1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 Journal of Geophysical Research – Atmospheres Supporting Information for Airborne quantification of upper tropospheric NOx production from lightning in deep convective storms over the United States Great Plains I. B. Pollack1, C. R. Homeyer2, T. B. Ryerson3, K. C. Aikin3,4, J. Peischl3,4, E. C. Apel5, T. Campos5, F. Flocke5, R. S. Hornbrook5, D. J. Knapp5, D. D. Montzka5, A. J. Weinheimer5, D. Riemer6, G. Diskin8, G. Sachse7, T. Mikoviny8, A. Wisthaler9, E. Bruning10, D. MacGorman11, K. A. Cummings12, K. E. Pickering13, H. Huntrieser14, M. Lichtenstern14, H. Schlager14, and M. C. Barth5 1 Atmospheric Science Department, Colorado State University, Fort Collins, CO, USA, 2School of Meteorology, University of Oklahoma, Norman, Oklahoma, USA, 3Cooperative Institute for Research in Environmental Sciences, University of Colorado, Boulder, Colorado, USA, 4Chemical Sciences Division, Earth System Research Laboratory, National Oceanic and Atmospheric Administration, Boulder, Colorado, USA, 5Atmospheric Chemistry Division, National Center for Atmospheric Research, Boulder, CO, USA, 6Rosenstiel School of Marine and Atmopsheric Science, University of Miami, Miami, FL, USA, 7NASA Langley Research Center, Hampton, Virginia, USA, 8Oak Ridge Associated Universities (ORAU), Oak Ridge, TN, USA, 9Institut fuer Ionenphysik und Angewandte Physik, Innsbruck, AUSTRIA, 10Department of Geosciences, Texas Tech University, Lubbock, TX, USA, 11NOAA/OAR National Severe Storms Laboratory, Norman, Oklahoma, USA, 12Department of Atmospheric and Oceanic Science, University of Maryland, College Park, MD, USA, 13Atmospheric Chemistry and Dynamics Laboratory, NASA Goddard Space Flight Center, Greenbelt, MD, USA, 14Institut für Physik der Atmosphäre, Deutsches Zentrum für Luft- und Raumfahrt (DLR), Oberpfaffenhofen, Germany 29 Contents of this file 30 Text S1 to S5 31 Figures S1 to S8 32 Table S1 33 34 35 Introduction This supporting information provides a detailed description of an indicator for when the 36 aircraft were sampling in cloud (S1), a comparison of NO, NO2, CO, and O3 measurements 37 acquired from three different instrumented aircraft during the Deep Convective Clouds and 1 38 Chemistry (DC3) Experiment (S2), exemplary vertical profiles that provide supporting evidence 39 that NOx enhancements due to lightning were measured in the outflow region of DC3 storms (S3, 40 an account of information used from atmospheric soundings (S4), a comparison of results from 41 the flux calculation with and without incorporating storm speed (S5), and details for calculating 42 the sensitivity of P(NOx) to NOx productivity per type of lightning flash (S6). Also included are 43 time series of chemical tracers measured in the outflow (similar to Figure 4 in the paper) and 44 time series of lightning flash counts (similar to Figure 9 in the paper) for each storm considered 45 in the analysis. 46 47 Text S1. 48 Only data points collected when the aircraft are sampling in cloud are retained for further 49 analysis. Here, we follow the work of Ridley et al. [1996] and use increases in ice concentration, 50 which correspond with increases in lightning-produced NO, as an in-situ indicator for in-cloud 51 sampling by the aircraft. Each aircraft was outfitted with one or more in-situ cloud probes 52 during DC3, providing several different data products that can be used to define this cloud 53 indicator. Liquid water content and ice particles ranging from 25 to 800 m encountered by the 54 G-V were measured using a 2D-C cloud probe (Particle Measuring Systems, Inc.); particles 55 ranging from 2 to 50 m (nominally) were also measured with a cloud droplet probe (Droplet 56 Measurement Technologies). Particles up to 47 m (nominally) encountered by the Falcon 57 aircraft were measured using a Forward Scattering Spectrometer Probe (FSSP, Particle 58 Measuring Systems, Inc.). Ice water content and particles ranging from 10 to 3000 m were 59 measured aboard the DC-8 using a 2D-S probe (SPEC Inc.) [Lawson et al., 2006]. However, 60 cloud data products are measured and processed differently among the three aircraft (e.g., 2 61 particle concentrations are processed using the “entire-in” algorithm by Heymsfield and Parrish 62 [1978] for the G-V and according to Lawson et al. [2011] for the DC-8, while a water content 63 parameter from the G-V is calculated using a spherical assumption with the density of water and 64 ice water content from the DC-8 is computed from particle projected areas as described in Baker 65 and Lawson [2006]). Therefore, we use different parameters to define when each aircraft had 66 penetrated the edge of the cloud. For the G-V, we use particle concentration > 1 L-1 from the 2D- 67 C probe, and for the Falcon we use particle concentration > 1 cm-3 from the FSSP. In the 68 absence of 2D-S data for all storms sampled prior to 29 May, a cloud indicator for the DC-8 69 aircraft was synthesized from forward-facing video camera footage; for storms on and after 29 70 May, the DC-8 cloud indicator is defined using a combination of video footage and ice water 71 content > 5 x 10-3 g m-3 (K. Froyd, Personal Communication, 2015). We observe little difference 72 (<2%) in the number of data points retained for further analysis when particle concentration 73 versus ice water content is applied, and thus the choice of cloud parameter for the cloud indicator 74 has little impact on the results of this analysis. Differences in the magnitude of the particle 75 concentrations measured by the different aircraft in a single storm, as shown in figure 3 of the 76 main paper, figure S6, and figure S7, reflect differences in the range of particle sizes that can be 77 detected by each probe and the degree to which each aircraft penetrated the anvil cloud. 78 79 80 Text S2. Intercomparison of airborne trace gas sensors aboard the NASA DC-8 and NSF/NCAR 81 G-V aircraft were performed on several occasions throughout the DC3 deployment (e.g., 25 82 May, 30 May, 01 June, 05 June, and 17 June). Intercomparisons were often conducted within 83 the first hour of flight for a period of 20-30 minutes. The aircraft typically flew in close 3 84 proximity at two altitude levels (e.g., 7 and 12 km), with a coordinated ascent in between, 85 resulting in sufficient variability in measured mixing ratios for correlation analysis. Scatter plots 86 comparing NO, NO2, CO, and O3 measurements from all five DC-8 and G-V intercomparisons 87 are illustrated in Figure S1. The slopes from linear least-squares (LLS) [Press et al.,, 1988] 88 orthogonal distance regression (ODR) [Boggs et al., 1987] of these scatter plots provide a 89 measure of the average percent difference between measurements from the two aircraft, and 90 result in differences of 2% for NO, 28% for NO2, 5% for CO, and < 1% for O3. Except for NO2, 91 all are within the combined uncertainties determined from addition of the individual 92 measurement uncertainties in quadrature. Differences in NO2 may be attributed to corrections 93 for thermal dissociation of methyl peroxy nitrate [Nault et al., 2015], which have been applied to 94 measurements acquired via laser-induced fluorescence aboard the DC-8. 95 Two intercomparisons between the DC-8 and DLR Falcon aircraft were conducted on 11 96 June, with the coordinated portions of the flight performed at 2.1 km and 6.7 km. Scatter plots 97 for CO and O3 are shown in Figure S2. NO and NOx resulted in too little variability for accurate 98 correlation analysis, and are thus shown as a time series in Figure S3. While the average O3 and 99 CO mixing ratios from the DC-8 and Falcon aircraft differ by < 3%, measurements of NO and 100 NOx show less agreement. Larger mixing ratios of NO and NOx by an average of 0.1 and 0.2 101 ppbv were measured by the Falcon aircraft; however, these difference are within the 102 uncertainties and limits of detection reported for these measurements from the Falcon aircraft 103 during the intercomparison flight (e.g., ± 50 pptv uncertainty, and detection limits of 50 pptv for 104 NO and 100 pptv for NOx). Although detection limits for NO and NOx are 20 pptv and 30 pptv, 105 respectively, for all other Falcon flights, detection limits were elevated during the 4 106 intercomparison flight due to excessively high temperatures in the aircraft cabin that caused an 107 unstable zero level in the instrument. 108 Here, we utilize the reported data from all three aircraft as it was archived in the final 109 DC3 data set for this analysis, and assume a total uncertainty of 30% for NOx measured in storms 110 sampled by the G-V and DC-8 (e.g., storms on 18 May, 19 May, 25 May, 29 May 16 June, and 111 22 June), and an overall uncertainty of 55% for NOx measured in storms sampled by the Falcon 112 (e.g., storms on 30 May and 12 June). 113 114 Text S3. 115 Vertical profiles of trace gases measured by the G-V and DC-8 aircraft in the latitude and 116 longitude region of each storm (e.g., the 19 May storm shown in Figure S4) illustrate evidence of 117 enhancements in NOx up to ~4 ppbv between 9 and 13 km m.s.l. due to lightning. These 118 observations are consistent with peak LNOx enhancements ranging between 1 and 19 ppbv 119 reported in previous studies of storms over the U.S. Great Plains [Dye et al., 2000; Luke et al., 120 1992; Ridley et al., 1994; Ridley et al., 1996; Stith et al., 1999]. Large ratios of NOx/NOy and 121 NO/NO2 at high altitudes demonstrate recent production of NO by lightning, while large NOy/O3 122 ratios indicate fresh sources of NO or NOx and photochemically unprocessed air [Ridley et al., 123 1996]. Thus, the observed NOx enhancements in the anvil are best explained by recent 124 production of NO by lightning. O3 enhancements within the cloud largely reflect 125 photochemically processed air and/or mixing with stratospheric air, as shown above for the 19 126 May storm. 127 128 The vertical profiles in Figure S4 also demonstrate vertical transport of chemical tracers from the planetary boundary layer into the upper troposphere by convection. Long-lived, low 5 129 solubility chemical tracers such as CO and CH4, and slightly more soluble tracers like acetone 130 and propanal, which do not have a stratospheric source, act as good indicators for convective 131 transport of anthropogenic species from the planetary boundary layer. Average enhancements in 132 CO, CH4, and (acetone+propanal) measured in the anvil outflow of each storm between 9 and 13 133 km m.s.l. are roughly half of the average enhancements above the free tropospheric background 134 measured in the planetary boundary layer. Therefore, measured NOx enhancements would be 135 much smaller than the mixing ratios observed in the outflow if NOx had been solely transported 136 upward from the boundary layer by convection. 137 138 Text S4. 139 In-situ atmospheric soundings, obtained from radiosondes launched in the vicinity of 140 these storms (e.g., by the NCAR Mobile Integrated Sounding System in the Colorado region and 141 by NOAA’s National Severe Storms Laboratory in the Oklahoma region), provided vertical 142 profiles of temperature, pressure, relative humidity, and winds. Convective available potential 143 energy (CAPE), in units of m2 s-2, is determined for each storm using these parameters, and is 144 employed here as an indicator of the severity of convective activity and the potential strength of 145 each storm [Djuric, 1994; Bluestein, 1993]. The time, location, and CAPE determined from 146 soundings performed during each storm are summarized in Table 1. CAPE for two storms (e.g., 147 one on 18 May and another on 12 June) occurring outside the realm of the in-field sounding 148 network are acquired from the National Weather Service radiosonde network (digested data 149 accessed from http://weather.uwyo.edu/upperair/sounding.html) from 00:00 UTC soundings 150 launched from Amarillo, TX (AMA site) and North Platte, NE (LBF site). A potential maximum 151 updraft velocity for each storm is calculated as 152 1993]. [Price and Rind, 1992; Bluestein, 6 153 154 Text S5. 155 Table S1 compares results for Pflux(NOx) with and without accounting for storm speed, s, 156 in equation (E5). As expected, the percent difference between Pflux(NOx) calculated with a only 157 and Pflux(NOx) calculated with (a -s) scales directly withs. However, since the difference 158 between wind speed and storm motion is directly related to the wind shear, one might question 159 whether the results in Figure 8 of the main paper are due to neglect of storm motion in the flux 160 calculation. Figure S5 shows a scatter plot of the percent difference in Pvol(NOx) and Pflux(NOx) 161 for all storms except 29 May calculated with (a -s) versus the 0-6 km wind shear reported in 162 Table 1 of the main paper. Linear regression of the data points in Figure S5 results in a negative 163 slope similar to that in Figure 8 of the main paper, and suggests that 15% of the variance in the 164 difference between the two methods (r2 = 0.15) can still be attributed to wind shear. 165 166 167 Text S6. The sensitivity of P(NOx) to NOx productivity per type of lightning flash is demonstrated 168 by comparing the effects of assuming IC flashes and CG flashes produce equal amounts of NOx 169 with the possibility that IC flashes could produce ten times less NOx than CG flashes. The 170 percent differences in P(NOx) for each geographical region is calculated according to equation 171 (ES1), and are based on fIC/fCG ratios of 4.9 for Colorado, 4.1 for northern Texas, and 3.9 for 172 Oklahoma [Boccippio et al., 2001]. 173 (ES1) 174 7 175 References 176 Baker, B. A., and R. P. Lawson (2006), Improvement in determination of ice water content from 177 two-dimensional particle imagery: Part I: Image to mass relationships, J. of Appl. Meteor. 178 Climatol., 45(9), 1282-1290. 179 180 181 182 183 Boccippio, D. J., et al. (2001), Regional differences in tropical lightning distributions, J. Appl. Meteorol., 39(12), 2231-2248, doi:10.1175/1520-0450(2001)040<2231:Rditld>2.0.Co;2. Boggs, P. T., et al. (1987), A stable and efficient algorithm for nonlinear orthogonal distance regression, SIAM J. Sci. Comput., 8, 1052-1078. Dye, J. E., et al. (2000), An overview of the Stratospheric-Tropospheric Experiment: Radiation, 184 Aerosols, and Ozone (STERAO)-Deep Convection experiment with results for the July 185 10, 1996 storm, J. Geophys. Res-Atmos., 105(D8), 10023-10045, 186 doi:10.1029/1999jd901116. 187 Heymsfield, A. J., Parrish, J. L. (1978), A Computational Technique for Increasing the Effective 188 Sampling Volume of the PMS Two-Dimensional Particle Size Spectrometer, J. Appl. 189 Meteor., 17, 1566-1572. 190 Lawson, R. P. et al. (2006), The 2D-S (stereo) probe: Design and preliminary tests of a new 191 airborne, high speed, high resolution particle imaging probe, J. Atmos. Oceanic Technol., 192 23, 1462-1477, doi:10.1175/JTECH1927.1. 193 194 195 196 Lawson, R. P. (2011), Effects of ice particles shattering on the 2D-S probe, Atmos. Meas. Tech., 4, 1361-1381, doi:10.5194/amt-4-1361-2011. Luke, W. T., et al., (1992), Tropospheric chemistry over the lower Great Plains of the United States, 2, Trace gas profiles and distributions, J. Geophys. Res., 97, 20647-20670. 8 197 198 Nault, B. A., et al. (2015), Measurements of CH3O2NO2 in the upper troposphere, Atmos. Meas. Tech., 8, 987-997, doi:10.5194/amt-8-987-2015. 199 Press, W. H., et al. (1988), Numerical recipes in C, Cambridge University Press, Cambridge. 200 Ridley, B. A., et al. (1994), Distributions of NO, NOx, NOy, and O-3 to 12-Km altitude during 201 the summer monsoon season over New-Mexico, J. Geophys. Res-Atmos., 99(D12), 202 25519-25534, doi:10.1029/94jd02210. 203 204 205 206 207 208 Ridley, B. A., et al. (1996), On the production of active nitrogen by thunderstorms over New Mexico, J. Geophys. Res-Atmos., 101(D15), 20985-21005, doi:10.1029/96jd01706. Stith, J., et al. (1999), NO signatures from lightning flashes, J. Geophys. Res-Atmos., 104(D13), 16081-16089, doi:10.1029/1999jd900174. Taylor, J. R. (1997), An introduction to error analysis: the study of uncertainties in physical measurements 2nd ed., University Science Books, Sausalito. 9 Figure S1. Scatter plots of NO, NO2, CO, and O3 measurements from the DC-8 and G-V aircraft. Data points represent measurements from all five intercomparisons between these two aircraft; results of LLS correlation analysis (solid black lines) are reported in the text boxes. 10 Figure S2. Same as Figure S1 for intercomparison of measurements from the DC-8 and Falcon aircraft. 11 Figure S3. Time series of CO, O3, NO, and NOx, measurements from a 20-minute intercomparison at 2.1 km (a) and a 12-minute intercomparison at 6.7 km (b) between the DC-8 and Falcon aircraft on 11 June. 12 Figure S4. Vertical profiles of NOx (black for DC-8, gray for G-V), CO (red for DC-8, pink for G-V), O3 (blue for DC-8, cyan for G-V), select hydrocarbons (green/purple), and ratios of NOx/NOy (black), NOy/O3 (blue), and NO/NO2 (red for DC-8 and pink for G-V) sampled by the aircraft in the spatial region of the 19 May storm. Shaded areas represent the vertical extent of the anvil. 13 % difference in P(NOx) (volume-flux) 100 80 60 40 20 0 0 10 20 30 -1 Shear (m s ) Figure S5. Same as Figure 8 in the main paper except the percent difference in P(NOx) is calculated using Pflux(NOx) (a - s) from Table S1. 14 Figure S6. Same as Figure 3 in the paper for the remaining storms in the Oklahoma region. 15 Figure S7. Same as Figure 3 in the paper, but for storms in the Colorado region. 16 Figure S8. Same as Figure 6 in the paper, but for storms in the Colorado region. 17 Table S1. Results of the flux calculations, in units of moles flash-1, with and without subtracting the storm velocity, vs, from the measured wind speed, va. The reported percent difference refers to the difference in Pflux(NOx), va - vs and Pflux(NOx), va and scales directly with vs. Date vs (m s-1) Pflux(NOx), va - vs Pflux(NOx), va % diff 19 May 8 265 ± 79 407 ± 131 35 25 May 17 45 ± 10 84 ± 19 46 29 May 10 110 ± 15 141 ± 19 22 16 June 2 192 ± 33 205 ± 36 6 18 May 11 50 ± 9 73 ± 12 32 22 June 15 67 ± 7 131 ± 15 49 18