Observations of cyanogen bromide (BrCN) in the global troposphere and their relation to polar surface O 3 destruction

. Bromine activation (the production of Br in an elevated oxidation state) promotes ozone destruction and mercury removal in the global


Introduction
Photochemically active halogen species in the lower troposphere affect the oxidizing capacity of the atmosphere via radical reactions that may either produce or destroy ozone (Saiz-Lopez and von Glasow, 2012;Simpson et al., 2015).In addition, active halogens play an important role in O 3 destruction when transported to the upper troposphere and lower stratosphere (UT/LS).Active halogen species are defined as halogen atoms, dihalogen compounds, or species that have an effective oxidation state above −1 (e.g., hypobromous acid, HOBr).A complete understanding of this chemistry requires accounting for reactions that produce or destroy active halogens in a variety of environments, ranging from the polar ice caps and the ocean surface layer to polluted continental regions.
Bromine chemistry in polar surface regions has been of particular interest since it was discovered that active bromine compounds were responsible for ozone destruction in those regions (Barrie et al., 1988).The chemistry behind the initiation and propagation of active bromine chemistry has since been the subject of numerous experimental and numerical modeling studies and several review articles (Abbatt et al., 2012;Simpson et al., 2015;Simpson et al., 2007), and ozone destruction is a widespread and persistent phenomenon in the Arctic boundary layer (Jacobi et al., 2010;Halfacre et al., 2014;Ridley et al., 2003).The review articles describe how ozone destruction follows from the production of Br 2 or BrCl on ice, snow, or particle surfaces, volatilization into the gas phase, and subsequent photolysis to two halogen atoms that react rapidly with O 3 to create halogen oxide (XO, where X = Cl, Br, or I).Halogen oxides have a number of pathways to form hypohalous acids (HOX) that can amplify the halogen chemistry through surface reactions with halide ions: for example, Several studies have shown that Br 2 tends not to form on sea ice surfaces (Pratt et al., 2013) because those surfaces are buffered at relatively high pH (Wren and Donaldson, 2012).The phenomenon represented by Reaction (R1) has been termed the "bromine explosion" when it accompanies the destruction of ozone (Wennberg, 1999;Platt and Janssen, 1995), and the participation of Br atoms in the photochemical cycle has been confirmed by direct observation of Br atoms (Wang et al., 2019).One of the keys to achieving a quantita-tive understanding of this Br chemistry is assessing the other heterogeneous reactions that HOBr can participate in.For example, there is evidence that HOBr reacting with dissolved organic matter (DOM), either on surface snow/ice or on particles, could be responsible for bromoform (CHBr 3 ) enhancements observed in polar environments (Carpenter et al., 2005;Gilman et al., 2010) and CHBr 3 and other organic bromine compounds observed in sea ice in the Antarctic winter (Abrahamsson et al., 2018).Reaction of HOBr with reduced nitrogen species to form cyanogen bromide (BrCN) could divert active bromine from the O 3 bromine explosion cycle.
The existence of cyanogen halides has been known for some time (e.g., ClCN was discovered in 1851; Wurtz, 1851), but to our knowledge they have not been reported in the ambient atmosphere.Note that cyanogen fluoride (FCN) is known, but FCN will not be formed in the environment due to the lack of chemical pathways that can form active F (e.g., HOF, F 2 ).In the environment, XCN compounds are formed from the reaction of active halogens, X 2 , or HOX (where X = Cl, Br, I) with reduced nitrogen species.For example, X 2 (HOX) + HCN → XCN + HX(H 2 O). (R2) This chemistry is well known in water and wastewater treatment processes where Cl 2 , NaOCl, or chloramines are added and reduced nitrogen species are present (Shah and Mitch, 2012;Yang and Shang, 2004).ClCN, and to some extent BrCN, has been measured in chlorination systems, including swimming pools, spas (Daiber et al., 2016), and water treatment systems (Heller-Grossman et al., 1999) because the reaction of active Cl compounds with bromide ions produces active Br.For example, As in the case of Cl chemistry, a range of N-containing substrates may be involved in BrCN formation.The solubility of XCN compounds has recently been found to range from only slightly soluble for ClCN to moderately soluble for ICN (Roberts and Liu, 2019).Thus, cyanogen halides will easily volatilize from solution and should be considered possible important participants in active halogen chemistry in the troposphere.
In addition to the above purely abiotic mechanisms, ClCN, BrCN, and ICN are known to be produced in biological systems through photosynthetic reactions involving H 2 O 2 , halides, and peroxidase enzymes present in neutrophils or other simple organisms (Vanelslander et al., 2012;Zgliczynski and Stelmaszynska, 1979;Schlorke et al., 2016).In those systems superoxide and hydrogen peroxide (O − 2 and H 2 O 2 ) are used by enzymes to produce HOX compounds and then XCN compounds by further reaction with N-containing substrates.In fact, there is evidence that several species of marine diatom have evolved to produce BrCN, and to some extent ICN, through photosynthetic production of H 2 O 2 and its conversion to HOX and then XCN compounds, by bromoand iodo-peroxidases (Vanelslander et al., 2012).One hypothesis is that microalgae have evolved this capability because BrCN suppresses other competing marine microbiota in marine biofilm communities (Vanelslander et al., 2012).Thus, cyanogen halides and BrCN in particular could have both biotic and abiotic sources, linked through common chemical mechanisms: the reactions of HOBr with reduced N compounds either in marine organisms and biofilms or on ice/snow and particles in the polar boundary layer.
The production of methyl halides in snowpacks and in soil environments next to glaciers appears to be due to a combination of snow photochemical and biological processes (see, for example, Macdonald et al., 2020;Swanson et al., 2007).The literature implies that co-production of the bromomethanes (dibromomethane (CH 2 Br 2 ) and CHBr 3 ) can be used to distinguish between biotic (soils, marine) and abiotic BrCN sources.Production in soils next to glaciers showed ratios of CHBr 3 /CH 2 Br 2 on the order of 1-3 (Macdonald et al., 2020).Laboratory and field measurements show that marine CH 2 Br 2 and CHBr 3 are co-products of the bromoperoxidase process operating in marine diatoms (Mehlmann et al., 2020;Moore et al., 1996;Hughes et al., 2013), with CHBr 3 the primary product of peroxidase-HOBr chemistry, and CH 2 Br 2 formed from CHBr 3 by bacterial action (Hughes et al., 2013).Abiotic HOBr chemistry, including water disinfection processes, produces CHBr 3 predominately (Maas et al., 2019;Mehlmann et al., 2020), so elevated CHBr 3 relative to CH 2 Br 2 would be a marker for the atmospheric chemistry that initiates and perpetuates the bromine explosion.This aspect is borne out by the observations of organic bromine compounds in the Antarctic winter (i.e., in the absence of photosynthesis) where CHBr 3 /CH 2 Br 2 ratios were often 10 or higher (Abrahamsson et al., 2018).The source of active bromine in Abrahamsson et al. (2018) was hypothesized to be the dark reaction of ozone with bromidecontaining solutions or ice, a process for which there is substantial experimental evidence (Artiglia et al., 2017;Oum et al., 1998;Sakamoto et al., 2018;Clifford and Donaldson, 2007).
The atmospheric loss processes of XCN compounds have not been studied extensively, but there are some limits that can be placed on them.Reactions of the radicals OH and Cl atoms with XCN compounds are likely quite slow (< 10 −13 cm 3 molec.−1 s −1 ) because any direct abstraction reactions (e.g., OH + BrCN → HOBr + CN) are highly en-dothermic, and addition reactions to the -CN group are expected to be quite slow by analogy to HCN and CH 3 CN reactions (Manion et al., 2020).XCN photolysis has been estimated to range from no tropospheric photolysis of ClCN, to a BrCN photolytic lifetime of ∼ = 135 d, to an ICN lifetime of ∼ = 9 h at ultraviolet wavelengths at summertime midlatitudes (Fig. S1 in the Supplement).The solubility and hydrolysis rates of XCN compounds have been measured under a variety of conditions (Roberts and Liu, 2019).That study showed that solubilities of ClCN and BrCN are relatively low (4.5 and 33 M atm −1 ) at 273 K, respectively), and their hydrolysis reactions are known to be base-catalyzed (Gerritsen et al., 1993) and relatively slow at ambient pH values (< 1 × 10 −5 s −1 at 273 K).The net effect of these features is that while ICN can photolyze relatively readily, ClCN and BrCN removal from the troposphere is likely governed by heterogeneous uptake and reaction with materials in those matrices, whether that be aerosol, cloud, or surfaces.
There have been almost no reported observations of XCN compounds in the gas phase in environmental systems in spite of the facile chemistry that forms XCN compounds in aquatic chemistry.ClCN has been observed by protontransfer-reaction high-resolution time-of-flight mass spectrometry (Mattila et al., 2020) in indoor air during experiments in which a home was cleaned with chlorine bleach solution, but to our knowledge, neither BrCN nor ICN has been observed previously in the atmosphere.Two factors may be responsible for the lack of ambient measurements of XCN compounds: (1) other chemical loss processes removing XCN species are likely much faster than hydrolysis, and (2) sensitive online analytical techniques for their measurement have only recently been available.
Here we report observations of BrCN in the global atmosphere during the second, third, and fourth deployments of the NASA Atmospheric Tomography (ATom) experiment in January-February 2017, September-October 2017, and April-May 2018 (Thompson et al., 2022).The measurements were obtained aboard the NASA DC-8 research aircraft by trifluoro methoxide (CF 3 O − ) chemical ionization with time-of-flight mass spectrometry detection (hereafter referred to as CIT-CIMS) during ATom-1, ATom-2, ATom-3, and ATom-4 and by iodide ion chemical ionization with high-resolution time-of-flight mass spectrometry (hereafter referred to as the I-CIMS) (Veres et al., 2020) during ATom-3 and ATom-4.The I-CIMS was not deployed for ATom-1 and ATom-2.The project also provided an extensive suite of co-measured species used to assess the relative role of biotic and abiotic BrCN production mechanisms.This paper summarizes the geographic distributions of BrCN and presents several case studies of large BrCN enhancements.We then present evidence showing that a significant fraction of BrCN was produced from active Br chemistry.

Experimental design
The ATom experiment was an extensive project, with a wideranging set of chemical and physical measurements during four separate seasonal deployments aboard the NASA DC-8 research aircraft.An overview of ATom has been given elsewhere (Thompson et al., 2022), so only aspects pertinent to this work will be discussed here.Two instruments detected BrCN during the ATom deployments: a time-offlight mass spectrometer that employed trifluoro methoxide (CF 3 O − ) ionization (CIT-CIMS) flew during all four deployments, and a high-resolution time-of-flight mass spectrometer that employed iodide ion ionization (I-CIMS) flew only on the third and fourth global circuits (ATom-3 and ATom-4) in October 2017 and May 2018.The aircraft sampled the troposphere from 86°S to 83°N in more than 180 vertical profiles in each mission interspersed with level legs (the term "level leg" refers to a flight segment during which the aircraft maintained a constant altitude (± a few percent) for at least several minutes or more) that ranged in altitude from about 0.150 to 13.2 km, with missed approaches (MAs) over Arctic airports as low as 0.043 km.The term "missed approach" refers to a flight period during which the aircraft descended into the controlled airspace above a designated airfield, almost to the point of touching down, and climbed back out.

I-CIMS
The measurement of BrCN during ATom-3 and ATom-4 was accomplished using a high-resolution time-of-flight mass spectrometer (Aerodyne Research, Billerica, Massachusetts) that employed iodide ion adduct ionization chemistry.The instrumental conditions were described by Veres et al. (2020) and included control of pressure and water vapor concentration in the ion-molecule reaction (IMR) region.The resolving power of the mass spectrometer was approximately 5000 (m/ m) in the mass range of interest.This resolving power, coupled with the negative mass defect of Br, yields a clear signal for BrCN, even for relatively small amounts (5.3 pptv) as shown in Fig. 1.BrCN is detected as the I − adducts, I q Br 79 CN − and I q Br 81 CN − , and those ions were well separated from other ions that appear at the same nominal mass.The combination of mass separation and isotope relative abundance provides conclusive identification of BrCN.The aircraft inlet for I-CIMS BrCN measurements has been partially described previously (Veres et al., 2020).Additional information is that the inlet consisted of a 0.75 m length of 0.75 cm ID PFA Teflon tubing thermostated at 35 °C and had a flow rate of 6 slpm.The instrument background for the BrCN signal was determined by overflowing the instrument inlet with scrubbed ambient air every 8 min for a 30 s period, and the detection limit of the measurements was determined by the variability in the residual signal at that mass.The scrubber system consisted of ambient air pumped from a separate aircraft inlet, via a diaphragm pump, through a packed trap containing activated charcoal, Purafil, Puracarb AM, and Chlorosorb Ultra and added to the main inlet periodically as an overflow.The scrubber material was independently checked for removal of halogens (Br 2 , Cl 2 , and BrCl) and other analytes of interest and found to be more than 99 % efficient at removing these dihalogens.We have every reason to expect that this scrubber also removed BrCN; however, we have examined zeroing periods that occurred in the middle of BrCN measurements that show this to be the case.An example of such a period is shown in Fig. S2 in the Supplement from the 19 October 2018 flight, in which several of the zero periods happened during elevated BrCN periods.The signals during those zeroing periods indicate that the scrubber was at least 92 % efficient at removing BrCN.Also, all the zero periods exhibited non-varying signals at, or lower than, the adjacent ambient signals observed.
Calibration of the XCN compounds was accomplished using the method described by Roberts and Liu (2019) following the ATom-3 deployment.ClCN was produced by conversion of a calibrated mixture of HCN in air to ClCN in a reactor containing chloramine-T (N -chloro-ptoluenesulfonamide sodium salt).The concentration of this calibrated stream was verified by a total reactive nitrogen (N r ) instrument (Stockwell et al., 2018) to be in the range of tens of parts per billion by volume at the CIMS inlet flow rates and the presence of ClCN confirmed by analysis with a high-resolution proton-transfer-reaction time-of-flight mass spectrometer (Hi-Res-PTR-ToF).The Hi-Res-PTR-ToF and its operating conditions have been described in the literature (Yuan et al., 2016(Yuan et al., , 2017)), and the compound was detected at ClCN q H + , a process greatly aided by the Cl iso-tope distribution and negative mass defect.The I-CIMS had no discernible response to ClCN at I q ClCN − or potential fragment ions.A similar absence of sensitivity to ClCN was also found in a study of indoor air chemistry during chlorine bleach treatment (Mattila et al., 2020), where a PTR-MS was able to observe ClCN but the I-CIMS deployed in the same study did not detect it (James Mattila, personal communication, 2020).Standard streams of BrCN and ICN in zero air were produced using the pure compounds (Sigma-Aldrich and Acros Organics, respectively) placed in diffusion cells and calibrated by the N r instrument under constant temperature and pressure conditions.The conversion efficiency of the N r catalyst was found to be 98 ± 10 % for ClCN and assumed to be the same for BrCN and ICN based on the X-CN bond energies of these molecules (Table S1 in the Supplement).The I-CIMS was calibrated at BrCN mixing ratios in the range of 18-68 ppbv, and response was found to be linear over that range.The IMR temperature was held constant at 40 °C during the sensitivity determinations and for a majority of the ambient measurements.The temperature dependence of the I-CIMS sensitivity to BrCN was determined in the laboratory to be nearly identical to that of formic acid (Robinson et al., 2022) and was used to correct the data from the flights on 25 and 27 October 2017 during which the IMR was operated at 45 °C.The I-CIMS sensitivity was also found to decrease with increased IMR water vapor concentration, in the manner shown in Fig. S3 in the Supplement, and the ion signals were normalized using the I q H 2 O − ion.Response factors were then determined for the conditions corresponding to the ATom-3 and ATom-4 deployments.The I-CIMS was approximately 8 times more sensitive to ICN compared to BrCN, which combined with the ClCN result gives I-CIMS relative sensitivities in the order ICN > BrCN > ClCN.Clear signals for ICN were observed in ambient air at the I q ICN − product ion, but the large instrument backgrounds caused by the use of iodide as the reagent ion prevented quantitation of ICN (see Sect. 3.2.1 below).Generally, detection limits of 1.5 pptv (3× standard deviation of the signal at zero BrCN) for a 10 s average with overall uncertainties of 0.4 pptv +25 %, as calibrated, pertain to most measurements, with the exception of the flights during ATom-4 on 12, 17, and 21 May 2018, during which the detection limit was 6 pptv for 10 s averages due to increased water vapor in the IMR and corresponding decreased sensitivity.
The instrument time response for BrCN was found to be fast (τ ∼ 1.5 s) both during calibration experiments and in assessing the time variability of signal attributed to ambient BrCN.Several pieces of evidence argue against significant loss of BrCN inlets.(1) BrCN equilibrates rapidly in the short PFA inlet, consistent with our understanding of the behavior of inorganic species on Teflon inlets as a function of Henry's law (Liu et al., 2019).(2) BrCN hydrolysis is relatively slow and is base-catalyzed (Roberts and Liu, 2019), and inlets used during ATom were acidic due to exposure to acidic aerosol (Nault et al., 2020), so loss of BrCN due to hydrolysis is not expected.
The potential formation of BrCN on the inlet surfaces of the instrument needs to be considered since it might involve the same chemistry that makes BrCN in the environment, i.e., the reaction of HOBr with reduced N species on inlet surfaces.Several pieces of evidence indicate a lack of any BrCN production in our system.First, calibrations of the instrument with Br 2 and BrO standards before and after these missions did not result in any observable BrCN above the detection limit.Second, the solubility, and therefore surface concentration, of HCN (a likely reaction partner) is quite low at the temperature at which the inlet was operated (40 °C).In contrast, the inlet is more likely to collect non-volatile Br − and convert HOBr to Br 2 , as demonstrated by previous measurements in the Arctic troposphere (Neuman et al., 2010).As noted above, both of these heterogeneous processes are also pH-dependent, and Br 2 will be much more favored at lower pH values that are likely present in the surface layers of the PFA inlet (Nault et al., 2020).The NOAA group has conducted preliminary lab tests aimed at examining the temperature and pH dependence of the Br 2 + HCN chemistry on ice/water surfaces and confirmed the absence of BrCN production in the absence of a high-pH aqueous surface on which it can take place.These experiments are described in the Supplement.
Several other halogen species were measured with good sensitivity by the I-CIMS as their I − adducts: Cl 2 , ClNO 2 , BrCl, and BrO (see Table S2 in the Supplement).Methods for the calibration of the I-CIMS for those species have been described previously (Neuman, et al., 2010;Osthoff, et al., 2008;Wild, et al., 2014) and were applied to the calibration of the ToF-CIMS used in this work.Significant losses of BrO on the actual I-ToF CIMS inlet were not apparent during calibrations that were performed before and after both ATom-3 and ATom-4 deployments.In addition, the intercomparison of in situ BrO measurements by CIMS with long-path differential absorption spectroscopy (LP-DOAS) reported by Liao et al. (2011) and tests reported by Liao et al. (2012a) provides further evidence that once flow into a Teflon inlet is properly initiated, an inlet of our type would not have significant BrO losses.Aside from a large shroud that was required to establish flow from a static air mass (Liao et al., 2012b) (not required for an aircraft inlet), the key feature of the Liao et al. (2011) CIMS inlet was a short section of PFA Teflon tubing heated to 40 °C and operated at high flow rates.Liao et al. (2011) report excellent agreement between the two methods for periods of steady wind flow without local NO pollution.Our inlet is slightly longer than that CIMS inlet but was made of the same material and operated at a high flow rate.
Laboratory tests were conducted during ATom calibrations to assess the amount of loss of BrO in the instrument inlet used in ATom.Those tests compared the signals observed when adding the BrO source directly to the IMR, with those observed with the addition of the 0.7 m long ATom inlet ophttps://doi.org/10.5194/acp-24-3421-2024Atmos.Chem.Phys., 24, 3421-3443, 2024 erated at 6.3 slpm.The results showed that the ATom inlet transmitted 90 ± 4 % of BrO, leading us to conclude there was minimal loss of BrO.We further note that this inlet loss was accounted for in the applied calibration factor, determined with the ATom inlet in place.We have not observed evidence of any other losses of BrO on the ATom inlet.Previous work has shown that Br 2 and HOBr measurements are not reliable with the inlet used on the aircraft due to interconversion reactions noted above (Neuman et al., 2010), so those species were not quantified.However, we will present some qualitative data on these species in the Results section that support our observations of active Br chemistry.

CIT-CIMS
HCN was measured by the Caltech chemical ionization mass spectrometer using a CF 3 O − reagent ion.HCN forms a cluster ion with CF 3 O − and is detected at m/z 112 (Crounse et al., 2006).HCN was calibrated before and after each ATom deployment, and a temperature-and water-dependent sensitivity was used to convert the signal at m/z 112 to HCN concentrations after accounting for instrumental backgrounds determined by periodic zero measurements.The CIT-CIMS instrument was zeroed every 15 min in flight by closing the instrument to ambient air sampling and adding ultrahighpurity (UHP) N 2 gas.A second type of zero was also performed every 15 min by flowing ambient air through a filter containing NaHCO 3 -coated nylon wool and palladiumcoated alumina pellets.Both types of zero generally agree well, except at very high ambient RH where HCN is not efficiently scrubbed by the NaHCO 3 filter.CIT-CIMS HCN calibration was performed in the lab using a compressed gas mixture of HCN in N 2 , and a dilution system composed of three mass flow controllers, and additional N 2 gas source (liquid nitrogen, LN 2 , boil-off).Fourier-transform infrared spectroscopy (FTIR) measurements were used to quantify and monitor the stability of the HCN mixing ratio in the compressed gas mixture using HITRAN HCN lines strengths.The laboratory HCN calibrations were proxied to flight data using periodic in-flight calibrations (every ∼ 3 h) of other species (H 2 O 2 , peroxy acetic acid, and ethylene glycol), after accounting for appropriate water vapor and temperature dependencies.
BrCN was also detected by CIT-CIMS as CF 3 O − cluster ions at m/z 190 and 192.The inlet of the CIT CIMS has been described previously (Crounse et al., 2006;Allen et al., 2022) and consisted of an ∼ 80 cm fluoro-polymer-coated (Fluoropel PFC 801A, Cytonix Corp) glass tube under high flow (ambient pressure flow > 50 m s −1 ) with the axis perpendicular to the direction of flight with an aft-facing cut, preventing cloud droplets and large aerosol particles from being sampled in the inlet.The signal at m/z 192 occasionally contained contributions from other molecules -signals that do not appear at m/z 190.Thus, the m/z 190 signal was used for quantifying BrCN, dividing the signal by its iso-topic abundance of 79 Br (0.51) due to the calibration method employed.When the signal at m/z 190 was elevated, the enhancement at m/z 192 was as well, reflecting the approximately equal abundance of 79 Br and 81 Br.Independent BrCN temperature-and water-vapor-dependent calibration factors for CIT-CIMS were determined in the Caltech laboratory using simple manometry in combination with FTIR spectroscopy.Five IR spectra with varying BrCN concentrations were collected as part of the calibration and compared to the sum of the mass spectrometer (MS) signals at m/z 190 and 192.An integrated absorption cross-section for the band centered at 2198 cm −1 was determined (2110-2250 cm −1 band: 1.08 × 10 −18 cm molec.−1 , log base-e at 298 K).To the extent that other gases are present in the BrCN vapor sample, the integrated IR cross-section and the CIMS sensitivity represent lower limits, and in turn derived ambient concentrations represent upper limits.The CIT-CIMS was calibrated for BrCN over the range of 3-130 ppbv and the response was found to be linear over this range.The 1σ BrCN precision for CIT-CIMS 10 s data, as calibrated, is 2.5 pptv.
Ambient BrCN mixing ratios from CIT-CIMS were compared with those from I-CIMS for two ATom-4 flights with the highest BrCN: 27 April 2018 and 19 May 2018.The BrCN mixing ratios from the CIT-CIMS are scattered against those from the I-CIMS in Fig. S4a for the two flights and in Fig. S4b from the data points for which the I-CIMS mixing ratio was > 3 pptv.The data in Fig. S4b were fit using an orthogonal-distance regression (ODR) that assumes uncertainty in both variables.The slope of the correlation of CIT-CIMS versus I-CIMS is 0.52 ± 0.01 and the intercept is −0.34.At this point it is not possible to privilege one calibration method and dataset over the other, so they were harmonized by correcting the two datasets to the mean.Accordingly, the I-CIMS data were multiplied by 0.76 and the CIT-CIMS data were multiplied by 1.46.As a result, the correct uncertainties of the I-CIMS BrCN measurements were 0.3 pptv + 50 %, with a detection limit of 1.1 pptv, and the 10 s precision of the CIT-CIMS measurements was 3.7 pptv.The I-CIMS data have an approximately 5 times better signal-to-noise ratio than the CIT-CIMS.Consequently, the I-CIMS data are used in the analyses of the ATom-3 and ATom-4 flights, and the CIT-CIMS data are used in the analyses of the ATom-2 Arctic flights, the only other instances in which the CIT BrCN was above the detection limit.The oxides of nitrogen, including nitric oxide (NO), nitrogen dioxide (NO 2 ) and total odd nitrogen (NO y ), as well as O 3 , were measured by a four-channel chemiluminescence system as described previously (Bourgeois et al., 2021).The inlets for the O 3 and NO y chemiluminescence instruments have been described previously (Bourgeois et al., 2020) (Ry-erson et al., 1999).The inlet for the NO measurement consisted of a 1.5 m long 4 mm i.d.PFA tube thermostated at 30 °C at a flow rate of 1 slpm, coupled to a fused silica tube of 12 mm i.d. and 450 mm length, used to match the residence time to the NO 2 channel of the instrument.The use of PFA Teflon for NO and O 3 sampling is well established, and losses of NO or O 3 due to chemical reactions would only be expected under extreme circumstances (sampling of highly polluted air with extremely high VOCs or NO).The NO y inlet consisted of a solid-gold tube situated in the aircraft inlet and heated to 300 °C.The loss or incomplete conversion of NO y species in the NO y convertor is routinely checked through the addition of NO 2 and HNO 3 standards and found to be negligible.The estimated uncertainties for these measurements and the instrument precision are ± (5 % + 6 pptv) for NO, ± (7 % + 20 pptv) for NO 2 , ± (12 % + 15 pptv) for NO y , and ± (2 % + 15 pptv) for O 3 .

Whole-air sampler
Bromoform (CHBr 3 ), dibromoethane (CH 2 Br 2 ), methyl bromide (CH 3 Br), and methyl iodide (CH 3 I) were measured during ATom-2, ATom-3, and ATom-4 using UC Irvine whole-air sampling (WAS).The WAS technique during airborne missions has been recently described by Simpson et al. (2020).Briefly, air from outside the aircraft was drawn through a stainless-steel manifold by a dual-head metal bellows pump into individual evacuated 2 L stainless-steel canisters that were sequentially filled to a pressure of 40 psig (roughly 3 atm).Air samples were collected at the discretion of samplers on board the aircraft.The average canister fill time was 53 ± 21 s (22-136 s) during ATom-2, 54 ± 25 s (18-181 s) during ATom-3, and 52 ± 24 s (16-198 s) during ATom-4, and the average sampling frequency was every 2.6 min for all missions.A total of 303 samples were collected for the two Arctic legs of ATom-2, and 1933 and 1853 samples were collected during ATom-3 and ATom-4, respectively, for an average of 149 and 143 whole-air samples per flight.The filled canisters were returned to UC Irvine and analyzed using multi-column gas chromatography.Complete analytical details and calibrations procedures are given in Simpson et al. (2020).The measurement precision is 5 % for CH 3 I, CH 3 Br, and CH 2 Br 2 and 10 % for CHBr 3 .The accuracy is 10 % for CH 3 Br and 20 % for CH 3 I, CH 2 Br 2 , and CHBr 3 .The detection limit is 0.005 pptv for CH 3 I, 0.5 pptv CH 3 Br, and 0.01 pptv for CH 2 Br 2 and CHBr 3 .

UV-visible actinic flux measurements
Photolysis frequencies were determined from chargedcoupled device actinic flux spectroradiometers (CAFSs) (Hall et al., 2018).Up and downwelling actinic flux is collected by 2 pi steradian optical collectors above and below the aircraft fuselage.The signals are directed via fiber optics to spectrometers to provide spectrally resolved fluxes from 290-640 nm.The photolysis frequencies are then calculated by applying the total actinic fluxes to molecular crosssections and quantum yields contained in the tropospheric ultraviolet and visible (TUV) radiative transfer model (v5.3) (Madronich and Flocke, 1999).Typical molecularly dependent uncertainties range from 12 %-20 %.

Box model description
The model used to explore the formation of BrCN in the Arctic environment has been described previously (Wang and Pratt, 2017).It includes gas-phase reactions, photolysis reactions, multi-phase reactions on both aerosol particles and snow, liquid-phase reactions in both deliquescent particles and liquid-like layers on snow and ice, and dry deposition of trace gases.The liquid-phase reactions of active bromine compounds with HCN/CN − were added according to the reactions and rates specified in the Supplement.The conditions and chemical measurements corresponding to the 27 April 2018 missed approach over Utqiagvik, Alaska, were used to initialize the model.

Statistical methods
Statistical analyses were performed using the standard routines for averaging and ODR fitting provided by Igor Pro Version 8 software.

Results
The flight paths of the NASA DC-8 during ATom-2, ATom-3, and ATom-4 provide a unique opportunity to assess the global extent of BrCN, as those flight paths consisted of alternating high-and low-altitude legs around most of the global background troposphere with vertical profiles in between.The ATom-2 observations by the CIT-CIMS are limited to Arctic wintertime and will be presented below.Maps summarizing ATom-3 and ATom-4 data from the I-CIMS instrument are shown in Fig. 2, where the flight paths are shown as colored and sized by BrCN mixing ratios.BrCN mixing ratios ranged from below the detection limit (1.1 pptv) up to 10 pptv for a 10 s average during ATom-3 and up to 36 pptv for a 10 s average during ATom-4.The highest BrCN mixing ratios observed during ATom-3 occurred during the low-level legs that dipped into the boundary layer at high latitudes (below 65°S and above 65°N), and the remaining observations were at or below the detection limit, which was consistently 1.1 pptv for the ATom-3 campaign.Likewise, the highest mixing ratios observed during ATom-4 occurred during low-level legs at high latitudes, but the degraded instrument sensitivity during the 12, 17, and 21 May flights (detection limit 4.6 pptv) resulted in greater variability at low mixing ratios on the ATom-4 map (Fig. 2b).Two points of comparison show that the BrCN from wildfire (WF) is quite small to negligible.Biomass burning (BB) plumes https://doi.org/10.5194/acp-24-3421-2024Atmos.Chem.Phys., 24, 3421-3443, 2024  Previous work that observed BrCN production from a marine diatom (Nitzschia cf pellucida) (Vanelslander et al., 2012) in laboratory cultures presents the possibility that the BrCN observed during ATom was emitted from marine biota.However, several aspects of the timing and location of the ATom observations argue against there being a significant biological source over most of the globe.BrCN was not observed in the marine boundary layer (MBL) over the areas of the ocean that had the highest biological productivity, as shown by the map in Fig. S5, which overlays the ATom flight tracks with the mean chlorophyll a surface concentration as compiled by the NASA Earth Observatory (NASA, 2020).Unfortunately, this satellite product does not work over areas having significant ice cover (higher latitudes), so we cannot rule out a source from sea ice biological communities.
The CIT-CIMS Arctic winter flights from ATom-2 make up the other set of observations that provide strong evidence that BrCN is a product of abiotic Br chemistry.The two flights on 18 February 2017 from the Azores to Thule, Greenland, and 19 February 2017 from Thule to Anchorage, Alaska, involved low-level legs over Baffin Bay and the Arctic Ocean, as well as MAs over BRW and the Prudhoe Bay/Deadhorse airport (SCC).A map of the ATom-2 flights where BrCN was observed is shown in Fig. S6.There was greatly reduced photosynthetic activity at the northern latitudes during this time compared to May 2018, yet BrCN and the ratio of CHBr 3 to CH 2 Br 2 were highly correlated (Fig. 4) and CHBr 3 /CH 2 Br 2 reached levels previously observed in the Antarctic winter (> 10) (Abrahamsson et al., 2018).The data for all points in both flights imply a background in CHBr 3 /CH 2 Br 2 of 2.7 ± 0.3 based on the x intercept in Fig. 4. Late winter photochemical production of Br 2 and I 2 has been noted in the snowpack at Utqiagvik, AK (Custard, et al., 2017;Pratt, et al., 2013;Raso, et al., 2017), and was probably the major source of Br 2 in this environment (Pratt et al., 2013).This active Br source participated in some O 3 destruction as indicated by some low-O 3 points in the vertical profile shown in Fig. S7, but BrCN was not closely anticorrelated with O 3 .Also, BrCN and CHBr 3 appear to be produced from reaction of active Br with dissolved organic nitrogen (DON) and DOM, but the biogenic processing of CHBr 3 to CH 2 Br 2 was greatly reduced compared to other seasons due to lower photosynthetic activity and lower temperatures.Note that ATom-1 took place during the austral winter (August, 2016), but unlike ATom-3 and ATom-4, the aircraft did not travel south of 65.3°S, no CHBr 3 /CH 2 Br 2 ratios above 2.5 were observed during that flight, and no BrCN above the CIT-CIMS detection limit was observed during the entire ATom-1 campaign.
We examine detailed measurements from ATom-3 and ATom-4 below for signs of O 3 destruction, as well as CHBr 3 and BrCN formation.These processes are in competition with one another, as they all depend on HOBr/Br 2 chemistry.The product channels depend on the availability of the reaction substrates -Br − , DOM, and dissolved organic nitrogen (DON) -and on reaction conditions (e.g., pH).As a result, we would expect some coincidence in time and space, but not necessarily close correlations between O 3 loss, excess CHBr 3 , and the appearance of BrCN.

Case studies
The following analysis focuses on case studies of locations within the polar boundary layer that had BrCN enhancements, since BrCN was below the detection limit throughout much of the troposphere.The data will be examined for evidence of coincident BrCN appearance and O 3 destruction chemistry, covariation of BrCN with other bromocarbons that might differentiate between biotic and abiotic origins, and indications of the processes that govern BrCN atmospheric lifetimes and removal processes.The highest BrCN observed during Southern Hemisphere spring was over the Weddell Sea during the 14 October 2017 flight of ATom-3 at about 15:15 UTC and about 68°S latitude.This polar boundary layer leg was also over sea ice at 170 m.However, in contrast to the 11 October 2017 polar boundary layer leg, this vertical profile shows that the polar boundary layer did not have a constant potential temperature even down to the lowest altitude sampled (Fig. S10 in the Supplement).As a result, the time profiles of BrCN and HCN showed considerable variability at the lowest altitudes, and it is not clear from other key species, including BrCl, halocarbons, and the vertical profile of O 3 , how much Br-associated O 3 destruction had occurred within this polar boundary layer environment.
We observed the first firm evidence of O 3 destruction and the association of BrCN with active Br chemistry later on the 14 October 2017 flight during the polar boundary layer leg centered around 18:20 UTC ranging from 75-76°S latitude.During these vertical profiles, there was evidence of O 3 loss and anticorrelation of O 3 and BrCN concentrations as shown in Fig. 5a and b.While it is difficult to identify a "background" O 3 level, i.e., a level of O 3 that would be present in the absence of local production, destruction, or mixing down of stratospheric O 3 , it seems clear from the entirety of the 14 October 2017 flight that O 3 mixing ratios are in the range of 30-40 ppbv in this environment (over the Weddell Sea) at mid-tropospheric altitudes (2-6 km).Unfortunately, video from the DC-8 is not available for that flight.The TER-RA/MODIS imagery from that date (NASA and Worldview, 2018) and nearby dates indicates that the Weddell Sea was largely frozen, but there was some indication from back trajectories that these air masses had passed over open leads.During the profiles shown in Figs.5a and b, O 3 between 2 and 4 km was on the order of 32 ppbv (dashed lines in Fig. 5a and b), while O 3 at lower altitudes was sometimes below 20 ppbv and those levels were anticorrelated with BrCN.This type of profile is consistent with active Br chemistry that involves O 3 destruction and the production of BrCN from reactions involving active Br compounds and reduced nitrogen substrates.In addition to this evidence, CHBr 3 was elevated relative to the other bromocarbons (Fig. S11 in the Supplement), which is consistent with its abiotic production from reactions of HOBr with DOM in snow/ice and particle surfaces.
The 9 May 2018 flight during ATom-4 also flew over the Weddell Sea, this time during austral fall.The BrCN mixing ratio approached 11 pptv (10 s average) and coincided with high CHBr 3 /CH 2 Br 2 ratios (∼ 3) but very little apparent O 3 loss (∼ 1 ppbv) as shown in Figs.S12 and S13 in the Supplement.The aircraft was over the ice pack, with broken leads (areas of open water where the ice pack has broken up and separated), during the two low legs where elevated BrCN was observed (14:15 and 15:35 UTC) and there were substantial clouds present.

25 October 2017 and 19 May 2018: flights over the Arctic ice pack
The first episode in which BrCN was observed over the Arctic ice pack during ATom-3 was on the flight on 25 October 2017, which was the northernmost leg from Bangor (Maine, USA) to Anchorage (Alaska, USA).BrCN was elevated above the detection limit on four of the polar boundary layer legs at levels ranging from 3.8 to 10 pptv (10 s average; Fig. S14 in the Supplement).On each of those polar boundary layer legs, the aircraft did not reach a polar boundary layer with constant potential temperature.However, there was still some evidence for minor amounts of O 3 destruction (3-4 ppbv).
The 19 May 2018 flight was similar to the 25 October 2017 flight in that it started in Bangor and ended at Anchorage and constituted the northernmost leg of ATom-4.The interesting features of this flight are that each polar boundary layer leg (aside from the final approach into Anchorage) corresponded to elevated BrCN and some degree of O 3 destruction, as shown in Fig. 6.The photochemical environment during this flight was somewhat consistent due to the fact that the aircraft was traveling east to west during daylight hours, creating a situation in which the photolysis rates did not change much with time (see Fig. S15 in the Supplement).As a result, the rates associated with Br radical chemistry (Br 2 , BrCl, and HOBr photolysis) were relatively consistent throughout the flight: jBr 2 → 2Br was in the range of 0.05 to 0.08 s −1 .The vertical profiles of potential temperature for each of the polar boundary layer legs (see Fig. S16 in the Supplement) showed that the lowest layers had constant potential temperatures for all the legs except the one that was centered around 21:30 UTC (leg E).Each of the polar boundary layer legs during the 19 May flight displayed O 3 destruction, with the lowest O 3 on leg F averaging below 5 ppbv.Remarkably, these polar boundary layer legs displayed averages of O 3 and BrCN that were highly anticorrelated: R 2 = 0.94 (Fig. 7).That this anticorrelation was observed over such a wide geographic expanse could mean the that O 3 destruction chemistry was uniform (due to the relatively uniform photochemical environment).This concept is consistent with observations and analysis presented by Halfacre et al. (2014), Ridley et al. (2003), andJacobi et al. (2010)  (normalized to I q H 2 O − ).ICN was sometimes observed when BrCN was observed, but they were not closely correlated.In addition, the instrument background for ICN was relatively high and variable, and the signal in scrubbed air was sometimes slightly higher than in ambient air, often leading to apparent negative ICN mixing ratios.The high background was probably due to the fact that substantial amounts of CH 3 I were used to make I − ions in the ion source and could be involved in neutral chemistry or causing surface artifacts which served to obscure ICN signals that might have been there but were not discernible given the signal variability.

1 October 2017 and 27 April 2018: missed
Approaches over Utqiagvik, Alaska The ATom-3 leg that started on 1 October 2017 and flew from Palmdale, California, USA, to Anchorage also included an MA over BRW at Utqiagvik shown in Fig. S20 in the Supple- ment.It is instructive to examine the details of that flight as it stands in contrast to the ATom-4 MA which will be shown in detail below.This MA did not correspond to elevated BrCN concentrations; instead, the BrCN values were slightly below zero due to uncertainties in the subtraction of the instrument background during a zero, yet there is some evidence that the polar boundary layer might have experienced a moderate amount of O 3 destruction (∼ 10-12 ppbv).One of the main differences between the 1 October 2017 MA and that on 27 April 2018 was the presence of low-level clouds over BRW during the 1 October episode as indicated by reduced jBr 2 and confirmed by visual evidence (Fig. S21 in the Supplement).It could be that the formation of BrCN is inhibited by the presence of clouds and/or BrCN was removed by uptake and reaction in clouds.
The last detailed episode to be explored took place on 27 April 2018 during an MA over BRW and involved the highest BrCN observed for the entire project.The aircraft got as low as 40 m a.s.l. as it conducted the approach west to east over the runway that runs true east-west (see Fig. S22 in the Supplement).The wind direction was from 100-120°a nd ranged from 4-14 m s −1 in the lowest 2.5 km of the flight path, which means that the aircraft should not have sampled recent emissions from the town of Utqiagvik, as the town is mostly north and southwest of BRW.The bottom panel of Fig. S22 is an image from the video camera on the nose of the DC-8.It shows that the ocean adjacent to Utqiagvik was packed with sea ice at least 10 km out, but it is clear that further offshore there was a mixture of open water and ice.In addition, the atmosphere was relatively clear of clouds and particles.The time series of the relevant chemical measurements during this period (Fig. 8) show that BrCN was confined to the very lowest altitude of the MA.The halocarbon data showed no elevated levels of CH 2 Br 2 , CH 3 Br, and CH 3 I but significant enhancement (∼ × 3) in CHBr 3 at the lowest altitude compared to the layer just above.The vertical profiles of key chemical constituents and temperature are shown in Fig. 9 for the lowest 0.6 km of the MA.There is an indication of a locally impacted layer between 0.15 and 0.3 km directly above the polar boundary layer that had elevated NO y with an NO/NO y ratio of ∼ 0.5, but the lowest layer (< 0.15 km) had a constant potential temperature and had no evidence of local pollution.That lowest layer had BrCN up to 36 pptv (10 s average) and also elevated BrCl, and O 3 was as low as 32 ppbv, so it was reduced compared to the layer above the local pollution, which was about 45 ppbv at 0.35-0.6km.
As noted above, a general coincidence in time and place can be expected among BrCN formation, high CHBr 3 /CH 2 Br 2 ratios, and O 3 destruction because while they all depend on active bromine chemistry, they are also in competition with each other.So, it is not surprising that the BrCN and O 3 levels from the 27 April 2018 MA do not fit the BrCN-O 3 correlation from 19 May 2018 that is shown in Fig. 7.However, the dataset does show a general correspondence between the appearance of BrCN and the ratio CHBr 3 /CH 2 Br 2 as shown in Fig. 10a and b.The relationship appeared in both the Arctic and Antarctic flights but was most pronounced in the Arctic springtime.This correspondence is expected if CHBr 3 is formed from active bromine reacting with DOM, and BrCN from reaction with DON, as DON is a subset of DOM.We explore some of the possible relevant BrCN formation and destruction chemistry in the next section.
The observations of BrCN in polar boundary layer air have some intriguing implications for the active Br chemistry that occurs in these environments.If there is multi-phase chemistry occurring that terminates active Br during classic bromine explosion chemistry to form BrCN, then the active Br system works differently at destroying O 3 and Hg than is currently thought.This impact also depends on the fate of BrCN, which is not well understood since gas-phase loss processes are either known to be, or likely to be, very slow (Roberts and Liu, 2019).In addition, BrCN solubility in water is low, and its hydrolysis rates are slow at environmental pH values.Yet, circumstantial evidence (e.g., the near absence of BrCN above the polar boundary layer) indicates that BrCN has a relatively short atmospheric lifetime.The mechanism for heterogenous removal of BrCN is also unclear and could have implications for whether that chemistry could reform active Br or be a net sink for active Br.We discuss the possibilities for BrCN formation chemistry and some constraints and possible mechanisms of heterogeneous loss in this section.

BrCN formation
As noted above, formation of BrCN has been demonstrated in a number of chemical systems, both abiotic and from marine biota.The bulk of the evidence in ATom-2, ATom-3, and ATom-4 datasets is that BrCN formation occurs only in polar regions when there is active Br chemistry occurring.Conversely, neither the ATom-3 and ATom-4 deployments observed instances where there was substantial O 3 destruction and no measurable BrCN present.The destruction of O 3 , i.e., O 3 substantially below what is in the lowest 1-2 km of the atmosphere above, is one tell-tale sign of active Br chemistry.Another sign of active Br chemistry is the presence of elevated CHBr 3 concentrations relative to the closely related biogenic compound CH 2 Br 2 .These markers could be considered evidence that BrCN was produced from active Br chemistry.As a consequence, it is useful to consider what chemistry could be forming BrCN from active Br -i.e., what is the source of reduced nitrogen and how would the heterogeneous formation chemistry work?
As with all XCN compounds, it is difficult to devise a chemical scheme in which BrCN is produced via gas-phase chemistry.There are basically two reasons for this: Br atoms are either not very reactive or only moderately reactive with most organic compounds (Barnes et al., 1989) but reasonably reactive with O 3 (k = 1 × 10 −12 cm 3 molec.−1 s −1 ).As a consequence, reaction with O 3 will outcompete any organic reactions due to its higher abundance as long as O 3 has not been completely depleted, a condition not observed in the ATom dataset.Conversely, even if there were a source of CN radicals, which is quite unlikely, they react so rapidly (for example with O 2 ) that it is highly improbable that there could be a Br compound that could compete with other CN reaction partners in rate or in mechanism (Manion et al., 2020).
The production of BrCN by heterogeneous or condensedphase (i.e., snow, ice, frost flower, aerosol particles) chemistry is much more plausible as condensed-phase mechanisms are known.However, there are still a number of unknowns that make it difficult to construct a quantitative model.Rate constants and solubilities of the key reactants are not known in what is presumably a liquid-like layer of water below 273 K.The active Br compounds that are involved are Br 2 and HOBr, but the identity and chemistry of the N-containing substrates are uncertain.The possibilities are HCN/CN − and reduced N moieties (amines, amides, amino acids) that are part of the DON present in polar environments.These DON compounds can be resident on particles (Dall'Osto et al., 2017) or ice/snow surfaces that are known to collect organic materials from a number of sources (McNeill et al., 2012).These include deposited atmospheric aerosol, sea spray, frost flowers, and seawater that has been wicked up into the ice floe.These sources by their nature are mostly DOM and hence provide the substrates needed to produce CHBr 3 from HOBr through the haloform reaction.Thus, we would expect BrCN and CHBr 3 enhancements to be coincident in time and location, which is what is observed in our polar boundary layer data.
It is useful to examine whether reaction of HCN/CN − on snow or ice to form BrCN could compete with propagation of Br explosion chemistry through known mechanisms and how conditions, particularly substrate pH, might affect BrCN formation from that pathway.Simple calculations based on the competition of HOBr between reaction with HCN/CN − to make BrCN and reaction with Br − or Cl − to make Br 2 or BrCl, as well as a box model calculation with more extensive Br chemistry (Wang and Pratt, 2017), are presented in the Supplement and only summarized here.The competitive reaction analysis showed a profound pH dependence with higher BrCN formation at higher pH (Figs. S23 and S24 in the Supplement).This was due to the pH dependence of HCN solubility and HOBr/OBr − equilibrium and also pH dependences of HCN/CN − reactions with HOBr/OBr − .Higher Cl − and Br − concentrations will serve to shift the pH at which BrCN becomes competitive to higher values, but the range still appears to be 6.5-8.5 pH units, a range that is applicable to matrices in polar environments.The box model with more extensive Br chemistry also showed a pH dependence, with higher BrCN favored at higher pH (Fig. S25 in the Supplement), but more Br propagation at mid-range pH because of pH-independent Br chemistry in the model.We are not aware of any measurements of CN − in natural snowpack or sea ice.
The pH of condensed phases in the Arctic environment can range from fairly acidic (pH 1-2) for aerosols (Nault et al., 2020) to over pH 8 for frost flowers or sea spray aerosol (Kalnajs and Avallone, 2006).In addition, the pH of sea ice is somewhat buffered at relatively high pH values (Wren and Donaldson, 2012), providing a persistent matrix for BrCN formation from HCN/CN − and other reduced N compounds.So, the coincidence of BrCN with elevated CHBr 3 and O 3 depletion seen in some of the data presented here is consistent with abiotic active Br chemistry.However, if the competition between production of BrCN and the propagation of active Br is pH-dependent, we would not necessarily expect the tight anticorrelation shown in Fig. 7 for the 19 May 2018 flight, unless the conditions in which this chemistry was taking place were relatively uniform over thousands of kilometers.Moreover, the fact that the BRW MA data do not fit the data from the 19 May 2018 flight might simply be due to differences in the amount and pH of the DON substrate available for reaction.
The observation that dihalogens are produced by photochemistry in the snowpack (Pratt et al., 2013;Custard et al., 2017;Halfacre et al., 2019) also presents the possibility that BrCN and CHBr 3 are produced by DON and DOM in that environment, the key reactions being with Br 2 or HOBr that are produced in the condensed phase.Since both BrCN and CHBr 3 are relatively insoluble they would be readily emitted to the atmosphere.Another intriguing possibility exists for the production of BrCN (and other active Br compounds) in snow/ice environments.The production of active Br in algae, HOBr in particular, is an enzymatic process that involves the reaction of H 2 O 2 and Br − in the presence of a peroxidase.As such, HOBr production is intimately tied to photosynthetic processes as has been shown in several laboratory studies (Hughes et al., 2013;Vanelslander et al., 2012;Moore et al., 1996).It is therefore possible that dihalogen production, along with BrCN and CHBr 3 , could appear photochemical in nature but in fact rely on the presence of photosynthetic algae and, in the case of BrCN and CHBr 3 , the presence of DON and DOM substrates that would go along with algae in this environment.Again, the correlations of BrCN with O 3 destruction argue for a substantial source of BrCN from abiotic active Br chemistry at least some of the time.

BrCN loss
As described in the Introduction, gas-phase loss processes of BrCN are either known to be slow (photolysis lifetime at UV wavelengths ∼ = 4 months at summer midlatitudes) or quite likely to be slow (OH and Cl radical reaction rate constants < 10 −14 cm 3 molec.−1 s −1 by analogy to HCN and CH 3 CN) (Manion et al., 2020).The heterogeneous loss of BrCN to surfaces, particles, or cloud water has only been estimated based on aqueous solubilities and a few liquid-phase reaction rates, e.g., hydrolysis and reaction with n-octanol (Roberts and Liu, 2019) and those range from several weeks to 0.5 years.There are numerous references on solutionphase reactions that BrCN undergoes, but we were not able to find quantitative information about reaction rates (see, for example, Li and Gevorgyan, 2011;von Braun and Schawarz, 1902;Van Kerrebroeck et al., 2022).At this point it is worth examining the ambient measurements for further indications of what the BrCN lifetime is in the polar boundary layer.Figure 11 shows vertical profiles of potential temperature, ozone, BrCN, and the halocarbons CH 2 Br 2 and CHBr 3 from the 19 May 2018 polar boundary layer leg at 22:30 UTC that was discussed above in Sect.3.2.1.There was very little BrCN above the polar boundary layer, and this was a general feature of all the instances where BrCN was observed.It is clear that BrCN shows a much sharper decrease with altitude than the bromocarbons (CHBr 3 , CH 2 Br 2 ) that have lifetimes on the order of 2-4 months at this latitude and season (Papanastasiou et al., 2014;Hossanini et al., 2010); thus, BrCN must have a shorter lifetime than those compounds.
Most of the observations of elevated BrCN occurred within layers that had constant potential temperature and appeared relatively well mixed; i.e., O 3 was depleted but constant.However, the interpretation of these measurements is complicated by the fact that our observations did not extend to the surface.Observations in polar boundary layers show https://doi.org/10.5194/acp-24-3421-2024Atmos.Chem.Phys., 24, 3421-3443, 2024 that there are often very shallow stable layers (a few to tens of meters) close to the surface (Anderson and Neff, 2008) below a relatively well-mixed layer a few hundred meters to a kilometer in depth.This intermediate layer is usually capped by a strong temperature inversion and there are often clouds in the vicinity of the inversion (Serreze et al., 1992).Several model studies have shown that very low diffusivities (1 × 10 −3 m 2 s −1 ) best describe atmospheric observations in and above these layers (Zeng et al., 2006;Wang et al., 2008).By analogy to molecular diffusion, this corresponds to transport times out of the boundary layer through this inversion that are quite long (> weeks).The other factor that comes into play for many of these polar boundary layer legs is that many occurred over open leads in the ice, which are the source of vertical transport due to the effects of warmer water (Serreze et al., 1992).As a consequence, transport of BrCN out of the top of polar boundary layers is likely more limited by synoptic disturbances like frontal passage or ice lead formation.From these features we can roughly estimate that BrCN could have a lifetime as short as a day or two, but probably not longer than 10 d in the polar boundary layer, the upper limit being based roughly on the frequency of synoptic disturbances in this environment.It follows from this, and the slowness of gas-phase loss processes, that heterogeneous reactions limit the BrCN atmospheric lifetime.The rates of these possible condensed-phase reactions can be estimated in the same type of analysis employed by Roberts and Liu (2019) given a few assumptions about the polar boundary layers encountered in this work and Henry's law solubilities.Deposition of a chemical species within a boundary layer can be thought of as two processes happening in series: physical transport to the surface and chemical reaction at the surface (see, for example, Cano-Ruiz et al., 1993).These can be parameterized with a simple resistance model: where the total resistance is 1/v d , with v d being the deposition velocity, which can also be expressed as the mixing layer height, h, divided by the lifetime of the chemical species, in this case t BrCN ; γ is the surface uptake coefficient and c is the mean molecular speed.
Our study lacks the detailed polar boundary layer dynamics measurements needed to fully evaluate R t , the resistance due to turbulent diffusion in the lowest-altitude legs.However, there are several aspects of the observations that allow us to make a useful limiting estimate using the 19 May 2018 22:30 UTC polar boundary layer leg as the prime example (Fig. 11).First, there were open leads (Fig. S26 in the Supplement) that are associated with polar boundary layer mixing and relatively high mixing heights (Serreze et al., 1992;Moore et al., 2014).Second, the fact that potential temperature is constant with altitude below 300 m implies that the polar boundary layer is well mixed at least as low as the aircraft sampled.Third, there were substantial vertical wind velocities measured by the gust probe aboard the DC-8 aircraft during this polar boundary layer leg, also shown in Fig. S26.All of these features support the assumption that, at least in this instance, turbulent resistance R t is small relative to the resistance due to chemical uptake, at least in the presence of open leads.This is consistent with estimated mixing times of several hours deduced in studies of ozone and mercury in polar boundary layers impacted by open leads (Moore et al., 2014).
Consequently, if chemical uptake is the limiting loss process, we can estimate the liquid-phase loss rate of BrCN (k l ) from Eqs. (1) and (2).The resistance due to chemical reaction is 1/(γ c /4) and the uptake coefficient (γ ) can be estimated from the following equation assuming surface accommodation is efficient (Kolb et al., 1995): where H is the Henry's coefficient, k l is the first-order liquidphase loss rate, D a is the diffusion coefficient of the reactant in solution, and RT represents the gas constant and temperature.Similarly to the analysis of HCN solubility, the parameters needed to estimate k l will need to be extrapolated below 273 K assuming the surfaces are liquid-like layers.In the case of BrCN, we use recent solubility measurements (Roberts and Liu, 2019) and assume H has the same temperature dependence (i.e., same enthalpy of solution) in the liquidlike layer below 273 K. Diffusion coefficients also vary as 1/T , and although there are no measurements of D BrCN , we estimate it as 0.5 × 10 −5 cm 2 s −1 at 263 K by analogy to HCN and the temperature dependence of diffusion coefficients (Tyn and Calus, 1975).Thus, the first-order loss rates of BrCN in solution that correspond to polar boundary layer lifetimes range from 1.2 × 10 −2 s −1 for a lifetime of 1 d to 1.2 × 10 −4 s −1 for a lifetime of 10 d.This range is faster than BrCN hydrolysis, which can be extrapolated to be approximately 1.5 × 10 −5 s −1 at 263 K (Roberts and Liu, 2019).Given that any reactants other than water would be present in micromolar to nanomolar concentrations, this range of firstorder loss rates corresponds to second-order rate constants that are in the range of 10 4 -10 7 M −1 s −1 .The possibility that BrCN could react with halide ions (Cl − , Br − , or I − ) and reform a dihalogen (e.g., XBr) should be considered, as those reactions would serve to propagate Br explosion chemistry.Reactions of BrCN with I − and Br − have been studied in solution (Nolan et al., 1975), and it was found that the rate-limiting step in BrCN + I − , which probably forms IBr, is relatively slow at 0.106 M −1 s −1 at 298 K.The solution-phase reaction eventually formed I − 3 , which would not be favored at typical I − concentrations in polar environments.The reaction of BrCN with Br − was estimated to be quite a bit slower (∼ 10 −8 M −1 s −1 ) based on rate measurements of Br 2 + HCN → BrCN + Br − + H + , and the measured equilibrium constant that was also given (Nolan et al., 1975).(3) We attempted to form Br 2 in a laboratory experiment at room temperature in which saturated NaBr solution was exposed to 150 ppbv of BrCN (see details in the Supplement), and no observable Br 2 resulted (upper limit of 0.1 % of BrCN), consistent with the above estimate that the reaction BrCN + Br − → Br 2 + CN − is quite slow.Although it has not been measured to our knowledge, we can expect the reaction of BrCN with Cl − to be quite slow as well, given established trends of halogen reactions.
The reaction of BrCN with active halogen species, particularly HOCl or HOBr, HOCl(or HOBr) + BrCN → BrCl(or Br 2 ) + HOCN, (R7) might also occur on snow/ice or particle surfaces.While there is no direct evidence for this, the addition of HOCl or Cl 2 to treated water where BrCN was present was observed to accelerate BrCN loss (Heller-Grossman et al., 1999).Such a reaction of HOCl or HOBr, combined with formation reactions discussed above, would lead to no net gain or loss of active halogen to the polar boundary layer.
There are a number of other reactions that BrCN is known to undergo, aside from simple hydrolysis, but none of them generate active Br.BrCN is known to react with R-OH-or R-SH-containing compounds and substituted amines (Siddiqui and Siddiqui, 1980;Kumar, 2005), with the net reaction yielding cyanate, thiocyanate, or nitrile functionalities and the Br ending up either as Br − or as a Br-carbon compound.To our knowledge, the rate constants of these reactions have not been measured but are likely to be reasonably fast given that many of these reactions are used for synthesis or column preparative derivatization (see, for example, March et al., 1974).The key point of emphasis here is that none of these reactions lead to the reformation of an active Br compound.

Conclusions
Two different instruments measured BrCN during the NASA ATom deployments, a CF 3 O − ToF CIMS and an I − ToF CIMS, along with two other active bromine compounds, BrCl and BrO, during NASA ATom deployments 3 and 4 in 2017 and 2018.The ATom-1 and ATom-2 measurements from the CF 3 O − ToF CIMS showed that BrCN was present above the detection limit (3σ of the 10 s precision was 11 pptv) only in the polar boundary layer during the Arctic winter.This Arctic BrCN approached levels as high as 38 pptv and was correlated with high ratios of CHBr 3 to CH 2 Br 2 , a marker for active Br chemistry in the absence of photosynthesis.The elevated BrCN and CHBr 3 have a common origin in the condensed-phase reactions of active bromine (HOBr, Br 2 ) with dissolved organic matter (DOM) and dissolved organic nitrogen (DON).In this late winter environment, there is greatly reduced photosynthetic activity, but Br 2 can be formed from photochemistry in the snowpack (Custard et al., 2017); hence, the relatively tight correlation of BrCN and CHBr 3 /CH 2 Br 2 arises due to the fact that DON is a subset of DOM.
The ATom-3 and ATom-4 measurements revealed elevated mixing ratios (> 3 pptv) of BrCN in both polar boundary layers during both seasons (spring and fall) in October 2017 and late April-May 2018.Mixing ratios of BrCN up to 36 pptv (10 s average) were observed during an MA over BRW airport on 28 April 2018 at Utqiagvik, Alaska.These observations also support the conclusion that least some of the BrCN came from active Br chemistry reactions on snow, ice, and/or particle surfaces, with the -CN group resulting from either HCN/CN − or other reduced nitrogen species from oceanic or cryospheric sources.Surface pH is a somewhat uncertain property of the liquidlike layers that are on the surfaces of aerosol, ice, and frost flowers, and it could also be that during a given O 3 depletion episode the chemistry could evolve to produce BrCN on basic surfaces such as frost flowers and brines or as surface acidity of snow and ice is depleted.We also note that sea ice surfaces are buffered with respect the deposition of acids, so they can remain at the higher pH values characteristic of seawater (Wren and Donaldson, 2012), which will favor BrCN formation chemistry.The higher mixing ratios of BrCN observed at times during polar boundary layer legs make it a potentially important contributor to the active Br cycle.Total inorganic Br values are typically on the order of a few tens of parts per trillion by volume in areas where bromine explosion chemistry is taking place (Simpson et al., 2015).In addition, very short-lived halocarbon species that contain bromine also usually amount to a few tens of parts per trillion by volume of Br, as indicated by bromocarbon mixing ratios reported in this paper.The BrCN concentrations observed in this study were often in the same range as these important Br reservoirs.
BrCN was confined to the polar boundary layer and vertical profiles showed a sharp cut-off at the level of the temperature inversion, strongly implying that BrCN has a short lifetime (1-10 d) in this environment.Given the relatively low aqueous solubility and slow hydrolysis reaction rates of BrCN, these vertical profiles imply that BrCN must undergo more rapid condensed-phase reactions (10 4 -10 7 M −1 s −1 ) that lead to relatively efficient uptake and loss in the polar boundary layer environment.The presence of BrCN indicates a loss of active bromine from the system since known condensed-phase loss mechanisms of BrCN result in either Br − or C-Br bonds.Preliminary laboratory experiments showed that BrCN does not reform active bromine when reacted with solution-phase Br − .Further intensive groundbased observations of BrCN with other active Br compounds and laboratory exploration of BrCN liquid-phase reactions will lead to better characterization of the processes that control halogen-induced O 3 loss in polar regions.

Figure 1 .
Figure 1.The mass spectra of ambient air (1 s average) during sampling in the marine boundary layer near Antarctica during ATom-3 (black) and that of ambient air above the MBL (grey).

2. 4
Additional measurements 2.4.1 NO y , NO x , and O 3 measurements

Figure 2 .
Figure 2. Maps of the BrCN mixing ratios (10 s averages) observed during ATom-3 (a) and ATom-4 (b) colored and sized by mixing ratio, as shown by the adjacent scales.The detection limits for most flights were 1.5 pptv, except for the observations made on 12, 17, and 21 May 2018 that had a higher detection limit (6 pptv) and are shown in grey.

Figure 3 .
Figure 3. Vertical profiles of BrCN mixing ratios (10 s averages) measured during ATom-3 (a) and ATom-4 (b).The colored points correspond to the lowest 4 km of altitude for profiles that encompassed polar boundary layer dips on dates noted when enhanced BrCN was observed, and the grey points show the remaining observations.The ATom-3 flights took place in October 2017 and the ATom-4 flights took place in late April through May 2018.The 11 October 2017 flight took place over the Southern Ocean, the 14 October 2017 and 9 May 2018 flights took place over the Weddell Sea, the 15 May 2018 flight took place over Greenland, and the 15 October 2017 and 19 May 2018 flights took place over the Arctic Ocean.The dot-dashed line shows the limit of detection (LOD) for the flights on 12, 17, and 21 May, and the dashed line shows the LOD for the remainder of the flights.

Figure 4 .
Figure 4.The BrCN observed by the CIT-CIMS during the ATom-2 Arctic flights versus the ratio CHBr 3 /CH 2 Br 2 measured by the UCI-WAS.The CIT-CIMS data were averaged over the UCI-WAS sample collection times.The blue points are from the 18 February 2017 flight from the Azores to Thule, Greenland, and the red circles are from the 19 February 2017 flight from Thule to Anchorage, Alaska.The dashed line is an iterative fit assuming a background in CHBr 3 /CH 2 Br 2 and using ODR.

Figure 5 .
Figure 5. Details of the measurements during the polar boundary layer leg of the 14 October 2017 flight over the Weddell Sea (75.7°S, 50.1°W) centered around 18:20 UTC.The top panel shows the time series for BrCN, BrO, BrCl, HCN, O 3 , and altitude, divided into vertical profiles during the descent (a) and the ascent (b), with a dashed line drawn at 32 ppbv O 3 .

Figure 6 .
Figure 6.Panel (a) shows the map of the 19 May 2018 flight during ATom-4, with the flight path colored and sized by BrCN, and the polar boundary layer legs labeled A-F.Panel (b) shows the time series of measured BrCN, BrCl, and O 3 and the associated altitude and polar boundary layer leg.Panel (c) shows selected halocarbons measured by whole-air sampling during the flight.Profile A was measured at 62.2°N, 83.8°W; profile B was measured at 70.9°N, 89.5°W; profile C was measured at 76.3°N, 96.6°W; profile D was measured at 81.4°N, 110.1°W; profile E was measured at 79.2°N, 130.7°W; profile F was measured at 73.4°N, 137.6°W.

Figure 7 .
Figure 7.The average O 3 vs. the average BrCN measured during the polar boundary layer legs of the 19 May 2018 flight of ATom-4.The bars denote the standard deviation of the means and the labels correspond to the periods shown in Fig. 6b.The linear regression line drawn through the points has an R 2 = 0.94.

Figure 8 .
Figure 8. Details of the measurements during the polar boundary layer legs of the 27 April 2018 flight when the aircraft executed a MA over BRW.Panel (b) shows the time series for BrCN, BrCl, BrO, HCN, O 3 , and altitude, and panel (a) shows the same time series expanded to show the lowest altitudes in more detail.Panel (c) shows the time series of the halocarbons CH 3 Br, CH 3 I, CH 2 Br 2 , and CHBr 3 .The duration of the WAS samples was shorter than the width of the symbols.

Figure 9 .
Figure 9. Vertical profiles over BRW on 27-28 April 2018 for the period between 00:25 and 00:43 UTC.Panel (a) shows the 1 s measurements of BrCN, BCl, and ambient temperature.Panel (b) shows 1 s measurements of HCN and O 3 , and panel (c) shows 1 s measurements of NO y , NO, and potential temperature.

Figure 10 .
Figure 10.The relationships between BrCN (10 s data averaged over the start and stop times of the WAS) and the ratio CHBr 3 /CH 2 Br 2 for the Arctic legs (a) and Antarctic legs (b), with the corresponding dates as noted and the standard deviation of the averages shown as error bars.Note that the 17 May 2018 data show the effects of degraded sensitivity due to the altered IMR humidity used on those flights.

Figure 11 .
Figure 11.The vertical distribution of BrCN (red dots), O 3 (grey), CHBr 3 (green open circles), CH 2 Br 2 (purple triangles), and potential temperature (black) during the low-level leg at 22:30 UTC on 19 May 2018 measured at 73.4°N, 137.6°W.The error bars are the standard deviation of the average altitude traversed during the WAS sampling time.
Instances where substantial BrCN was observed corresponded to other indicators of active Br chemistry: O 3 depletion, elevated CHBr 3 relative to CH 2 Br 2 , https://doi.org/10.5194/acp-24-3421-2024Atmos.Chem.Phys., 24, 3421-3443, 2024 and usually elevated BrO and BrCl mixing ratios.A simple competitive reaction model of the liquid-phase reactions of HOBr/OBr − with HCN/CN − or Cl − /Br − and a box model of Br chemistry both show that BrCN formation can compete with active Br propagation at higher pH values (pH > 6).