<?xml version="1.0" encoding="utf-8"?><rss version="2.0"><channel><title>ACPD - Latest Articles</title><link>http://www.atmos-chem-phys-discuss.net/</link><description>Atmospheric Chemistry and Physics Discussions Latest Articles</description><language>en</language><item><title>Atmospheric histories and growth trends of C&lt;sub&gt;4&lt;/sub&gt;F&lt;sub&gt;10&lt;/sub&gt;, C&lt;sub&gt;5&lt;/sub&gt;F&lt;sub&gt;12&lt;/sub&gt;, C&lt;sub&gt;6&lt;/sub&gt;F&lt;sub&gt;14&lt;/sub&gt;, C&lt;sub&gt;7&lt;/sub&gt;F&lt;sub&gt;16&lt;/sub&gt; and C&lt;sub&gt;8&lt;/sub&gt;F&lt;sub&gt;18&lt;/sub&gt;</title><link>http://www.atmos-chem-phys-discuss.net/12/4165/2012/</link><description>&lt;b&gt;Atmospheric histories and growth trends of C&lt;sub&gt;4&lt;/sub&gt;F&lt;sub&gt;10&lt;/sub&gt;, C&lt;sub&gt;5&lt;/sub&gt;F&lt;sub&gt;12&lt;/sub&gt;, C&lt;sub&gt;6&lt;/sub&gt;F&lt;sub&gt;14&lt;/sub&gt;, C&lt;sub&gt;7&lt;/sub&gt;F&lt;sub&gt;16&lt;/sub&gt; and C&lt;sub&gt;8&lt;/sub&gt;F&lt;sub&gt;18&lt;/sub&gt;&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Chemistry and Physics Discussions, 12, 4165-4184, 2012&lt;br /&gt;&lt;br /&gt;Author(s): D. J. Ivy, T. Arnold, C. M. Harth, L. P. Steele, J. Mühle, M. Rigby, P. K. Salameh, M. Leist, P. B. Krummel, P. J. Fraser, R. F. Weiss, and R. G. Prinn&lt;br /&gt;&lt;br /&gt;The first atmospheric observations and trends are presented
      for the high molecular weight perfluorocarbons (PFCs):
      decafluorobutane (C&lt;sub&gt;4&lt;/sub&gt;F&lt;sub&gt;10&lt;/sub&gt;), dodecafluoropentane
      (C&lt;sub&gt;5&lt;/sub&gt;F&lt;sub&gt;12&lt;/sub&gt;), tetradecafluorohexane (C&lt;sub&gt;6&lt;/sub&gt;F&lt;sub&gt;14&lt;/sub&gt;),
      hexadecafluoroheptane (C&lt;sub&gt;7&lt;/sub&gt;F&lt;sub&gt;16&lt;/sub&gt;) and
      octadecafluorooctane (C&lt;sub&gt;8&lt;/sub&gt;F&lt;sub&gt;18&lt;/sub&gt;). Their atmospheric
      histories are based on measurements of 38 Northern Hemisphere
      and 46 Southern Hemisphere archived air samples collected
      between 1973 to 2011 using the Advanced Global Atmospheric
      Gases Experiment (AGAGE) &quot;Medusa&quot; preconcentration gas
      chromatography-mass spectrometry systems. A new calibration
      scale was prepared for each PFC, with estimated accuracies of
      6.8% for C&lt;sub&gt;4&lt;/sub&gt;F&lt;sub&gt;10&lt;/sub&gt;, 7.8% for
      C&lt;sub&gt;5&lt;/sub&gt;F&lt;sub&gt;12&lt;/sub&gt;, 4.0% for C&lt;sub&gt;6&lt;/sub&gt;F&lt;sub&gt;14&lt;/sub&gt;, 6.6%
      for C&lt;sub&gt;7&lt;/sub&gt;F&lt;sub&gt;16&lt;/sub&gt; and 7.9% for C&lt;sub&gt;8&lt;/sub&gt;F&lt;sub&gt;18&lt;/sub&gt;. Based
      on our observations the 2011 globally averaged dry air mole
      fractions of these heavy PFCs are: 0.18 parts-per-trillion
      (ppt, i.e., parts per 10&lt;sup&gt;12&lt;/sup&gt;) for C&lt;sub&gt;4&lt;/sub&gt;F&lt;sub&gt;10&lt;/sub&gt;, 0.12
      ppt for C&lt;sub&gt;5&lt;/sub&gt;F&lt;sub&gt;12&lt;/sub&gt;, 0.28 ppt for C&lt;sub&gt;6&lt;/sub&gt;F&lt;sub&gt;14&lt;/sub&gt;, 0.12
      ppt for C&lt;sub&gt;7&lt;/sub&gt;F&lt;sub&gt;16&lt;/sub&gt; and 0.09 ppt for
      C&lt;sub&gt;8&lt;/sub&gt;F&lt;sub&gt;18&lt;/sub&gt;. These atmospheric mole fractions combine to
      contribute to a global average radiative forcing of
      0.35 mW m&lt;sup&gt;−2&lt;/sup&gt;, which is 3.6% of the total PFC
      radiative forcing. The globally averaged mean atmospheric
      growth rates of these PFCs during 1973–2011 are 4.58 parts
      per quadrillion (ppq, i.e., parts per 10&lt;sup&gt;15&lt;/sup&gt;) per year (yr)
      for C&lt;sub&gt;4&lt;/sub&gt;F&lt;sub&gt;10&lt;/sub&gt;, 3.29 ppq yr&lt;sup&gt;−1&lt;/sup&gt; for
      C&lt;sub&gt;5&lt;/sub&gt;F&lt;sub&gt;12&lt;/sub&gt;, 7.50 ppq yr&lt;sup&gt;−1&lt;/sup&gt; for C&lt;sub&gt;6&lt;/sub&gt;F&lt;sub&gt;14&lt;/sub&gt;,
      3.19 ppq yr&lt;sup&gt;−1&lt;/sup&gt; for C&lt;sub&gt;7&lt;/sub&gt;F&lt;sub&gt;16&lt;/sub&gt; and
      2.51 ppq yr&lt;sup&gt;−1&lt;/sup&gt; for C&lt;sub&gt;8&lt;/sub&gt;F&lt;sub&gt;18&lt;/sub&gt;. The growth rates of
      the heavy perfluorocarbons were largest in the early 1990s for
      C&lt;sub&gt;4&lt;/sub&gt;F&lt;sub&gt;10&lt;/sub&gt; and C&lt;sub&gt;5&lt;/sub&gt;F&lt;sub&gt;12&lt;/sub&gt; and in the mid-to-late
      1990s for C&lt;sub&gt;6&lt;/sub&gt;F&lt;sub&gt;14&lt;/sub&gt;, C&lt;sub&gt;7&lt;/sub&gt;F&lt;sub&gt;16&lt;/sub&gt; and
      C&lt;sub&gt;8&lt;/sub&gt;F&lt;sub&gt;18&lt;/sub&gt;. The more recent slow down in the growth
      rates of the high molecular weight PFCs suggests that
      emissions are declining as compared to the 1980s and
      1990s. Nevertheless continued monitoring of these potent,
      extremely long-lived greenhouse gases is necessary to verify
      that global PFC emissions continue to decline.</description><pubDate>Fri, 03 Feb 2012 00:00:00 +0100</pubDate></item><item><title>Central Arctic atmospheric summer conditions during the Arctic Summer Cloud  Ocean Study (ASCOS): contrasting to previous expeditions</title><link>http://www.atmos-chem-phys-discuss.net/12/4101/2012/</link><description>&lt;b&gt;Central Arctic atmospheric summer conditions during the Arctic Summer Cloud  Ocean Study (ASCOS): contrasting to previous expeditions&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Chemistry and Physics Discussions, 12, 4101-4164, 2012&lt;br /&gt;&lt;br /&gt;Author(s): M. Tjernström, C. E. Birch, I. M. Brooks, M. D. Shupe, P. O. G. Persson, J. Sedlar, T. Mauritsen, C. Leck, J. Paatero, M. Szczodrak, and C. R. Wheeler&lt;br /&gt;&lt;br /&gt;Understanding the rapidly changing climate in the Arctic is limited by
      a lack of understanding of underlying strong feedback mechanisms that
      are specific to the Arctic. Progress in this field can only be
      obtained by process-level observations; this is the motivation for
      intensive ice-breaker-based campaigns such as that described in this
      paper: the Arctic Summer Cloud-Ocean Study (ASCOS). However, detailed field observations also have to be put in the context of the larger-scale
      meteorology, and short field campaigns have to be analysed within the
      context of the underlying climate state and temporal anomalies from
      this.
&lt;br&gt;&lt;/br&gt;
      To aid in the analysis of other parameters or processes observed
      during this campaign, this paper provides an overview of the
      synoptic-scale meteorology and its climatic anomaly during the ASCOS
      field deployment. It also provides a statistical analysis of key
      features during the campaign, such as some key meteorological
      variables, the vertical structure of the lower troposphere and clouds,
      and energy fluxes at the surface. In order to assess the
      representativity of the ASCOS results, we also compare these features
      to similar observations obtained during three earlier summer
      experiments in the Arctic Ocean, the AOE-96, SHEBA and AOE-2001
      expeditions.
&lt;br&gt;&lt;/br&gt;
      We find that these expeditions share many key features of the
      summertime lower troposphere. Taking ASCOS and the previous
      expeditions together, a common picture emerges with a large
      amount of low-level cloud in a well-mixed shallow boundary layer,
      capped by a weak to moderately strong inversion where moisture, and
      sometimes also cloud top, penetrate into the lower parts of the
      inversion. Much of the boundary-layer mixing is due to cloud-top
      cooling and subsequent buoyant overturning of the cloud. The cloud
      layer may, or may not, be connected with surface processes depending
      on the depths of the cloud and surface-based boundary layers and on
      the relative strengths of surface-shear and cloud-buoyancy turbulence
      generation. The latter also implies a connection between the cloud
      layer and the free troposphere through entrainment at cloud top.</description><pubDate>Fri, 03 Feb 2012 00:00:00 +0100</pubDate></item><item><title>Distributions, long term trends and emissions of four perfluorocarbons  in remote parts of the atmosphere and firn air</title><link>http://www.atmos-chem-phys-discuss.net/12/4073/2012/</link><description>&lt;b&gt;Distributions, long term trends and emissions of four perfluorocarbons  in remote parts of the atmosphere and firn air&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Chemistry and Physics Discussions, 12, 4073-4100, 2012&lt;br /&gt;&lt;br /&gt;Author(s): J. C. Laube, C. Hogan, M. J. Newland, F. S. Mani, P. J. Fraser, C. A. M. Brenninkmeijer, P. Martinerie, D. E. Oram, T. Röckmann, J. Schwander, E. Witrant, G. P. Mills, C. E. Reeves, and W. T. Sturges&lt;br /&gt;&lt;br /&gt;We report the first data set of atmospheric abundances for the
      following four perfluoroalkanes: &lt;i&gt;n&lt;/i&gt;-decafluorobutane
      (&lt;i&gt;n&lt;/i&gt;-C&lt;sub&gt;4&lt;/sub&gt;F&lt;sub&gt;10&lt;/sub&gt;), &lt;i&gt;n&lt;/i&gt;-dodecafluoropentane
      (&lt;i&gt;n&lt;/i&gt;-C&lt;sub&gt;5&lt;/sub&gt;F&lt;sub&gt;12&lt;/sub&gt;), &lt;i&gt;n&lt;/i&gt;-tetradecafluorohexane
      (&lt;i&gt;n&lt;/i&gt;-C&lt;sub&gt;6&lt;/sub&gt;F&lt;sub&gt;14&lt;/sub&gt;) and &lt;i&gt;n&lt;/i&gt;-hexadecafluoroheptane
      (&lt;i&gt;n&lt;/i&gt;-C&lt;sub&gt;7&lt;/sub&gt;F&lt;sub&gt;16&lt;/sub&gt;). All four compounds could be detected
      and quantified in air samples from remote locations in the Southern
      Hemisphere (at Cape Grim, Tasmania, archived samples dating back to
      1978) and the upper troposphere (a passenger aircraft flying from
      Germany to South Africa). Further observations originate from air
      samples extracted from deep firn in Greenland and allow trends of
      atmospheric abundances in the earlier 20th century to be inferred. All
      four compounds were not present in the atmosphere prior to the
      1960s. &lt;i&gt;n&lt;/i&gt;-C&lt;sub&gt;4&lt;/sub&gt;F&lt;sub&gt;10&lt;/sub&gt; and &lt;i&gt;n&lt;/i&gt;-C&lt;sub&gt;5&lt;/sub&gt;F&lt;sub&gt;12&lt;/sub&gt;
      were also measured in samples collected in the stratosphere confirming
      their very long atmospheric lifetimes. Emissions were inferred from
      these observations and found to be comparable with emissions from the
      EDGAR database for &lt;i&gt;n&lt;/i&gt;-C&lt;sub&gt;6&lt;/sub&gt;F&lt;sub&gt;14&lt;/sub&gt;. However, emissions
      of &lt;i&gt;n&lt;/i&gt;-C&lt;sub&gt;4&lt;/sub&gt;F&lt;sub&gt;10&lt;/sub&gt;, &lt;i&gt;n&lt;/i&gt;-C&lt;sub&gt;5&lt;/sub&gt;F&lt;sub&gt;12&lt;/sub&gt; and
      &lt;i&gt;n&lt;/i&gt;-C&lt;sub&gt;7&lt;/sub&gt;F&lt;sub&gt;16&lt;/sub&gt; were found to differ by up to five
      orders of magnitude. Although the abundances of the four
      perfluorocarbons reported here are currently small (less than
      0.3 ppt, parts per trillion) they have
      strong Global Warming Potentials several thousand times higher than
      carbon dioxide and continue to increase in the atmosphere. The sum of
      their cumulative emissions reached 325 mt (million metric tonnes)
      CO&lt;sub&gt;2&lt;/sub&gt; equivalent at the end of
      2009.</description><pubDate>Fri, 03 Feb 2012 00:00:00 +0100</pubDate></item><item><title>Retrieval of aerosol optical depth over land based on a time series technique using MSG/SERIVI data</title><link>http://www.atmos-chem-phys-discuss.net/12/4031/2012/</link><description>&lt;b&gt;Retrieval of aerosol optical depth over land based on a time series technique using MSG/SERIVI data&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Chemistry and Physics Discussions, 12, 4031-4071, 2012&lt;br /&gt;&lt;br /&gt;Author(s): L. Mei, Y. Xue, G. de Leeuw, T. Holzer-Popp, J. Guang, Y. Li, L. Yang, H. Xu, X. Xu, C. Li, Y. Wang, C. Wu, T. Hou, X. He, J. Liu, J. Dong, and Z. Chen&lt;br /&gt;&lt;br /&gt;A novel approach for the joint retrieval of aerosol optical depth (AOD) and
surface reflectance, using Meteosat Second Generation – Spinning Enhanced
Visible and Infrared Imagers (MSG/SEVIRI) observations in two solar
channels, is presented. The retrieval is based on a time series (TS)
technique, which makes use of the two visible bands at 0.6 μm and
0.8 μm in three orderly scan times (15 min interval between two scans)
to retrieve the AOD over land. Using the radiative transfer equation for
plane-parallel atmospheres two coupled differential equations for the upward
and downward fluxes are derived. The boundary conditions for the upward and
downward fluxes at the top and at the bottom of the atmosphere are used in
these equations to provide an analytic solution for the surface reflectance.
To derive these fluxes, the aerosol single scattering albedo (SSA)  and asymmetry
factor are required to provide a solution. These are provided from a set of
six pre-defined aerosol types with the SSA and
asymmetry factor (&lt;i&gt;g&lt;/i&gt;). We assume one aerosol type for a grid of 1° × 1°
and the surface reflectance changes little between two consequent scans. A
&lt;i&gt;k&lt;/i&gt; approximation was used in the inversion to find the best solution of
atmospheric properties and surface reflectance. The algorithm makes use of
numerical minimisation routines to obtain the optimal solution of
atmospheric properties and surface reflectance by selection of the most
suitable aerosol type from pre-defined sets. Also, it is assumed that the
surface reflectance is little influenced by aerosol scattering at 1.6 μm
and therefore the ratio of surface reflectances in the solar band for two
consequent scans can be well-approximated by the ratio of the reflectances
at 1.6 μm. A further assumption is that the surface reflectance varies
only slightly over a period of 30 min.
&lt;br&gt;&lt;br&gt;
A detailed analysis of the retrieval results show that it is suitable for
AOD retrieval over land. Six Aerosol Robotic Network (AERONET) sites with different surface types
were used for detailed analysis and 42 other AERONET sites were used for
validation. From 445 collocations representing stable and homogeneous
aerosol type, we found that &gt;75% of MSG-retrieved AOD values compared
to AERONET observed values with an error envelope of &amp;plusmn;0.05 &amp;plusmn; 0.15&amp;tau; and a high correlation
(&lt;i&gt;R&lt;/i&gt; &gt; 0.86). The AOD datasets derived using the TS method with SEVIRI data
was also compared with collocated AOD products derived from the NASA TERRA
and AQUA MODIS data using the dark dense vegetation (DDV) method and the
Deep Blue algorithms. Using the TS method, AOD could be retrieved for more
pixels than with the NASA Deep Blue algorithm. The AOD values derived
compare favourably.</description><pubDate>Fri, 03 Feb 2012 00:00:00 +0100</pubDate></item><item><title>MAX-DOAS measurements of NO&lt;sub&gt;2&lt;/sub&gt;, HCHO and CHOCHO at a rural site in Southern China</title><link>http://www.atmos-chem-phys-discuss.net/12/3983/2012/</link><description>&lt;b&gt;MAX-DOAS measurements of NO&lt;sub&gt;2&lt;/sub&gt;, HCHO and CHOCHO at a rural site in Southern China&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Chemistry and Physics Discussions, 12, 3983-4029, 2012&lt;br /&gt;&lt;br /&gt;Author(s): X. Li, T. Brauers, A. Hofzumahaus, K. Lu, Y. P. Li, M. Shao, T. Wagner, and A. Wahner&lt;br /&gt;&lt;br /&gt;We performed MAX-DOAS measurements during the PRIDE-PRD2006 campaign
      in the Pearl River Delta region (PRD), China, for 4 weeks in July 2006
      at a site located 60 km north of Guangzhou. The vertical
      distributions of NO&lt;sub&gt;2&lt;/sub&gt;, HCHO, and CHOCHO were
      independently retrieved by an automated iteration method. The MAX-DOAS
      measured NO&lt;sub&gt;2&lt;/sub&gt; mixing ratios showed reasonable agreement with
      the simultaneous, ground based in-situ data. While the tropospheric
      NO&lt;sub&gt;2&lt;/sub&gt; vertical column densities (VCDs) observed by OMI on board
      EOS-Aura satellite agreed with those by MAX-DOAS, the 3-D chemical
      transport model CMAQ overestimated the NO&lt;sub&gt;2&lt;/sub&gt; VCDs as well as the
      surface concentrations by about 40%. From this observation,
      a reduction of NO&lt;sub&gt;X&lt;/sub&gt; emission strength in CMAQ seems to be
      necessary in order to well reproduce the NO&lt;sub&gt;2&lt;/sub&gt; observations. The
      average mixing ratios of HCHO and CHOCHO were 12 ppb
      and 1.6 ppb, respectively, substantially higher than in other rural
      or semirural environments. The high ratio of 0.135 between
      CHOCHO and HCHO corresponds to the high VOCs reactivity
      and high HO&lt;sub&gt;X&lt;/sub&gt; turnover rate consistent with other observations
      during the campaign.</description><pubDate>Fri, 03 Feb 2012 00:00:00 +0100</pubDate></item><item><title>Tropospheric methanol observations from space: retrieval evaluation  and constraints on the seasonality of biogenic emissions</title><link>http://www.atmos-chem-phys-discuss.net/12/3941/2012/</link><description>&lt;b&gt;Tropospheric methanol observations from space: retrieval evaluation  and constraints on the seasonality of biogenic emissions&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Chemistry and Physics Discussions, 12, 3941-3982, 2012&lt;br /&gt;&lt;br /&gt;Author(s): K. C. Wells, D. B. Millet, L. Hu, K. E. Cady-Pereira, Y. Xiao, M. W. Shephard, C. L. Clerbaux, L. Clarisse, P.-F. Coheur, E. C. Apel, J. de Gouw, C. Warneke, H. B. Singh, A. H. Goldstein, and B. C. Sive&lt;br /&gt;&lt;br /&gt;Methanol retrievals from nadir-viewing space-based sensors offer
      powerful new information for quantifying methanol emissions on
      a global scale. Here we apply an ensemble of aircraft observations
      over North America to evaluate new methanol measurements from the
      Tropospheric Emission Spectrometer (TES) on the Aura satellite, and
      combine the TES data with observations from the Infrared Atmospheric
      Sounding Interferometer (IASI) on the MetOp-A satellite to investigate
      the seasonality of methanol emissions from northern midlatitude
      ecosystems. Using the GEOS-Chem chemical transport model as an
      intercomparison platform, we find that the TES retrieval performs well
      when the degrees of freedom for signal (DOFS) are above 0.5, in which
      case the model : TES regressions are generally consistent with the
      model : aircraft comparisons. Including retrievals with DOFS below
      0.5 degrades the comparisons, as these are excessively influenced by
      the a priori. The comparisons suggest DOFS &gt; 0.5 as a minimum
      threshold for interpreting retrievals of trace gases with a weak
      tropospheric signal. We analyze one full year of satellite
      observations and find that GEOS-Chem, driven with MEGANv2.1 biogenic
      emissions, underestimates observed methanol concentrations throughout
      the midlatitudes in springtime, with the timing of the seasonal peak
      in model emissions 1–2 months too late. We attribute this
      discrepancy to an underestimate of emissions from new leaves in MEGAN,
      and apply the satellite data to better quantify the seasonal change in
      methanol emissions for midlatitude ecosystems. The derived parameters
      (relative emission factors of 11.0, 1.0, 0.05 and 8.6 for new,
      growing, mature, and old leaves, respectively, plus a leaf area index
      activity factor of 0.75 for expanding canopies with leaf area
      index &lt; 2.0) provide a more realistic simulation of seasonal
      methanol concentrations in midlatitudes on the basis of IASI, TES, and
      ground-based measurements.</description><pubDate>Fri, 03 Feb 2012 00:00:00 +0100</pubDate></item><item><title>Projections of mid-century summer air-quality for North America: effects of changes in climate and precursor emissions</title><link>http://www.atmos-chem-phys-discuss.net/12/3875/2012/</link><description>&lt;b&gt;Projections of mid-century summer air-quality for North America: effects of changes in climate and precursor emissions&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Chemistry and Physics Discussions, 12, 3875-3940, 2012&lt;br /&gt;&lt;br /&gt;Author(s): J. Kelly, P. A. Makar, and D. A. Plummer&lt;br /&gt;&lt;br /&gt;Ten year simulations of North American current and future air-quality were
carried out using a regional air-quality model driven by a regional climate
model, in turn driven by a general circulation model. Three separate summer
scenarios were performed: a scenario representing the years 1997 to 2006,
and two SRES A2 climate scenarios for the years 2041 to 2050. The first
future climate scenario makes use of 2002 anthropogenic precursor emissions,
and the second applied emissions scaling factors derived from the IPCC
Representative Concentration Pathway 6 (RCP 6) scenario to estimate
emissions for 2050 from existing 2020 projections. Ten-year averages of
ozone and PM&lt;sub&gt;2.5&lt;/sub&gt; at North American monitoring network stations were used
to evaluate the model's current chemical climatology. The model was found to
have a similar performance for ozone as when driven by an operational
weather forecast model. The PM&lt;sub&gt;2.5&lt;/sub&gt; predictions had larger negative
biases, likely resulting from the absence of rainwater evaporation, and from
sub-regional negative biases in the surface temperature fields, in the
version of the climate model used here.
&lt;br&gt;&lt;br&gt;
The differences between the two future climate simulations and the current
climate simulation were used to predict the changes to air-quality that
might be expected in a future warmer climate, if anthropogenic precursor
emissions remain constant at their current levels, versus if the RCP 6
emissions controls were adopted. Metrics of concentration, human health, and
ecosystem damage were compared for the simulations. The scenario with future
climate and current anthropogenic emissions resulted in worse air-quality
than for current conditions – that is, the effect of climate-change alone,
all other factors being similar, would be a worsening of air-quality. These
effects are spatially inhomogeneous, with the magnitude and sign of the
changes varying with region. The scenario with future climate and RCP 6
emissions for 2050 resulted in an improved air-quality, with decreases in
key pollutant concentrations, in acute human mortality associated with
air-pollution, and in sulphur and ozone deposition to the ecosystem. The
positive outcomes of the RCP 6 emissions reductions were found to be of
greater magnitude than the negative outcomes of climate change alone. The
RCP 6 scenario however resulted in an increase in the deposition of
nitrogen, as a result of increased ammonia emissions expected in that
scenario, compared to current ammonia emissions levels.
&lt;br&gt;&lt;br&gt;
The results of the study raise the possibility that simultaneous reductions
of greenhouse gases and air pollution precursors may further reduce air
pollution levels, with the added benefits of an immediate reduction in the
impacts of air pollution on human and ecosystem health. Further scenarios to
investigate this possibility are therefore recommended.</description><pubDate>Fri, 03 Feb 2012 00:00:00 +0100</pubDate></item><item><title>The EMEP MSC-W chemical transport model &amp;ndash; Part 1: Model description</title><link>http://www.atmos-chem-phys-discuss.net/12/3781/2012/</link><description>&lt;b&gt;The EMEP MSC-W chemical transport model &amp;ndash; Part 1: Model description&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Chemistry and Physics Discussions, 12, 3781-3874, 2012&lt;br /&gt;&lt;br /&gt;Author(s): D. Simpson, A. Benedictow, H. Berge, R. Bergström, L. D. Emberson, H. Fagerli, G. D. Hayman, M. Gauss, J. E. Jonson, M. E. Jenkin, A. Nyíri, C. Richter, V. S. Semeena, S. Tsyro, J.-P. Tuovinen, Á. Valdebenito, and P. Wind&lt;br /&gt;&lt;br /&gt;The Meteorological Synthesizing Centre-West (MSC-W) of
the European Monitoring and Evaluation Programme (EMEP)  has been performing
model calculations in support of the Convention on Long Range Transboundary Air Pollution (CLRTAP)
for more than 30 yr.
The EMEP MSC-W chemical transport model is still one of the key tools within
European air pollution policy assessments.
&lt;br&gt;&lt;br&gt;
Traditionally, the EMEP  model has covered all of Europe with
a resolution of about 50 × 50 km&lt;sup&gt;2&lt;/sup&gt;,
and extending vertically from ground
level to the tropopause (100 hPa). The model has undergone substantial
development in recent years, and is now applied on scales
ranging from local (ca. 5 km grid size) to global (with 1 degree
resolution).
The  model is used to simulate photo-oxidants and
both inorganic and organic aerosols.
&lt;br&gt;&lt;br&gt;
In 2008 the EMEP model was released for the first time as public domain
code, along with all required input data for model runs for one year.
Since then, many changes have been made to the model physics, and input data.
The second release of the EMEP MSC-W model
became available in mid
2011, and a new release is targeted for early 2012.  This publication is
intended to document this third release of the EMEP MSC-W model.
The model formulations are given, along with details
of input data-sets which are used, and brief background
on some of the choices made in the formulation are
presented.
The model code itself is available at 
&lt;a href=&quot;http://www.emep.int&quot;target=&quot;_blank&quot;&gt;www.emep.int&lt;/a&gt;, along with
the data required to  run for a full year over Europe.</description><pubDate>Thu, 02 Feb 2012 00:00:00 +0100</pubDate></item><item><title>Lessons learnt from the first EMEP intensive measurement periods</title><link>http://www.atmos-chem-phys-discuss.net/12/3731/2012/</link><description>&lt;b&gt;Lessons learnt from the first EMEP intensive measurement periods&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Chemistry and Physics Discussions, 12, 3731-3780, 2012&lt;br /&gt;&lt;br /&gt;Author(s): W. Aas, S. Tsyro, E. Bieber, R. Bergström, D. Ceburnis, T. Ellermann, H. Fagerli, M. Frölich, R. Gehrig, U. Makkonen, E. Nemitz, R. Otjes, N. Perez, C. Perrino, A. S. H. Prévôt, J.-P. Putaud, D. Simpson, G. Spindler, M. Vana, and K. E. Yttri&lt;br /&gt;&lt;br /&gt;The first EMEP intensive measurement periods were held in June 2006 and
January 2007. The measurements aimed to characterize the aerosol chemical
compositions, including the gas/aerosol partitioning of inorganic compounds.
The measurement program during these periods included daily or hourly
measurements of the secondary inorganic components, with additional
measurements of elemental- and organic carbon (EC and OC) and mineral dust
in PM&lt;sub&gt;1&lt;/sub&gt;, PM&lt;sub&gt;2.5&lt;/sub&gt; and PM&lt;sub&gt;10&lt;/sub&gt;. These measurements have provided
extended knowledge regarding the composition of particulate matter and the
temporal and spatial variability of PM, as well as an extended database for
the assessment of chemical transport models. This paper summarise the first
experiences of making use of measurements from the first EMEP intensive
measurement periods along with EMEP model results from the updated model
version to characterise aerosol composition. We investigated how the PM
chemical composition varies between the summer and the winter month and
geographically.
&lt;br&gt;&lt;br&gt;
The observation and model data are in general agreement regarding the main
features of PM&lt;sub&gt;10&lt;/sub&gt; and PM&lt;sub&gt;2.5&lt;/sub&gt; composition and the relative
contribution of different components, though the EMEP model tends to
slightly underestimate PM&lt;sub&gt;10&lt;/sub&gt; and PM&lt;sub&gt;2.5&lt;/sub&gt; compared to measurements.
The intensive measurement data has identified areas where improvements are
needed. In particular, the model description of formation of coarse nitrate
on sea salt and dust particles requires further attention. Hourly concurrent
measurements of gaseous and particulate components for the first time
facilitated testing of modelled diurnal variability of the gas/aerosol
partitioning of nitrogen species. In general, the modelled diurnal cycles of
nitrate and ammonium aerosols are in good agreement with the measurements.
As expected, the diurnal variability of ammonia is not very well captured,
but this will probably improve if the EMEP model is coupled to a dynamic,
mechanistic ammonia emission module. The largest underestimations of aerosol
mass are seen in Italy during winter, which to a large extent may be
explained by an underestimation of residential wood burning source. It
should be noted that both primary and secondary OC has been included in the
calculations for the first time, showing promising results. Mineral dust is
important, especially in southern Europe, and the model seems to capture the
dust episodes well. The lack of measurements of mineral dust hampers the
possibility for model evaluation for this highly uncertain PM component.
&lt;br&gt;&lt;br&gt;
There are also lessons learnt regarding improved measurements for future
intensive periods. There is a need for increased comparability between the
measurements at different sites. For the nitrogen compounds it is clear that
more measurements using artefact free methods based on continuous
measurement methods and/or denuders are needed. For EC/OC, a reference
methodology (both in field and laboratory) was lacking during these periods
giving problems with comparability, though presently measurement protocols
have been established and these should be followed by the Parties to the
EMEP Protocol. For measurements with no defined protocols, it might be a
good solution to use centralised laboratories to ensure comparability across
the network. To cope with the introduction of these new measurements new
reporting guidelines have been developed to ensure that all proper
information about the methodologies and data quality is given.</description><pubDate>Thu, 02 Feb 2012 00:00:00 +0100</pubDate></item><item><title>Regional air-quality forecasting for the Pacific Northwest using MOPITT/TERRA assimilated carbon monoxide MOZART-4 forecasts as a near real-time boundary condition</title><link>http://www.atmos-chem-phys-discuss.net/12/3695/2012/</link><description>&lt;b&gt;Regional air-quality forecasting for the Pacific Northwest using MOPITT/TERRA assimilated carbon monoxide MOZART-4 forecasts as a near real-time boundary condition&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Chemistry and Physics Discussions, 12, 3695-3730, 2012&lt;br /&gt;&lt;br /&gt;Author(s): F. L. Herron-Thorpe, G. H. Mount, L. K. Emmons, B. K. Lamb, S. H. Chung, and J. K. Vaughan&lt;br /&gt;&lt;br /&gt;Results from a regional air quality forecast model, AIRPACT-3, were compared
to AIRS carbon monoxide column densities for the spring of 2010 over the
Pacific Northwest. AIRPACT-3 column densities showed high correlation
(&lt;i&gt;R&lt;/i&gt;&gt;0.9) but were significantly biased (~25 %) with significant
under-predictions for spring months with significant transport from Asia. The
AIRPACT-3 CO bias relative to AIRS was eliminated by incorporating dynamic
boundary conditions derived from NCAR's MOZART forecasts with assimilated
MOPITT carbon monoxide. Changes in ozone-related boundary conditions derived
from MOZART forecasts are also discussed and found to affect background
levels by ±10 ppb but not found to significantly affect peak ozone
surface concentrations.</description><pubDate>Thu, 02 Feb 2012 00:00:00 +0100</pubDate></item><item><title>Biogenic influence on cloud microphysics over the global ocean</title><link>http://www.atmos-chem-phys-discuss.net/12/3655/2012/</link><description>&lt;b&gt;Biogenic influence on cloud microphysics over the global ocean&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Chemistry and Physics Discussions, 12, 3655-3694, 2012&lt;br /&gt;&lt;br /&gt;Author(s): A. Lana, R. Simó, S. M. Vallina, and J. Dachs&lt;br /&gt;&lt;br /&gt;Aerosols have a large potential to influence climate through their
      effects on the microphysics and optical properties of clouds and,
      hence, on the Earth's radiation budget. Aerosol-cloud interactions
      have been intensively studied in polluted air, but the possibility
      that the marine biosphere plays a role in regulating cloud
      brightness in the pristine oceanic atmosphere remains largely
      unexplored. We used 9 yr of global satellite data and ocean
      climatologies to derive parameterizations of (a) production fluxes of
      sulfur aerosols formed by the oxidation of the biogenic gas
      dimethylsulfide emitted from the sea surface; (b) production fluxes of
      secondary organic aerosols from biogenic organic volatiles;
      (c) emission fluxes of biogenic primary organic aerosols ejected by
      wind action on sea surface; and (d) emission fluxes of sea salt also
      lifted by the wind upon bubble bursting. Series of global weekly
      estimates of these fluxes were correlated to series of cloud droplet
      effective radius data derived from satellite (MODIS). Similar analyses
      were conducted in more detail at 6 locations spread among polluted and
      clean regions of the oceanic atmosphere. The outcome of the
      statistical analysis was that negative correlation was common at mid
      and high latitude for sulfur and organic secondary aerosols,
      indicating both might be important in seeding cloud droplet
      activation. Conversely, primary aerosols (organic and sea salt) showed
      more variable, non-significant or positive correlations, indicating
      that, despite contributing to large shares of the marine aerosol mass,
      they are not major drivers of the variability of cloud
      microphysics. Uncertainties and synergisms are discussed, and
      recommendations of research needs are given.</description><pubDate>Thu, 02 Feb 2012 00:00:00 +0100</pubDate></item><item><title>Signals of El Niño Modoki in the tropical tropopause layer and stratosphere</title><link>http://www.atmos-chem-phys-discuss.net/12/3619/2012/</link><description>&lt;b&gt;Signals of El Niño Modoki in the tropical tropopause layer and stratosphere&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Chemistry and Physics Discussions, 12, 3619-3653, 2012&lt;br /&gt;&lt;br /&gt;Author(s): F. Xie, J. Li, W. Tian, and J. Feng&lt;br /&gt;&lt;br /&gt;The effects of El Niño Modoki events on the tropical tropopause layer
(TTL) and on the stratosphere were investigated using European Center for
Medium Range Weather Forecasting (ECMWF) reanalysis data, satellite
observations from the Aura satellite Microwave Limb Sounder (MLS), oceanic
El Niño indices, and general climate model outputs. El Niño Modoki
events tend to depress convective activities in the western and eastern
Pacific but enhance convective activities in the central and northern
Pacific. Consequently, during Modoki events, negative water vapor anomalies
occur in the western and eastern Pacific upper troposphere, whereas there
are positive anomalies in the central and northern Pacific upper
troposphere. The spatial patterns of the outgoing longwave radiation (OLR)
and upper tropospheric water vapor anomalies exhibit a tripolar form. The
empirical orthogonal function (EOF) analysis of the OLR and upper
tropospheric water vapor anomalies reveals that canonical El Niño events
are associated with the leading mode of the EOF, while El Niño Modoki
events correspond to the second mode. El Niño Modoki activities tend to
moisten the lower and middle stratosphere, but dry the upper stratosphere.
It was also found that the canonical El Niño signal can overlay linearly
on the QBO signal in the stratosphere, whereas the interaction between the
El Niño Modoki and QBO signals is non-linear. Because of these
non-linear interactions, El Niño Modoki events have a reverse effect on
high latitudes stratosphere, as compared with the effects of typical Modoki
events, i.e. the northern polar vortex is stronger and colder but the
southern polar vortex is weaker and warmer during El Niño Modoki events.
However, simulations suggest that canonical El Niño and El Niño
Modoki activities actually have the same influence on high latitudes
stratosphere, in the absence of interactions between QBO and ENSO signals.
The present results also reveal that canonical El Niño events have a
greater impact on the high-latitude Northern Hemisphere stratosphere than on
the high-latitude Southern Hemisphere stratosphere. However, El Niño
Modoki events can more profoundly influence the high-latitude Southern
Hemisphere stratosphere than the high-latitude Northern Hemisphere
stratosphere.</description><pubDate>Thu, 02 Feb 2012 00:00:00 +0100</pubDate></item><item><title>Effects of cosmic ray decreases on cloud microphysics</title><link>http://www.atmos-chem-phys-discuss.net/12/3595/2012/</link><description>&lt;b&gt;Effects of cosmic ray decreases on cloud microphysics&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Chemistry and Physics Discussions, 12, 3595-3617, 2012&lt;br /&gt;&lt;br /&gt;Author(s): J. Svensmark, M. B. Enghoff, and H. Svensmark&lt;br /&gt;&lt;br /&gt;Using cloud data from MODIS we investigate the response of cloud microphysics
to sudden decreases in galactic cosmic radiation – Forbush decreases – and
find responses in effective emissivity, cloud fraction, liquid water content,
and optical thickness above the 2–3 sigma level 6–9 days after the minimum in
atmospheric ionization and less significant responses for effective radius
and cloud condensation nuclei (&lt;2 sigma). The magnitude of the signals
agree with derived values, based on simple equations for atmospheric
parameters. Furthermore principal components analysis gives a total
significance of the signal of 3.1 sigma. We also see a correlation between
total solar irradiance and strong Forbush decreases but a clear mechanism
connecting this to cloud properties is lacking. There is no signal in the UV
radiation. The responses of the parameters correlate linearly with the
reduction in the cosmic ray ionization. These results support the suggestion
that ions play a significant role in the life-cycle of clouds.</description><pubDate>Wed, 01 Feb 2012 00:00:00 +0100</pubDate></item><item><title>A mechanistic model of global soil nitric oxide emissions: implementation and space based-constraints</title><link>http://www.atmos-chem-phys-discuss.net/12/3555/2012/</link><description>&lt;b&gt;A mechanistic model of global soil nitric oxide emissions: implementation and space based-constraints&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Chemistry and Physics Discussions, 12, 3555-3594, 2012&lt;br /&gt;&lt;br /&gt;Author(s): R. C. Hudman, N. E. Moore, R. V. Martin, A. R. Russell, A. K. Mebust, L. C. Valin, and R. C. Cohen&lt;br /&gt;&lt;br /&gt;Soil emissions have been identified as a major source (~15%) of
global nitrogen oxide (NO&lt;sub&gt;x&lt;/sub&gt;) emissions. Parameterizations of soil
NO&lt;sub&gt;x&lt;/sub&gt; emissions (&lt;i&gt;S&lt;/i&gt;&lt;sub&gt;NO&lt;sub&gt;x&lt;/sub&gt;&lt;/sub&gt;) for use in the current
generation of chemical transport models were designed to capture mean
seasonal behaviour. These parameterizations do not, however, respond
quantitatively to the meteorological triggers that result in pulsed &lt;i&gt;S&lt;/i&gt;&lt;sub&gt;NO&lt;sub&gt;x&lt;/sub&gt;&lt;/sub&gt; as are widely observed. Here we present a new mechanistic
parameterization of &lt;i&gt;S&lt;/i&gt;&lt;sub&gt;NO&lt;sub&gt;x&lt;/sub&gt;&lt;/sub&gt; implemented into a global chemical
transport model (GEOS-Chem). The parameterization represents available
nitrogen (N) in soils using biome specific emission factors, online wet- and
dry-deposition of N as well as fertilizer and manure N derived from a
spatially explicit dataset distributed using seasonality derived from data
obtained by the Moderate Resolution Imaging Spectrometer. Moreover, it
represents the functional form of emissions derived from point measurements
and ecosystem scale experiments including pulsing following soil wetting by
rain or irrigation, and emissions that are a smooth function of soil
moisture. This parameterization yields global above-soil &lt;i&gt;S&lt;/i&gt;&lt;sub&gt;NO&lt;sub&gt;x&lt;/sub&gt;&lt;/sub&gt;
of 10.7 Tg N yr&lt;sup&gt;−1&lt;/sup&gt;, including 1.8 Tg N yr&lt;sup&gt;−1&lt;/sup&gt; from fertilizer N
input (0.68% of applied N) and 0.5 Tg N yr&lt;sup&gt;−1&lt;/sup&gt; from atmospheric N
deposition. Over the United States Great Plains, &lt;i&gt;S&lt;/i&gt;&lt;sub&gt;NO&lt;sub&gt;x&lt;/sub&gt;&lt;/sub&gt; are
predicted to comprise 15–40% of the tropospheric NO&lt;sub&gt;2&lt;/sub&gt; column and
increase column variability by a factor of 2–4 during the summer months due
to chemical fertilizer application and warm temperatures. &lt;i&gt;S&lt;/i&gt;&lt;sub&gt;NO&lt;sub&gt;x&lt;/sub&gt;&lt;/sub&gt; enhancements of 50–80% of the simulated NO&lt;sub&gt;2&lt;/sub&gt; column are
predicted over the African Sahel during the monsoon onset (April–June). In
this region the day-to-day variability of column NO&lt;sub&gt;2&lt;/sub&gt; is increased by a
factor of 5 due to pulsed-N emissions. We evaluate the model by comparison to
observations of the NO&lt;sub&gt;2&lt;/sub&gt; column from the OMI instrument. We find the
model is able to reproduce observations of pulsed-N induced interannual
variability over the US Great Plains. We also show that the OMI mean (median)
NO&lt;sub&gt;2&lt;/sub&gt; on the overpass following first rainfall over the Sahel is 49%
(23%) higher than in the five days preceding. The measured NO&lt;sub&gt;2&lt;/sub&gt; on
the day after rainfall is still 23% (5%) higher, providing a direct
measure of the pulse's decay time of 1–2 days. This is consistent with the
pulsing representation used in our parameterization and much shorter than
5–14 day pulse decay length used in current models.</description><pubDate>Wed, 01 Feb 2012 00:00:00 +0100</pubDate></item><item><title>Black carbon from ships: a review of the effects of ship speed, fuel  quality and exhaust gas scrubbing</title><link>http://www.atmos-chem-phys-discuss.net/12/3509/2012/</link><description>&lt;b&gt;Black carbon from ships: a review of the effects of ship speed, fuel  quality and exhaust gas scrubbing&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Chemistry and Physics Discussions, 12, 3509-3554, 2012&lt;br /&gt;&lt;br /&gt;Author(s): D. A. Lack and J. J. Corbett&lt;br /&gt;&lt;br /&gt;The International Maritime Organization (IMO) has moved to address the
      health and climate impact of the emissions from the combustion of
      low-quality residual fuels within the commercial shipping
      industry. Fuel sulfur content (&lt;i&gt;F&lt;/i&gt;&lt;sub&gt;S&lt;/sub&gt;) limits and an efficiency
      design index for future ships are examples of such IMO actions. The
      impacts of black carbon (BC) emissions from shipping are now under
      review by the IMO, with a particular focus on the potential impacts of
      future Arctic shipping.
&lt;br&gt;&lt;br&gt;
      Recognizing that associating impacts with BC emissions requires both
      ambient and onboard observations, we provide recommendations for the
      measurement of BC. We also evaluate current insights regarding the
      effect of ship speed (engine load), fuel quality and exhaust gas
      scrubbing on BC emissions from ships. Observations demonstrate that BC
      emission factors (EF&lt;sub&gt;BC&lt;/sub&gt;) increases 3 to 6 times at very low
      engine loads (&lt;25% compared to EF&lt;sub&gt;BC&lt;/sub&gt; at 85–100%
      load); absolute BC emissions (per nautical mile of travel) also
      increase up to 100% depending on engine load, even with reduced
      load fuel savings. If fleets were required to operate at lower maximum
      engine loads, presumably associated with reduced speeds, then engines
      could be re-tuned, which would reduce BC emissions.
&lt;br&gt;&lt;br&gt;
      Ships operating in the Arctic are likely running at highly variable
      engine loads (25–100%) depending on ice conditions and ice
      breaking requirements. The ships operating at low load may be emitting
      up to 50% more BC than they would at their rated load. Such
      variable load conditions make it difficult to assess the likely
      emissions rate of BC.
&lt;br&gt;&lt;br&gt;
      Current fuel sulfur regulations have the effect of reducing
      EF&lt;sub&gt;BC&lt;/sub&gt; by an average of 30% and potentially up to
      80% regardless of engine load; a removal rate similar to that of
      scrubbers.
&lt;br&gt;&lt;br&gt;
      Uncertainties among current observations demonstrate there is a need
      for more information on (a) the impact of fuel quality on
      EF&lt;sub&gt;BC&lt;/sub&gt; using robust measurement methods and (b) the efficacy of
      scrubbers for the removal of particulate matter by size and
      composition.</description><pubDate>Tue, 31 Jan 2012 00:00:00 +0100</pubDate></item><item><title>Interaction of anthropogenic and natural emission sources during a wild-land fire event – influence on ozone formation</title><link>http://www.atmos-chem-phys-discuss.net/12/3467/2012/</link><description>&lt;b&gt;Interaction of anthropogenic and natural emission sources during a wild-land fire event – influence on ozone formation&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Chemistry and Physics Discussions, 12, 3467-3507, 2012&lt;br /&gt;&lt;br /&gt;Author(s): E. Bossioli, M. Tombrou, A. Karali, A. Dandou, D. Paronis, and M. Sofiev&lt;br /&gt;&lt;br /&gt;The objective of this study is to investigate the contribution of biomass
burning in the formation of tropospheric O&lt;sub&gt;3&lt;/sub&gt;. Furthermore, the impact of
biogenic emissions under fire and no fire conditions is examined. This is
achieved by applying the CAMx chemistry transport model for a wild-land fire
event over Western Russia (24 April–10 May 2006). The model results are
compared with O&lt;sub&gt;3&lt;/sub&gt; and isoprene observations from 117 and 9 stations of
the EMEP network, respectively.

&lt;br&gt;&lt;br&gt;

Model computations show that the fire episode altered the O&lt;sub&gt;3&lt;/sub&gt;
sensitivity in the area. In particular, the fire emissions increased surface
O&lt;sub&gt;3&lt;/sub&gt; over Northern and Eastern Europe by up to 80% (40–45 ppb). In
case of adopting a high fire NO&lt;sub&gt;x&lt;/sub&gt;/CO emission ratio (0.06), the area
(Eastern Europe and Western Russia) is characterized by VOC-sensitive
O&lt;sub&gt;3&lt;/sub&gt; production and the impact of biogenic emissions is proven
significant, contributing up to 8 ppb. Under a lower ratio (0.025), total
surface O&lt;sub&gt;3&lt;/sub&gt; is almost doubled due to higher O&lt;sub&gt;3&lt;/sub&gt; production at the
fire spots and lower fires' NO emissions. In this case as well as in the
absence of fires, the impact of biogenic emissions is almost negligible.
Injection height of the fire emissions accounted for O&lt;sub&gt;3&lt;/sub&gt; differences of
the order of 10%, both at surface and over the planetary boundary layer
(PBL).</description><pubDate>Tue, 31 Jan 2012 00:00:00 +0100</pubDate></item><item><title>The scavenging processes controlling the seasonal cycle in Arctic sulphate and black carbon aerosol</title><link>http://www.atmos-chem-phys-discuss.net/12/3409/2012/</link><description>&lt;b&gt;The scavenging processes controlling the seasonal cycle in Arctic sulphate and black carbon aerosol&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Chemistry and Physics Discussions, 12, 3409-3465, 2012&lt;br /&gt;&lt;br /&gt;Author(s): J. Browse, K. S. Carslaw, S. R. Arnold, K. Pringle, and O. Boucher&lt;br /&gt;&lt;br /&gt;The seasonal cycle in Arctic aerosol is typified by high
      concentrations of large aged anthropogenic particles
      transported from lower latitudes in the late Arctic winter and
      early spring followed by a sharp transition to low
      concentrations of locally sourced smaller particles in the
      summer. However, multi-model assessments show that many models
      fail to simulate a realistic cycle. Here, we use a global
      aerosol microphysics model and surface-level aerosol
      observations to understand how wet scavenging processes
      control the seasonal variation in Arctic black carbon (BC) and
      sulphate aerosol concentrations. We show that the transition
      from high wintertime to low summertime Arctic aerosol
      concentrations is caused by the change from inefficient
      scavenging in ice clouds to the much more efficient scavenging
      in warm liquid clouds. This seasonal cycle is amplified
      further by the appearance of warm drizzling cloud in late
      spring and summer at a time when aerosol transport shifts
      mainly to low levels. Implementing these processes in a model
      greatly improves the agreement between the model and
      observations at the three Arctic ground-stations Alert, Barrow
      and Zeppelin Mountain on Svalbard. The SO&lt;sub&gt;4&lt;/sub&gt;
      model-observation correlation coefficient (&lt;i&gt;R&lt;/i&gt;) increases from:
      &amp;minus;0.33 to 0.71 at Alert (82.5&amp;deg; N), from &amp;minus;0.16 to
      0.70 at Point Barrow (71.0&amp;deg; N) and from &amp;minus;0.42 to
      0.40 at Zeppelin Mountain (78&amp;deg; N) while, the BC
      model-observation correlation coefficient increases from
      &amp;minus;0.68 to 0.72 at Alert and from &amp;minus;0.42 to 0.44 at
      Barrow. Observations at three marginal Arctic sites
      (Janiskoski, Oulanka and Karasjok) indicate a far weaker
      aerosol seasonal cycle, which we show is consistent with the
      much smaller seasonal changes in ice clouds compared to the
      higher latitude sites. Our results suggest that the seasonal
      cycle in Arctic aerosol is driven by temperature-dependent
      scavenging processes that may be susceptible to modification
      in a future climate.</description><pubDate>Tue, 31 Jan 2012 00:00:00 +0100</pubDate></item><item><title>Uncertainties of parameterized near-surface downward longwave and clear-sky direct radiation</title><link>http://www.atmos-chem-phys-discuss.net/12/3357/2012/</link><description>&lt;b&gt;Uncertainties of parameterized near-surface downward longwave and clear-sky direct radiation&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Chemistry and Physics Discussions, 12, 3357-3407, 2012&lt;br /&gt;&lt;br /&gt;Author(s): S. Gubler, S. Gruber, and R. S. Purves&lt;br /&gt;&lt;br /&gt;As many environmental models rely on simulating the energy balance at
      the Earth's surface based on parameterized radiative fluxes, knowledge
      of the inherent uncertainties is important. In this study we evaluate
      one parameterization of clear-sky incoming shortwave radiation (SDR)
      and diverse parameterizations of clear-sky and all-sky incoming
      longwave radiation (LDR). In a first step, the clear-sky
      global SDR is estimated based measured input variables and mean
      parameter values for hourly time steps during the year 1996 to 2008, and
      validated using the high quality measurements of seven Alpine Surface
      Radiation Budget (ASRB) stations in Switzerland covering different
      elevations. Then, twelve clear-sky LDR parameterizations are
      fitted to the ASRB measurements. One of the best performing LDR
      parameterizations is chosen to estimate the all-sky LDR based
      on cloud transmissivity. Cloud transmissivity is
      estimated using measured and modeled global SDR during daytime. For
      the night, the performance of several interpolation methods is
      evaluated.
&lt;br&gt;&lt;br&gt;
      Input variable and parameter uncertainties are assigned to estimate
      the total output uncertainty of the mentioned models, resulting in
      a mean relative uncertainty of 10% for the clear-sky direct,
      15% for diffuse and 2.5% for global SDR, and 2.5% for
      the fitted all-sky LDR. Further, a function representing the
      uncertainty in dependence of the radiation is assigned for each
      model. Validation of the model outputs shows that direct SDR is
      underestimated (the mean error (ME) is around
      &amp;minus;33 W m&lt;sup&gt;&amp;minus;2&lt;/sup&gt;), while diffuse radiation is
      overestimated (ME around 19 W m&lt;sup&gt;&amp;minus;2&lt;/sup&gt;). The root mean
      squared error (RMSE) scatters around 60  W m&lt;sup&gt;&amp;minus;2&lt;/sup&gt; for
      direct, and 40 W m&lt;sup&gt;&amp;minus;2&lt;/sup&gt; for diffuse SDR. The best
      behaviour is found, due to the compensating effects of direct and
      diffuse SDR, for global SDR with MEs around
      &amp;minus;13 W m&lt;sup&gt;&amp;minus;2&lt;/sup&gt; and RMSEs around
      40 W m&lt;sup&gt;&amp;minus;2&lt;/sup&gt;. The ME of the fitted all-sky LDR
      is around &amp;plusmn;10 W m&lt;sup&gt;&amp;minus;2&lt;/sup&gt;, and
      the RMSE goes up to 40 W m&lt;sup&gt;&amp;minus;2&lt;/sup&gt;. This is obtained by
      linearly interpolating the average of the cloud transmissivity of the
      four hours of the preceeding afternoon and the following morning.</description><pubDate>Tue, 31 Jan 2012 00:00:00 +0100</pubDate></item><item><title>Multi-generation gas-phase oxidation, equilibrium partitioning, and the formation and evolution of secondary organic aerosol</title><link>http://www.atmos-chem-phys-discuss.net/12/3295/2012/</link><description>&lt;b&gt;Multi-generation gas-phase oxidation, equilibrium partitioning, and the formation and evolution of secondary organic aerosol&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Chemistry and Physics Discussions, 12, 3295-3356, 2012&lt;br /&gt;&lt;br /&gt;Author(s): C. D. Cappa and K. R. Wilson&lt;br /&gt;&lt;br /&gt;A new statistical model of secondary organic aerosol (SOA) formation is
developed that explicitly takes into account multi-generational oxidation as
well as fragmentation of gas-phase compounds. The model framework requires
three tunable parameters to describe the kinetic evolution of SOA mass, the
average oxygen-to-carbon atomic ratio and the mean particle volatility as
oxidation proceeds. These parameters describe (1) the relationship between
oxygen content and volatility, (2) the probability of fragmentation and (3)
the amount of oxygen added per reaction. The time-evolution and absolute
value of the SOA mass depends sensitively on all three tunable parameters.
Of the tunable parameters, the mean O:C is most sensitive to the
oxygen/volatility relationship, exhibiting only a weak dependence on the
other two. The mean particle O:C produced from a given compound is primarily
controlled by the number of carbon atoms comprising the SOA precursor. It
is found that gas-phase compounds with larger than 11 carbon atoms are
unlikely to form SOA with O:C values &gt;0.4, which suggests that so-called
&quot;intermediate-volatility&quot; organic compounds (IVOCs) and &quot;semi-volatile&quot;
organic compounds (SVOCs) are not major contributors to the ambient SOA
burden when high O:C ratios are observed, especially at short atmospheric
times. The model is tested against laboratory measurements of SOA formation
from the photooxidation of α-pinene and &lt;i&gt;n&lt;/i&gt;-pentadecane and performs
well (after tuning). This model may provide a generalized framework for the
interpretation of laboratory SOA formation experiments in which explicit
consideration of multiple-generations of products is required, which is true
for all photo-oxidation experiments.</description><pubDate>Tue, 31 Jan 2012 00:00:00 +0100</pubDate></item><item><title>Stochastic parameterization of dust emission and application to convective atmospheric conditions</title><link>http://www.atmos-chem-phys-discuss.net/12/3263/2012/</link><description>&lt;b&gt;Stochastic parameterization of dust emission and application to convective atmospheric conditions&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Chemistry and Physics Discussions, 12, 3263-3293, 2012&lt;br /&gt;&lt;br /&gt;Author(s): M. Klose and Y. Shao&lt;br /&gt;&lt;br /&gt;We develop a parameterization scheme of convective dust emission for
regional and global atmospheric models. Convective dust emission occurs in the absence
of saltation as large eddies intermittently produce strong shear stresses
on the surface and thereby entrain dust particles into the air. The new scheme presented here
takes account of the stochastic nature of convective dust emission. It
consists of the statistical representations of soil particle size, inter-particle
cohesion and instantaneous surface shear stress. A method of determining the probability
density function of the latter quantity is proposed. Dust emission is then
estimated from the overlap of the probability density functions of the aerodynamic
lifting and inter-particle cohesive forces. The new scheme is implemented
into the WRF/Chem model and applied to dust modeling in the Taklimakan Desert. A
comparison with lidar data shows that the model can reproduce the main features of the dust
patterns and their diurnal variations. For the case studied, convective dust emission
is typically several μg m&lt;sup&gt;−2&lt;/sup&gt; s&lt;sup&gt;−1&lt;/sup&gt; and at times up to 50 μg m&lt;sup&gt;−2&lt;/sup&gt; s&lt;sup&gt;−1&lt;/sup&gt;.</description><pubDate>Mon, 30 Jan 2012 00:00:00 +0100</pubDate></item></channel></rss>
