List of <strong>Abstracts</strong> 175P-Observations 2.21 ID:4514 10:30The Use of Satellite based GOME and SCIAMACHY data to Study the Tropospheric Ozone amountover the TropicsAnnette Ladstaetter-Weissenmayer, Stefan Boetel, Christian V. Savigny, Mark Weber, Sergji Puzankov, JohnP. BurrowsUniversity of Bremen, GermanyContact: lad@iup.physik.uni-bremen.deThe Global Ozone Monitoring Experiment (GOME) launched in April 1995 is measuring the sunlight backscattered by the surface in nadir viewing mode (240-790 nm) to detect O3, NO2, BrO, OClO, HCHO andSO2. SCIAMACHY (Scanning Imaging Absorption Spectrometer for Atmospheric ChartographY) launchedin March 2002 is measuring sunlight, transmitted, reflected and scattered by the earth atmosphere or surface(240 nm - 2380 nm). SCIAMACHY measurements yield the amounts and distribution of O3, BrO, OClO,ClO, SO2, H2CO, NO2, CO, CO2, CH4, H2O, N2O, p, T, aerosol, radiation, cloud cover and cloud topheight in limb and nadir mode. Over the tropics e.g. biomass burning is extensive. During these burningevents large amounts of aerosols and trace gases like nitrogen oxide NOx, hydrocarbons, formaldehyde(HCHO) and carbon monoxide (CO) are emitted into the troposphere. In photochemical reactionstropospheric O3 is produced. GOME- and SCIAMACHY-data were analysed to observe an increasing ofthis trace gas during the fire event and to compare then these results with the data of a “non-burning-season”to calculate the additional impact.P-Observations 2.22 ID:4213 10:30The Bihar Pollution Pool as observed from MOPITT (version 4 data), CALIPSO and troposphericozone residual dataJayanta Kar 1 , Merritt Deeter 2 , Jack Fishman 3 , Zhaoyan Liu 3 , John Creilson 3 , Ali Omar 3 , CharlesTrepte 3 , David Winker 31 Science Systems and Applications Inc., Hampton, VA, USA2 National Center for Atmospheric Research, Boulder, CO, USA3 NASA Langley Research Center, Hampton, VA, USAContact: jayanta.kar@nasa.govThe Bihar pollution pool covers an extensive region in the eastern parts of the Indo-Gangetic basin and ismost intense during winter. We use recently improved (version 4) retrievals of carbon monoxide (CO) fromthe MOPITT observations along with the aerosol data from the latest version of the CALIPSO lidarinstrument to provide new insight into the vertical structure of this pollution. In addition, the troposphericozone residual products from the TOMS/SBUV and OMI/MLS database are examined to characterize thispollution pool. The feature is seen primarily in the lower troposphere from about November to February withstrong concomitant increase in the CO, aerosol and ozone tropospheric columns. The height resolved aerosoldata from CALIPSO confirm the trapping of the pollution pool at the lowest altitudes. The CALIPSOsubtype data indicate polluted dust to be the dominant aerosol type. In winter the dust is probably of localorigin. The observations suggest that MOPITT can capture this low altitude phenomenon even in winterconditions as indicated by the averaging kernels. The simultaneous observations of the feature in both thetropospheric ozone column products suggest photochemical production of ozone from the enhancedprecursor abundances at low altitudes.iCACGP-<strong>IGAC</strong> 2010 14 July, 2010
List of <strong>Abstracts</strong> 176P-Observations 2.23 ID:4259 10:30Effects of regional pollution and long range transport on the lower tropospheric ozone over an urbansite in western IndiaShuchita Srivastava 1 , Shyam Lal 1 , Manish Naja 2 , S. Venkataramani 1 , T.A. Rajesh 11 Physical Research Laboratory, Ahmedabad, India2 Aryabhatta Research Institute of Observational Sciences, Nainital, IndiaContact: shuchita@prl.res.inThe balloon borne measurements of vertical distribution of ozone and meteorological parameters were madefortnightly from April 2003 to July 2007 at Physical Research Laboratory, Ahmedabad (23.03º N, 72.54º E,49m amsl). The seasonal distributions of ozone are investigated for the boundary layer (1-2 km) and lowertroposphere (2.5 to 4 km) using back-trajectory analysis. Three geographical sectors are defined for theregional pollution, marine region and long range transport, and residence time of trajectories for balloonflight days are estimated. These residence times are tagged with the corresponding ozone mixing ratios. Theozone levels increase with increasing residence time till 4-6 days for all seasons except winter in the regionalsector. The significant ozone build up is absent during winter probably due to high levels of local pollutants.The slope of ozone vs residence time is extrapolated to zeroth day to get the “background ozone mixingratio”. The average background ozone mixing ratios are found to be about 28 ppbv for boundary layer and42 ppbv for the free troposphere. The background ozone mixing ratio is comparable to average ozone mixingratio during summer-monsoon season in the boundary layer. The seasonal variation of ozone shows higherozone levels during late autumn, winter and early spring (> 50 ppbv) and minimum during summer-monsoon(~30 ppbv) in the boundary layer. The higher ozone levels during late autumn, winter and spring seasons aredominated by regionally polluted airmass whereas poor ozone levels during summer-monsoon are influencedby marine airmass. In the lower troposphere, seasonal variation of ozone is found to be affected by regionalpollution and long range transport. Detailed results will be presented.P-Observations 2.24 ID:4578 10:30High-resolution tropospheric ozone fields for INTEX and ARCTAS from IONS ozonesondesDavid Tarasick 1 , Jinjian Jin 2 , Vitali Fioletov 3 , Guiping Liu 3 , Anne Thompson 4 , Samuel Oltmans 5 ,Christopher Sioris 3 , Xiong Liu 6 , Owen Cooper 7 , Tom Dann 3 , Jingxian Liu 31 Department of Meteorology, 510 Walker Building, Pennsylvania State University2 Jet Propulsion Laboratory, California Institute of Technology3 Environment Canada4 Department of Meteorology, Pennsylvania State University5 NOAA Climate Monitoring and Diagnostics Laboratory6 Goddard Earth Sciences and Technology Center, University of Maryland7 Cooperative Institute for Research in Environmental Sciences, University of ColoradoContact: david.tarasick@ec.gc.caThe IONS-04, IONS-06 and ARC-IONS ozone sounding campaigns over North America in 2004, 2006 and2008 obtained approximately 1400 profiles, in five series of coordinated and closely-spaced (typically daily)launches. Although this coverage is unprecedented, it is still somewhat sparse in its geographical spacing.<strong>Here</strong> we use forward and back- trajectory calculations for each sounding to map ozone measurements to anumber of other locations, and so to fill in the spatial domain. This is possible because the lifetime of ozonein the troposphere is of the order of weeks. The trajectory-mapped ozone values show reasonable correlationwith estimates from OMI and, where they overlap, to each other. Further validation with MOZAIC profilesand surface station data will be presented. A variable-length smoothing algorithm is used to fill data gaps.The total tropospheric ozone column maps calculated by integrating the smoothed fields agree well withsimilar maps derived from TOMS and OMI/MLS measurements. The resulting three-dimensional picture ofiCACGP-<strong>IGAC</strong> 2010 14 July, 2010
- Page 2 and 3:
List of Abstracts 1Plenary.1 ID:459
- Page 4 and 5:
List of Abstracts 3Chemistry-Climat
- Page 6 and 7:
List of Abstracts 5Chemistry-Climat
- Page 8 and 9:
List of Abstracts 7correlations are
- Page 10 and 11:
List of Abstracts 9P-Sources.2 ID:4
- Page 12 and 13:
List of Abstracts 11P-Sources.6 ID:
- Page 14 and 15:
List of Abstracts 13calculation of
- Page 16 and 17:
List of Abstracts 15P-Sources.13 ID
- Page 18 and 19:
List of Abstracts 17emissions made
- Page 20 and 21:
List of Abstracts 19modeling techni
- Page 22 and 23:
List of Abstracts 21than true uncer
- Page 24 and 25:
List of Abstracts 23affect regions
- Page 26 and 27:
List of Abstracts 25P-Sources.31 ID
- Page 28 and 29:
List of Abstracts 27An inverse mode
- Page 30 and 31:
List of Abstracts 29transport of CO
- Page 32 and 33:
List of Abstracts 31in the levels o
- Page 34 and 35:
List of Abstracts 33P-Sources.46 ID
- Page 36 and 37:
List of Abstracts 35Reductions in b
- Page 38 and 39:
List of Abstracts 37P-Sources.53 ID
- Page 40 and 41:
List of Abstracts 39includes emissi
- Page 42 and 43:
List of Abstracts 41will be present
- Page 44 and 45:
List of Abstracts 43parameterizatio
- Page 46 and 47:
List of Abstracts 45measurements an
- Page 48 and 49:
List of Abstracts 47Multiphase halo
- Page 50 and 51:
List of Abstracts 49be explained by
- Page 52 and 53:
List of Abstracts 51Contact: tzhu@p
- Page 54 and 55:
List of Abstracts 53particle-resolv
- Page 56 and 57:
List of Abstracts 551 University of
- Page 58 and 59:
List of Abstracts 57Contact: visahi
- Page 60 and 61:
List of Abstracts 59Weather and cli
- Page 62 and 63:
List of Abstracts 61on the global M
- Page 64 and 65:
List of Abstracts 63will be compare
- Page 66 and 67:
List of Abstracts 65P-Chemistry Cli
- Page 68 and 69:
List of Abstracts 67P-Chemistry Cli
- Page 70 and 71:
List of Abstracts 69have included s
- Page 72 and 73:
List of Abstracts 71Contact: bumiya
- Page 74 and 75:
List of Abstracts 73particle, chang
- Page 76 and 77:
List of Abstracts 75P-Chemistry Cli
- Page 78 and 79:
List of Abstracts 77of the rain bel
- Page 80 and 81:
List of Abstracts 79Community Atmos
- Page 82 and 83:
List of Abstracts 81climate conditi
- Page 84 and 85:
List of Abstracts 835 IMK, Karlsruh
- Page 86 and 87:
List of Abstracts 85P-Observations
- Page 88 and 89:
List of Abstracts 87P-Observations
- Page 90 and 91:
List of Abstracts 89We have previou
- Page 92 and 93:
List of Abstracts 91particles, from
- Page 94 and 95:
List of Abstracts 933 Department of
- Page 96 and 97:
List of Abstracts 95also from agric
- Page 98 and 99:
List of Abstracts 97P-Observations
- Page 100 and 101:
List of Abstracts 99P-Observations
- Page 102 and 103:
List of Abstracts 101(WMO, Geneva),
- Page 104 and 105:
List of Abstracts 103START-08 campa
- Page 106 and 107:
List of Abstracts 105frequency of t
- Page 108 and 109:
List of Abstracts 107Observations 2
- Page 110 and 111:
List of Abstracts 109Interfaces 1.1
- Page 112 and 113:
List of Abstracts 1111 Met Office H
- Page 114 and 115:
List of Abstracts 113year are almos
- Page 116 and 117:
List of Abstracts 115transport mode
- Page 118 and 119:
List of Abstracts 117of carbon mono
- Page 120 and 121:
List of Abstracts 119Plenary 3 ID:4
- Page 122 and 123:
List of Abstracts 121In this study,
- Page 124 and 125:
List of Abstracts 123both microphys
- Page 126 and 127: List of Abstracts 1251 University o
- Page 128 and 129: List of Abstracts 127humidities bet
- Page 130 and 131: List of Abstracts 129Contact: jerem
- Page 132 and 133: List of Abstracts 131developed at N
- Page 134 and 135: List of Abstracts 133P-Transformati
- Page 136 and 137: List of Abstracts 135We will presen
- Page 138 and 139: List of Abstracts 137airborne data
- Page 140 and 141: List of Abstracts 139P-Transformati
- Page 142 and 143: List of Abstracts 141on the identif
- Page 144 and 145: List of Abstracts 143P-Transformati
- Page 146 and 147: List of Abstracts 145P-Transformati
- Page 148 and 149: List of Abstracts 147hydrometeors a
- Page 150 and 151: List of Abstracts 149intercompariso
- Page 152 and 153: List of Abstracts 151P-Transformati
- Page 154 and 155: List of Abstracts 153P-Transformati
- Page 156 and 157: List of Abstracts 155radicals are t
- Page 158 and 159: List of Abstracts 157of the kinetic
- Page 160 and 161: List of Abstracts 159+ i-butanol) =
- Page 162 and 163: List of Abstracts 161km) covering t
- Page 164 and 165: List of Abstracts 163P-Observations
- Page 166 and 167: List of Abstracts 165number of gase
- Page 168 and 169: List of Abstracts 167the highest va
- Page 170 and 171: List of Abstracts 169range transpor
- Page 172 and 173: List of Abstracts 171P-Observations
- Page 174 and 175: List of Abstracts 173quality proble
- Page 178 and 179: List of Abstracts 177the tropospher
- Page 180 and 181: List of Abstracts 179masses and eva
- Page 182 and 183: List of Abstracts 181P-Observations
- Page 184 and 185: List of Abstracts 183P-Observations
- Page 186 and 187: List of Abstracts 185P-Observations
- Page 188 and 189: List of Abstracts 187OMI also measu
- Page 190 and 191: List of Abstracts 189seasonal varia
- Page 192 and 193: List of Abstracts 191P-Observations
- Page 194 and 195: List of Abstracts 193climate.P-Obse
- Page 196 and 197: List of Abstracts 195aerosols and c
- Page 198 and 199: List of Abstracts 197Health Organiz
- Page 200 and 201: List of Abstracts 199December 2008-
- Page 202 and 203: List of Abstracts 201P-Observations
- Page 204 and 205: List of Abstracts 203Contact: anls@
- Page 206 and 207: List of Abstracts 205P-Observations
- Page 208 and 209: List of Abstracts 207Temuco is a fa
- Page 210 and 211: List of Abstracts 209context of Cen
- Page 212 and 213: List of Abstracts 211P-Observations
- Page 214 and 215: List of Abstracts 213addition to th
- Page 216 and 217: List of Abstracts 215Ca, Cd, Cu, Fe
- Page 218 and 219: List of Abstracts 217for the MBL co
- Page 220 and 221: List of Abstracts 219and particulat
- Page 222 and 223: List of Abstracts 2213 Princeton Un
- Page 224 and 225: List of Abstracts 223Robinson, A.L.
- Page 226 and 227:
List of Abstracts 225Observations 4
- Page 228 and 229:
List of Abstracts 227minor contribu
- Page 230 and 231:
List of Abstracts 229linked to know
- Page 232 and 233:
List of Abstracts 231identified pse
- Page 234 and 235:
List of Abstracts 233Wake-up 1.1 ID
- Page 236 and 237:
List of Abstracts 235Wake-up 2.1 ID
- Page 238 and 239:
List of Authors 237Beck, Veronica .
- Page 240 and 241:
List of Authors 239Dann, Tom.......
- Page 242 and 243:
List of Authors 241Gioda, Adriana .
- Page 244 and 245:
List of Authors 243Keating, Terry .
- Page 246 and 247:
List of Authors 245Mao, Jingqiu....
- Page 248 and 249:
List of Authors 247Perri, Mark.....
- Page 250 and 251:
List of Authors 249Shank, Lindsey .
- Page 252 and 253:
List of Authors 251Van Donkelaar, A