow></mml:math></inline-formula>Br mixture should nearly double the
sensitivity at <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 112. Using Br<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula> also allows for the measurement of
HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> at a lower <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> which may decrease the likelihood of measurement
interferences and reduce ambiguity in peak identification, as a smaller
number of possible chemical formulas for ion products are possible.
Furthermore, Br has a high electron affinity, which makes the production of
small charged ions from ionization and collisional dissociation unlikely.</p>
      <p>Ambient measurements were conducted in Atlanta in June 2015 to demonstrate
the performance and capability of the instrument. The sensitivity using
Br<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula> (5.1 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 1.00 cps ppt<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> per 10<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mn mathvariant="normal">6</mml:mn><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mn>79</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>Br ion counts) was
sufficient for ground-based measurements as the observed baselines were
relatively low. Furthermore, the absolute sensitivity for HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> may also
be significantly improved by using a radioactive source with higher
activity, provided that measures are taken to suppress the increased
background due to internal HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> generation. The measured HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
diurnal profile behaves in a manner consistent with the NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and
HNO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> abundance, though there exist no previous measurements for
HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> in Atlanta available for a more quantitative comparison. Future
work will focus on optimizing the instrument sensitivity to HO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>,
conducting instrument intercomparisons, and further exploring Br<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula>
ionization for the measurement of other atmospherically important species.</p>
</sec>
<sec id="Ch1.S7">
  <title>Data availability</title>
      <p>The data presented in this paper are available upon request from
the corresponding author.</p>
</sec>

      
      </body>
    <back><app-group>
        <supplementary-material position="anchor"><p><bold>The Supplement related to this article is available online at <inline-supplementary-material xlink:href="http://dx.doi.org/10.5194/amt-9-3851-2016-supplement" xlink:title="pdf">doi:10.5194/amt-9-3851-2016-supplement</inline-supplementary-material>.</bold></p></supplementary-material>
        </app-group><ack><title>Acknowledgements</title><p>This work was supported by National Science Foundation
grant 1455588. The HR-ToF-CIMS was purchased with NSF Major Research
Instrumentation (MRI) grant 1428738. J. Sanchez acknowledges support by the
NASA Earth and Space Science Fellowship (NESSF) and the Alfred P. Sloan
Minority Ph.D. (MPHD) Scholarship. D. Chen, L. Huey, and D. Tanner were
supported by NSF grant #1262033. The authors would like to thank Wing Y. Tuet for helpful comments.
<?xmltex \hack{\newline}?><?xmltex \hack{\newline}?>
Edited by: A. Hofzumahaus<?xmltex \hack{\newline}?>
Reviewed by: two anonymous referees</p></ack><ref-list>
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    </app></app-group></back>
    <!--<article-title-html>A new technique for the direct detection of HO<sub>2</sub> radicals using bromide
chemical ionization mass spectrometry (Br-CIMS): initial characterization</article-title-html>
<abstract-html><p class="p">Hydroperoxy radicals (HO<sub>2</sub>) play an important part in tropospheric
photochemistry, yet photochemical models do not capture ambient HO<sub>2</sub>
mixing ratios consistently. This is likely due to a combination of
uncharacterized chemical pathways and measurement limitations. The indirect
nature of current HO<sub>2</sub> measurements introduces challenges in accurately
measuring HO<sub>2</sub>; therefore a direct technique would help constrain
HO<sub><i>x</i></sub> chemistry in the atmosphere. In this work we evaluate the
feasibility of using chemical ionization mass spectrometry (CIMS) and
propose a direct HO<sub>2</sub> detection scheme using bromide as a reagent ion.
Ambient observations were made with a high-resolution time-of-flight
chemical ionization mass spectrometer (HR-ToF-CIMS) in Atlanta over the
month of June 2015 to demonstrate the capability of this direct measurement
technique. Observations displayed expected diurnal profiles, reaching
daytime median values of  ∼  5 ppt between 2 and 3 p.m.
local time. The HO<sub>2</sub> diurnal profile was found to be influenced by
morning-time vehicular NO<sub><i>x</i></sub> emissions and shows a slow decrease into the
evening, likely from non-photolytic production, among other factors.
Measurement sensitivities of approximately 5.1 ± 1.0 cps ppt<sup>−1</sup> for a
bromide ion (<sup>79</sup>Br<sup>−</sup>) count rate of 10<sup>6</sup> cps were observed. The
relatively low instrument background allowed for a 3<i>σ</i> lower detection
limit of 0.7 ppt for a 1 min integration time. Mass spectra of ambient
measurements showed the <sup>79</sup>BrHO<sub>2</sub><sup>−</sup> peak was the major component
of the signal at nominal mass-to-charge 112, suggesting high selectivity for
HO<sub>2</sub> at this mass-to-charge. More importantly, this demonstrates that
these measurements can be achieved using instruments with only unit mass
resolution capability.</p></abstract-html>
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