<?xml version="1.0" encoding="utf-8"?><!DOCTYPE rss PUBLIC "-//Netscape Communications//DTD RSS 0.91//EN" "http://my.netscape.com/publish/formats/rss-0.91.dtd"><rss version="0.91"><channel><title>ACP - Latest Articles</title><link>http://www.atmos-chem-phys.net/</link> <description>Atmospheric Chemistry and Physics Latest Articles</description><language>en</language><item><title>A functional group oxidation model (FGOM) for SOA formation and aging</title><link>http://www.atmos-chem-phys.net/13/5907/2013/</link><description>&lt;b&gt;A functional group oxidation model (FGOM) for SOA formation and aging&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Chemistry and Physics, 13, 5907-5926, 2013&lt;br /&gt;&lt;br /&gt;Author(s): X. Zhang and J. H. Seinfeld&lt;br /&gt;&lt;br /&gt;Secondary organic aerosol (SOA) formation from a volatile organic compound
(VOC) involves multiple generations of oxidation that include
functionalization and fragmentation of the parent carbon backbone and
likely particle-phase oxidation and/or accretion reactions. Despite the
typical complexity of the detailed molecular mechanism of SOA formation and
aging, a relatively small number of functional groups characterize the
oxidized molecules that constitute SOA. Given the carbon number and set of
functional groups, the volatility of the molecule can be estimated. We
present here a functional group oxidation model (FGOM) that represents the
process of SOA formation and aging. The FGOM contains a set of parameters
that are to be determined by fitting of the model to laboratory chamber data:
total organic aerosol concentration, and O : C and H : C atomic ratios.
The sensitivity of the model prediction to variation of the adjustable
parameters allows one to assess the relative importance of various pathways
involved in SOA formation. An analysis of SOA formation from the high- and
low-NO&lt;sub&gt;x&lt;/sub&gt; photooxidation of four C&lt;sub&gt;12&lt;/sub&gt; alkanes (n-dodecane,
2-methylundecane, hexylcyclohexane, and cyclododecane) using the FGOM is
presented, and comparison with the statistical oxidation model (SOM) of Cappa
et al. (2013) is discussed.</description><pubDate>Tue, 18 Jun 2013 00:00:00 +0200</pubDate></item><item><title>Estimation of volatile organic compound emissions for Europe using data assimilation</title><link>http://www.atmos-chem-phys.net/13/5887/2013/</link><description>&lt;b&gt;Estimation of volatile organic compound emissions for Europe using data assimilation&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Chemistry and Physics, 13, 5887-5905, 2013&lt;br /&gt;&lt;br /&gt;Author(s): M. R. Koohkan, M. Bocquet, Y. Roustan, Y. Kim, and C. Seigneur&lt;br /&gt;&lt;br /&gt;The emissions of non-methane volatile organic compounds (VOCs) over western
Europe for the year 2005 are estimated via inverse modelling by assimilation
of in situ observations of concentration and then subsequently compared to
a standard emission inventory. The study focuses on 15 VOC species: five
aromatics, six alkanes, two alkenes, one alkyne and one biogenic diene. The
inversion relies on a validated fast adjoint of the chemical transport model
used to simulate the fate and transport of these VOCs.  The assimilated
ground-based measurements over Europe are provided by the European Monitoring
and Evaluation Programme (EMEP) network.  The background emission errors and
the prior observational errors are estimated by maximum-likelihood approaches.
The positivity assumption on the VOC emission fluxes is pivotal for a
successful inversion, and this maximum-likelihood approach consistently
accounts for the positivity of the fluxes.  For most species, the retrieved
emissions lead to a significant reduction of the bias, which underlines the
misfit between the standard inventories and the observed concentrations.  The
results are validated through a forecast test and a cross-validation test.  An
estimation of the posterior uncertainty is also provided.  It is shown that
the statistically consistent non-Gaussian approach based on a reliable
estimation of the errors offers the best performance. The efficiency in
correcting the inventory depends on the lifetime of the VOCs and the accuracy
of the boundary conditions. In particular, it is shown that the use of in situ
observations using a sparse monitoring network to estimate emissions of
isoprene is inadequate because its short chemical lifetime significantly
limits the spatial radius of influence of the monitoring data. For species
with a longer lifetime (a few days), successful, albeit partial, emission
corrections can reach regions hundreds of kilometres away from the stations.
Domain-wide corrections of the emission inventories of some VOCs are
significant, with underestimations of the order of a factor of 2 for
propane, ethane, ethylene and acetylene.</description><pubDate>Tue, 18 Jun 2013 00:00:00 +0200</pubDate></item><item><title>Modeling air pollution in Lebanon: evaluation at a suburban site in Beirut during summer</title><link>http://www.atmos-chem-phys.net/13/5873/2013/</link><description>&lt;b&gt;Modeling air pollution in Lebanon: evaluation at a suburban site in Beirut during summer&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Chemistry and Physics, 13, 5873-5886, 2013&lt;br /&gt;&lt;br /&gt;Author(s): A. Waked, C. Seigneur, F. Couvidat, Y. Kim, K. Sartelet, C. Afif, A. Borbon, P. Formenti, and S. Sauvage&lt;br /&gt;&lt;br /&gt;Beirut, the capital of Lebanon, which is located on the eastern shore
of the Mediterranean basin, experiences high air pollution episodes. Annual
average concentrations of coarse and fine particulate matter (PM&lt;sub&gt;2.5&lt;/sub&gt;) as
well as nitrogen oxides (NO&lt;sub&gt;x&lt;/sub&gt;) often exceed the World Health
Organization (WHO) guidelines. Therefore, improving air quality in this
region is essential. The Polyphemus/Polair3D modeling system is used here to
investigate air pollution episodes in Beirut during 2 to 18 July 2011. The
modeling domain covers two nested grids of 1 and 5 km horizontal resolution
over greater Beirut and Lebanon, respectively. The anthropogenic
emission inventory was developed earlier (Waked et al., 2012). The Weather
and Research Forecasting (WRF) model is used to generate the meteorological
fields and the Model of Emissions of Gases and Aerosols from Nature (MEGAN)
is used for biogenic emissions. The results of the study are compared to
measurements from a field campaign conducted in the suburb of Beirut during
2–18 July 2011. The model reproduces satisfactorily the concentrations of
most gaseous pollutants, the total mass of PM&lt;sub&gt;2.5&lt;/sub&gt; as well as PM&lt;sub&gt;2.5&lt;/sub&gt;
elemental carbon (EC), organic carbon (OC), and sulfate. Ozone
concentrations are overestimated and it appears that this overestimation
results mainly from the boundary conditions.</description><pubDate>Mon, 17 Jun 2013 00:00:00 +0200</pubDate></item><item><title>Formation of aqueous-phase α-hydroxyhydroperoxides (α-HHP): potential atmospheric impacts</title><link>http://www.atmos-chem-phys.net/13/5857/2013/</link><description>&lt;b&gt;Formation of aqueous-phase α-hydroxyhydroperoxides (α-HHP): potential atmospheric impacts&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Chemistry and Physics, 13, 5857-5872, 2013&lt;br /&gt;&lt;br /&gt;Author(s): R. Zhao, A. K. Y. Lee, R. Soong, A. J. Simpson, and J. P. D. Abbatt&lt;br /&gt;&lt;br /&gt;The focus of this work is on quantifying the degree of the aqueous-phase
formation of α-hydroxyhydroperoxides (α-HHPs) via reversible
nucleophilic addition of H&lt;sub&gt;2&lt;/sub&gt;O&lt;sub&gt;2&lt;/sub&gt; to aldehydes. Formation of this
class of highly oxygenated organic hydroperoxides represents a poorly
characterized aqueous-phase processing pathway that may lead to enhanced SOA
formation and aerosol toxicity. Specifically, the equilibrium constants of
α-HHP formation have been determined using proton nuclear-magnetic-resonance
(&lt;sup&gt;1&lt;/sup&gt;H NMR) spectroscopy and proton-transfer-reaction mass spectrometry
(PTR-MS). Significant α-HHP formation was observed from
formaldehyde, acetaldehyde, propionaldehyde, glycolaldehyde, glyoxylic acid,
and methylglyoxal, but not from methacrolein and ketones. Low temperatures
enhanced the formation of α-HHPs but slowed their formation rates.
High inorganic salt concentrations shifted the equilibria toward the
hydrated form of the aldehydes and slightly suppressed α-HHP
formation. Using the experimental equilibrium constants, we predict the
equilibrium concentration of α-HHPs to be in the μM level in
cloud water, but it may also be present in the mM level in aerosol liquid water
(ALW), where the concentrations of H&lt;sub&gt;2&lt;/sub&gt;O&lt;sub&gt;2&lt;/sub&gt; and aldehydes can be high.
Formation of α-HHPs in ALW may significantly affect the effective
Henry's law constants of H&lt;sub&gt;2&lt;/sub&gt;O&lt;sub&gt;2&lt;/sub&gt; and aldehydes but may not affect
their gas-phase levels. The photochemistry and reactivity of this class of
atmospheric species have not been studied.</description><pubDate>Mon, 17 Jun 2013 00:00:00 +0200</pubDate></item><item><title>Black carbon physical properties and mixing state in the European megacity Paris</title><link>http://www.atmos-chem-phys.net/13/5831/2013/</link><description>&lt;b&gt;Black carbon physical properties and mixing state in the European megacity Paris&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Chemistry and Physics, 13, 5831-5856, 2013&lt;br /&gt;&lt;br /&gt;Author(s): M. Laborde, M. Crippa, T. Tritscher, Z. Jurányi, P. F. Decarlo, B. Temime-Roussel, N. Marchand, S. Eckhardt, A. Stohl, U. Baltensperger, A. S. H. Prévôt, E. Weingartner, and M. Gysel&lt;br /&gt;&lt;br /&gt;Aerosol hygroscopicity and refractory black carbon (rBC) properties were
characterised during wintertime at a suburban site in Paris, one of the
biggest European cities. Hygroscopic growth factor (GF) frequency
distributions, characterised by distinct modes of more-hygroscopic background
aerosol and non- or slightly hygroscopic aerosol of local (or regional)
origin, revealed an increase of the relative contribution of the local
sources compared to the background aerosol with decreasing particle size.
BC-containing particles in Paris were mainly originating from fresh traffic
emissions, whereas biomass burning only gave a minor contribution. The mass
size distribution of the rBC cores peaked on average at an rBC core mass
equivalent diameter of &lt;i&gt;D&lt;/i&gt;&lt;sub&gt;MEV&lt;/sub&gt; ~ 150 nm. The
BC-containing particles were moderately coated (coating thickness
&amp;Delta;&lt;sub&gt;coat&lt;/sub&gt; ~ 33 nm on average for rBC cores with
&lt;/i&gt;D&lt;/i&gt;&lt;sub&gt;MEV&lt;/sub&gt; = 180–280 nm) and an average mass absorption
coefficient (MAC) of ~ 8.6 m&lt;sup&gt;2&lt;/sup&gt; g&lt;sup&gt;&amp;minus;1&lt;/sup&gt; at the
wavelength λ = 880 nm was observed.
&lt;br&gt;&lt;br&gt;
Different time periods were selected to investigate the properties of
BC-containing particles as a function of source and air mass type. The
traffic emissions were found to be non-hygroscopic (GF ≈ 1.0), and
essentially all particles with a dry mobility diameter (&lt;i&gt;D&lt;/i&gt;&lt;sub&gt;0&lt;/sub&gt;) larger than
&lt;i&gt;D&lt;/i&gt;&lt;sub&gt;0&lt;/sub&gt; = 110 nm contained an rBC core. rBC from traffic emissions
was further observed to be uncoated within experimental uncertainty
(&amp;Delta;&lt;sub&gt;coat&lt;/sub&gt; ~ 2 nm ± 10 nm), to have
the smallest BC core sizes (maximum of the rBC core mass size distribution
at &lt;i&gt;D&lt;/i&gt;&lt;sub&gt;MEV&lt;/sub&gt; ~ 100 nm) and to have the smallest MAC
(~ 7.3 m&lt;sup&gt;2&lt;/sup&gt;g&lt;sup&gt;&amp;minus;1&lt;/sup&gt; at λ = 880 nm).

&lt;br&gt;&lt;br&gt;

The biomass burning aerosol was slightly more hygroscopic than the traffic
emissions (with a distinct slightly-hygroscopic mode peaking at
GF ≈ 1.1–1.2). Furthermore, only a minor fraction
(&amp;leq; 10%) of the slightly-hygroscopic particles with
1.1 &amp;leq; GF &amp;leq; 1.2 (and &lt;i&gt;D&lt;/i&gt;&lt;sub&gt;0&lt;/sub&gt; = 265 nm) contained
a detectable rBC core. The BC-containing particles from biomass burning were
found to have a medium coating thickness as well as slightly larger mean rBC
core sizes and MAC values compared to traffic emissions.
&lt;br&gt;&lt;br&gt;
The aerosol observed under the influence of aged air masses and air masses
from Eastern Continental Europe was dominated by a~more-hygroscopic mode
peaking at GF ≈ 1.6. Most particles (95%), in the
more-hygroscopic mode at &lt;i&gt;D&lt;/i&gt;&lt;sub&gt;0&lt;/sub&gt; = 265 nm, did not contain a
detectable rBC core. A significant fraction of the BC-containing particles
had a substantial coating with non-refractory aerosol components. MAC values
of ~ 8.8 m&lt;sup&gt;2&lt;/sup&gt;g&lt;sup&gt;&amp;minus;1&lt;/sup&gt; and
~ 8.3 m&lt;sup&gt;2&lt;/sup&gt;g&lt;sup&gt;&amp;minus;1&lt;/sup&gt; at λ = 880 nm and
mass mean rBC core diameters of 150 nm and 200 nm were
observed for the aged and continental air mass types, respectively. The
reason for the larger rBC core sizes compared to the fresh emissions –
transport effects or a different rBC source – remains unclear.
&lt;br&gt;&lt;br&gt;
The dominant fraction of the BC-containing particles was found to have no or
very little coating with non-refractory matter. The lack of coatings is
consistent with the observation that the BC-containing particles are non- or
slightly-hygroscopic, which makes them poor cloud condensation nuclei. It can
therefore be expected that wet removal through nucleation scavenging is
inefficient for fresh BC-containing particles in urban plumes. The
mixing-state-specific cloud droplet activation behaviour of BC-containing
particles including the effects of atmospheric aging processes should be
considered in global simulations of atmospheric BC, as the wet removal
efficiency remains a major source of uncertainty in its life-cycle.</description><pubDate>Fri, 14 Jun 2013 00:00:00 +0200</pubDate></item><item><title>Ozone and fine particle in the western Yangtze River Delta: an overview of 1 yr data at the SORPES station</title><link>http://www.atmos-chem-phys.net/13/5813/2013/</link><description>&lt;b&gt;Ozone and fine particle in the western Yangtze River Delta: an overview of 1 yr data at the SORPES station&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Chemistry and Physics, 13, 5813-5830, 2013&lt;br /&gt;&lt;br /&gt;Author(s): A. J. Ding, C. B. Fu, X. Q. Yang, J. N. Sun, L. F. Zheng, Y. N. Xie, E. Herrmann, W. Nie, T. Petäjä, V.-M. Kerminen, and M. Kulmala&lt;br /&gt;&lt;br /&gt;This work presents an overview of 1 yr measurements of ozone (O&lt;sub&gt;3&lt;/sub&gt;) and
fine particular matter (PM&lt;sub&gt;2.5&lt;/sub&gt;) and related trace gases at a recently
developed regional background site, the Station for Observing Regional
Processes of the Earth System (SORPES), in the western part of the Yangtze
River Delta (YRD) in eastern China. Ozone and PM&lt;sub&gt;2.5&lt;/sub&gt; showed strong seasonal
cycles but with contrast patterns: O&lt;sub&gt;3&lt;/sub&gt; reached a maximum in warm seasons
but PM&lt;sub&gt;2.5&lt;/sub&gt; in cold seasons. Correlation analysis suggests a
VOC-sensitive regime for O&lt;sub&gt;3&lt;/sub&gt; chemistry and a formation of secondary
aerosols under conditions of high O&lt;sub&gt;3&lt;/sub&gt; in summer. Compared with the
National Ambient Air Quality Standards in China, our measurements report 15
days of O&lt;sub&gt;3&lt;/sub&gt; exceedance and 148 days of PM&lt;sub&gt;2.5&lt;/sub&gt; exceedance during the
1 yr period, suggesting a severe air pollution situation in this region.
Case studies for typical O&lt;sub&gt;3&lt;/sub&gt; and PM&lt;sub&gt;2.5&lt;/sub&gt; episodes demonstrated that
these episodes were generally associated with an air mass transport pathway
over the mid-YRD, i.e.,  along the Nanjing–Shanghai axis with its city
clusters, and showed that synoptic weather played an important role in air
pollution, especially for O&lt;sub&gt;3&lt;/sub&gt;. Agricultural burning activities caused
high PM&lt;sub&gt;2.5&lt;/sub&gt; and O&lt;sub&gt;3&lt;/sub&gt; pollution during harvest seasons, especially in
June. A calculation of potential source contributions based on Lagrangian
dispersion simulations suggests that emissions from the YRD contributed to
over 70% of the O&lt;sub&gt;3&lt;/sub&gt; precursor CO, with a majority from the mid-YRD.
North-YRD and the North China Plain are the main contributors to PM&lt;sub&gt;2.5&lt;/sub&gt;
pollution in this region. This work shows an important environmental impact
from industrialization and urbanization in the YRD region, and suggests an
urgent need for improving air quality in these areas through collaborative
control measures among different administrative regions.</description><pubDate>Fri, 14 Jun 2013 00:00:00 +0200</pubDate></item><item><title>Validation of MIPAS-ENVISAT H&lt;sub&gt;2&lt;/sub&gt;O operational data collected between July 2002 and March 2004</title><link>http://www.atmos-chem-phys.net/13/5791/2013/</link><description>&lt;b&gt;Validation of MIPAS-ENVISAT H&lt;sub&gt;2&lt;/sub&gt;O operational data collected between July 2002 and March 2004&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Chemistry and Physics, 13, 5791-5811, 2013&lt;br /&gt;&lt;br /&gt;Author(s): G. Wetzel, H. Oelhaf, G. Berthet, A. Bracher, C. Cornacchia, D. G. Feist, H. Fischer, A. Fix, M. Iarlori, A. Kleinert, A. Lengel, M. Milz, L. Mona, S. C. Müller, J. Ovarlez, G. Pappalardo, C. Piccolo, P. Raspollini, J.-B. Renard, V. Rizi, S. Rohs, C. Schiller, G. Stiller, M. Weber, and G. Zhang&lt;br /&gt;&lt;br /&gt;Water vapour (H&lt;sub&gt;2&lt;/sub&gt;O) is one of the operationally retrieved key species of
the Michelson Interferometer for Passive Atmospheric Sounding (MIPAS)
instrument aboard the Environmental Satellite (ENVISAT) which was launched
into its sun-synchronous orbit on 1 March 2002 and operated until April
2012. Within the MIPAS validation activities, independent observations from
balloons, aircraft, satellites, and ground-based stations have been compared
to European Space Agency (ESA) version 4.61 operational H&lt;sub&gt;2&lt;/sub&gt;O data
comprising the time period from July 2002 until March 2004 where MIPAS
measured with full spectral resolution. No significant bias in the MIPAS
H&lt;sub&gt;2&lt;/sub&gt;O data is seen in the lower stratosphere (above the hygropause)
between about 15 and 30 km. Differences of H&lt;sub&gt;2&lt;/sub&gt;O quantities observed by
MIPAS and the validation instruments are mostly well within the combined
total errors in this altitude region. In the upper stratosphere (above about
30 km), a tendency towards a small positive bias (up to about 10%) is
present in the MIPAS data when compared to its balloon-borne counterpart
MIPAS-B, to the satellite instruments HALOE (Halogen Occultation Experiment)
and ACE-FTS (Atmospheric Chemistry Experiment, Fourier Transform
Spectrometer), and to the millimeter-wave airborne sensor AMSOS (Airborne Microwave
Stratospheric Observing System). In the mesosphere the situation is unclear
due to the occurrence of different biases when comparing HALOE and ACE-FTS
data. Pronounced deviations between MIPAS and the correlative instruments
occur in the lowermost stratosphere and upper troposphere, a region where
retrievals of H&lt;sub&gt;2&lt;/sub&gt;O are most challenging. Altogether it can be concluded
that MIPAS H&lt;sub&gt;2&lt;/sub&gt;O profiles yield valuable information on the vertical
distribution of H&lt;sub&gt;2&lt;/sub&gt;O in the stratosphere with an overall accuracy of
about 10 to 30% and a precision of typically 5 to 15% – well within
the predicted error budget, showing that these global and continuous data
are very valuable for scientific studies. However, in the region around the
tropopause retrieved MIPAS H&lt;sub&gt;2&lt;/sub&gt;O profiles are less reliable, suffering
from a number of obstacles such as retrieval boundary and cloud effects,
sharp vertical discontinuities, and frequent horizontal gradients in both
temperature and H&lt;sub&gt;2&lt;/sub&gt;O volume mixing ratio (VMR). Some profiles are
characterized by retrieval instabilities.</description><pubDate>Fri, 14 Jun 2013 00:00:00 +0200</pubDate></item><item><title>Formation of organic aerosol in the Paris region during the MEGAPOLI summer campaign: evaluation of the volatility-basis-set approach within the CHIMERE model</title><link>http://www.atmos-chem-phys.net/13/5767/2013/</link><description>&lt;b&gt;Formation of organic aerosol in the Paris region during the MEGAPOLI summer campaign: evaluation of the volatility-basis-set approach within the CHIMERE model&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Chemistry and Physics, 13, 5767-5790, 2013&lt;br /&gt;&lt;br /&gt;Author(s): Q. J. Zhang, M. Beekmann, F. Drewnick, F. Freutel, J. Schneider, M. Crippa, A. S. H. Prevot, U. Baltensperger, L. Poulain, A. Wiedensohler, J. Sciare, V. Gros, A. Borbon, A. Colomb, V. Michoud, J.-F. Doussin, H. A. C. Denier van der Gon, M. Haeffelin, J.-C. Dupont, G. Siour, H. Petetin, B. Bessagnet, S. N. Pandis, A. Hodzic, O. Sanchez, C. Honoré, and O. Perrussel&lt;br /&gt;&lt;br /&gt;Simulations with the chemistry transport model CHIMERE
are compared to measurements performed during the MEGAPOLI 
(Megacities: Emissions, urban, regional and Global Atmospheric
POLlution and climate effects, and Integrated tools for assessment and
mitigation) summer campaign
in the Greater Paris region in July 2009. The volatility-basis-set approach
(VBS) is implemented into this model, taking into account the volatility of
primary organic aerosol (POA) and the chemical aging of semi-volatile
organic species. Organic aerosol is the main focus and is simulated with
three different configurations with a modified treatment of POA volatility
and modified secondary organic aerosol (SOA) formation schemes. In addition,
two types of emission inventories are used as model input in order to test
the uncertainty related to the emissions. Predictions of basic
meteorological parameters and primary and secondary pollutant concentrations
are evaluated, and four pollution regimes are defined according to the air mass
origin. Primary pollutants are generally overestimated, while ozone is
consistent with observations. Sulfate is generally overestimated, while
ammonium and nitrate levels are well simulated with the refined emission
data set. As expected, the simulation with non-volatile POA and a
single-step SOA formation mechanism largely overestimates POA and
underestimates SOA. Simulation of organic aerosol with the VBS approach
taking into account the aging of semi-volatile organic compounds (SVOC)
shows the best correlation with measurements. High-concentration events
observed mostly after long-range transport are well reproduced by the model.
Depending on the emission inventory used, simulated POA levels are either
reasonable or underestimated, while SOA levels tend to be overestimated.
Several uncertainties related to the VBS scheme (POA volatility, SOA yields,
the aging parameterization), to emission input data, and to simulated OH
levels can be responsible for this behavior. Despite these uncertainties,
the implementation of the VBS scheme into the CHIMERE model allowed for much
more realistic organic aerosol simulations for Paris during summertime. The
advection of SOA from outside Paris is mostly responsible for the highest OA
concentration levels. During advection of polluted air masses from
northeast (Benelux and Central Europe), simulations indicate high levels of
both anthropogenic and biogenic SOA fractions, while biogenic SOA dominates
during periods with advection from Southern France and Spain.</description><pubDate>Fri, 14 Jun 2013 00:00:00 +0200</pubDate></item><item><title>Immersion freezing of ice nucleation active protein complexes</title><link>http://www.atmos-chem-phys.net/13/5751/2013/</link><description>&lt;b&gt;Immersion freezing of ice nucleation active protein complexes&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Chemistry and Physics, 13, 5751-5766, 2013&lt;br /&gt;&lt;br /&gt;Author(s): S. Hartmann, S. Augustin, T. Clauss, H. Wex, T. Šantl-Temkiv, J. Voigtländer, D. Niedermeier, and F. Stratmann&lt;br /&gt;&lt;br /&gt;Utilising the Leipzig Aerosol Cloud Interaction Simulator (LACIS), the
immersion freezing behaviour of droplet ensembles containing monodisperse
particles, generated from a Snomax™ solution/suspension, was
investigated. Thereto ice fractions were measured in the temperature range
between −5 °C to −38 °C. Snomax™ is an
industrial product applied for artificial snow production and contains
&lt;i&gt;Pseudomonas&lt;/i&gt; syringae} bacteria which have long been used as model
organism for atmospheric relevant ice nucleation active (INA) bacteria. The
ice nucleation activity of such bacteria is controlled by INA protein
complexes in their outer membrane.
&lt;br&gt;&lt;br&gt;
In our experiments, ice fractions increased steeply in the temperature range
from about −6 °C to about −10 °C and then levelled
off at ice fractions smaller than one. The plateau implies that not all
examined droplets contained an INA protein complex. Assuming the INA protein
complexes to be Poisson distributed over the investigated droplet
populations, we developed the CHESS model (stoCHastic modEl of similar and
poiSSon distributed ice nuclei) which allows for the calculation of ice
fractions as function of temperature and time for a given nucleation rate.
Matching calculated and measured ice fractions, we determined and
parameterised the nucleation rate of INA protein complexes exhibiting class
III ice nucleation behaviour. Utilising the CHESS model, together with the
determined nucleation rate, we compared predictions from the model to
experimental data from the literature and found good agreement.
&lt;br&gt;&lt;br&gt;
We found that (a) the heterogeneous ice nucleation rate expression
quantifying the ice nucleation behaviour of the INA protein complex is
capable of describing the ice nucleation behaviour observed in various
experiments for both, Snomax™ and &lt;i&gt;P. syringae&lt;/i&gt; bacteria,
(b) the ice nucleation rate, and its temperature dependence, seem to be very
similar regardless of whether the INA protein complexes inducing ice
nucleation are attached to the outer membrane of intact bacteria or membrane
fragments, (c) the temperature range in which heterogeneous droplet freezing
occurs, and the fraction of droplets being able to freeze, both depend on the
actual number of INA protein complexes present in the droplet ensemble, and
(d) possible artifacts suspected to occur in connection with the drop
freezing method, i.e., the method frequently used by biologist for
quantifying ice nucleation behaviour, are of minor importance, at least for
substances such as &lt;i&gt;P. syringae&lt;/i&gt;, which induce freezing at comparably
high temperatures. The last statement implies that for single ice nucleation
entities such as INA protein complexes, it is the number of entities present
in the droplet population, and the entities' nucleation rate, which control
the freezing behaviour of the droplet population. Quantities such as ice
active surface site density are not suitable in this context.
&lt;br&gt;&lt;br&gt;
The results obtained in this study allow a different perspective on the
quantification of the immersion freezing behaviour of bacterial ice
nucleation.</description><pubDate>Fri, 14 Jun 2013 00:00:00 +0200</pubDate></item><item><title>Diel peroxy radicals in a semi-industrial coastal area: nighttime formation of free radicals</title><link>http://www.atmos-chem-phys.net/13/5731/2013/</link><description>&lt;b&gt;Diel peroxy radicals in a semi-industrial coastal area: nighttime formation of free radicals&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Chemistry and Physics, 13, 5731-5749, 2013&lt;br /&gt;&lt;br /&gt;Author(s): M. D. Andrés-Hernández, D. Kartal, J. N. Crowley, V. Sinha, E. Regelin, M. Martínez-Harder, V. Nenakhov, J. Williams, H. Harder, H. Bozem, W. Song, J. Thieser, M. J. Tang, Z. Hosaynali Beigi, and J. P. Burrows&lt;br /&gt;&lt;br /&gt;Peroxy radicals were measured by a PeRCA (Peroxy Radical Chemical Amplifier)
instrument in the boundary layer during the DOMINO (Diel Oxidant Mechanisms
In relation to Nitrogen Oxides) campaign at a coastal, forested site
influenced by urban-industrial emissions in southern Spain in late autumn.
Total peroxy radicals (RO&lt;sub&gt;2&lt;/sub&gt;* = HO&lt;sub&gt;2&lt;/sub&gt; + &amp;Sigma;RO&lt;sub&gt;2&lt;/sub&gt;)
generally showed a daylight maximum between 10 and 50 pptv at 13:00 UTC,
with an average of 18 pptv over the 15 days of measurements. Emissions from
the industrial area of Huelva often impacted the measurement site at night
during the campaign. The processing of significant levels of anthropogenic
organics leads to an intense nocturnal radical chemistry accompanied by
formation of organic peroxy radicals at comparable levels to those of summer
photochemical conditions with peak events up to 60–80 pptv. The RO&lt;sub&gt;2&lt;/sub&gt;
production initiated by reactions of NO&lt;sub&gt;3&lt;/sub&gt; with organic trace gases was
estimated to be significant, but not sufficient to account for the
concentrations of RO&lt;sub&gt;2&lt;/sub&gt;* observed in air masses carrying high
pollutant loading. The nocturnal production of peroxy radicals in those
periods seems therefore to be dominated by ozonolysis of volatile organic
compounds, in particular alkenes of industrial petrochemical origin.
&lt;br&gt;&lt;br&gt;
RO&lt;sub&gt;2&lt;/sub&gt;* diurnal variations were consistent with HO&lt;sub&gt;2&lt;/sub&gt;
measurements available at the site. HO&lt;sub&gt;2&lt;/sub&gt;/RO&lt;sub&gt;2&lt;/sub&gt;* ratios
generally varied between 0.3 and 0.6, though on some occasions this ratio
was likely to have been affected by instrumental artifacts (overestimated
HO&lt;sub&gt;2&lt;/sub&gt;) associated with high RO&lt;sub&gt;2&lt;/sub&gt; loads.</description><pubDate>Fri, 14 Jun 2013 00:00:00 +0200</pubDate></item><item><title>Production of methyl vinyl ketone and methacrolein via the hydroperoxyl pathway of isoprene oxidation</title><link>http://www.atmos-chem-phys.net/13/5715/2013/</link><description>&lt;b&gt;Production of methyl vinyl ketone and methacrolein via the hydroperoxyl pathway of isoprene oxidation&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Chemistry and Physics, 13, 5715-5730, 2013&lt;br /&gt;&lt;br /&gt;Author(s): Y. J. Liu, I. Herdlinger-Blatt, K. A. McKinney, and S. T. Martin&lt;br /&gt;&lt;br /&gt;The photo-oxidation chemistry of isoprene (ISOP; C&lt;sub&gt;5&lt;/sub&gt;H&lt;sub&gt;8&lt;/sub&gt;) was studied
in a continuous-flow chamber under conditions such that the reactions of the
isoprene-derived peroxyl radicals (RO&lt;sub&gt;2&lt;/sub&gt;) were dominated by the
hydroperoxyl (HO&lt;sub&gt;2&lt;/sub&gt;) pathway. A proton-transfer-reaction time-of-flight
mass spectrometer (PTR-TOF-MS) with switchable H&lt;sub&gt;3&lt;/sub&gt;O&lt;sup&gt;+&lt;/sup&gt; and NO&lt;sup&gt;+&lt;/sup&gt;
reagent ions was used for product analysis. The products methyl vinyl ketone
(MVK; C&lt;sub&gt;4&lt;/sub&gt;H&lt;sub&gt;6&lt;/sub&gt;O) and methacrolein (MACR; C&lt;sub&gt;4&lt;/sub&gt;H&lt;sub&gt;6&lt;/sub&gt;O) were
differentiated using NO&lt;sup&gt;+&lt;/sup&gt; reagent ions. The MVK and MACR yields via the
HO&lt;sub&gt;2&lt;/sub&gt; pathway were (3.8 ± 1.3)% and (2.5 ± 0.9)%,
respectively, at +25 &amp;deg;C and &lt; 2% relative humidity. The
respective yields were (41.4 ± 5.5)% and (29.6 ± 4.2)%
via the NO pathway. Production of MVK and MACR via the HO&lt;sub&gt;2&lt;/sub&gt; pathway
implies concomitant production of hydroxyl ((6.3 ± 2.1)%) and
hydroperoxyl ((6.3 ± 2.1)%) radicals, meaning a HO&lt;sub&gt;x&lt;/sub&gt;
recycling of (12.6 ± 4.2)% given that HO&lt;sub&gt;2&lt;/sub&gt; was both a reactant
and product. Other isoprene oxidation products, believed to be mostly organic
hydroperoxides, also contributed to the ion intensity at the same
mass-to-charge (&lt;i&gt;m/z&lt;/i&gt;) ratios as the MVK and MACR product ions for
HO&lt;sub&gt;2&lt;/sub&gt;-dominant conditions. These products were selectively removed from
the gas phase by placement of a cold trap (−40 &amp;deg;C) inline prior to
the PTR-TOF-MS. When incorporated into regional and global chemical transport
models, the yields of MVK and MACR and the concomitant HO&lt;sub&gt;x&lt;/sub&gt;
recycling reported in this study can improve the accuracy of the simulation
of the HO&lt;sub&gt;2&lt;/sub&gt; reaction pathway of isoprene, which is believed to be the
fate of approximately half of atmospherically produced isoprene-derived
peroxy radicals on a global scale.</description><pubDate>Fri, 14 Jun 2013 00:00:00 +0200</pubDate></item><item><title>Estimating regional methane surface fluxes: the relative importance of surface and GOSAT mole fraction measurements</title><link>http://www.atmos-chem-phys.net/13/5697/2013/</link><description>&lt;b&gt;Estimating regional methane surface fluxes: the relative importance of surface and GOSAT mole fraction measurements&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Chemistry and Physics, 13, 5697-5713, 2013&lt;br /&gt;&lt;br /&gt;Author(s): A. Fraser, P. I. Palmer, L. Feng, H. Boesch, A. Cogan, R. Parker, E. J. Dlugokencky, P. J. Fraser, P. B. Krummel, R. L. Langenfelds, S. O'Doherty, R. G. Prinn, L. P. Steele, M. van der Schoot, and R. F. Weiss&lt;br /&gt;&lt;br /&gt;We use an ensemble Kalman filter (EnKF), together with the GEOS-Chem
chemistry transport model, to estimate regional monthly methane (CH&lt;sub&gt;4&lt;/sub&gt;)
fluxes for the period June 2009–December 2010 using proxy dry-air
column-averaged mole fractions of methane (XCH&lt;sub&gt;4&lt;/sub&gt;) from GOSAT (Greenhouse
gases Observing SATellite) and/or NOAA ESRL (Earth System Research
Laboratory) and CSIRO GASLAB (Global Atmospheric Sampling Laboratory) CH&lt;sub&gt;4&lt;/sub&gt;
surface mole fraction measurements. Global posterior estimates using GOSAT
and/or surface measurements are between 510–516 Tg yr&lt;sup&gt;−1&lt;/sup&gt;, which is
less than, though within the uncertainty of, the prior global flux of
529 ± 25 Tg yr&lt;sup&gt;−1&lt;/sup&gt;. We find larger differences between regional
prior and posterior fluxes, with the largest changes in monthly emissions
(75 Tg yr&lt;sup&gt;−1&lt;/sup&gt;) occurring in Temperate Eurasia. In non-boreal regions the
error reductions for inversions using the GOSAT data are at least three times
larger (up to 45%) than if only surface data are assimilated, a reflection
of the greater spatial coverage of GOSAT, with the two exceptions of
latitudes &gt;60° associated with a data filter and over Europe
where the surface network adequately describes fluxes on our model spatial
and temporal grid. We use CarbonTracker and GEOS-Chem XCO&lt;sub&gt;2&lt;/sub&gt; model output to
investigate model error on quantifying proxy GOSAT XCH&lt;sub&gt;4&lt;/sub&gt; (involving model
XCO&lt;sub&gt;2&lt;/sub&gt;) and inferring methane flux estimates from surface mole fraction data
and show similar resulting fluxes, with differences reflecting initial
differences in the proxy value. Using a series of observing system simulation
experiments (OSSEs) we characterize the posterior flux error introduced by
non-uniform atmospheric sampling by GOSAT. We show that clear-sky
measurements can theoretically reproduce fluxes within 10% of true
values, with the exception of tropical regions where, due to a large seasonal
cycle in the number of measurements because of clouds and aerosols, fluxes
are within 15% of true fluxes. We evaluate our posterior methane
fluxes by incorporating them into GEOS-Chem and sampling the model at the
location and time of surface CH&lt;sub&gt;4&lt;/sub&gt; measurements from the AGAGE (Advanced
Global Atmospheric Gases Experiment) network and column XCH&lt;sub&gt;4&lt;/sub&gt; measurements
from TCCON (Total Carbon Column Observing Network). The posterior fluxes
modestly improve the model agreement with AGAGE and TCCON data relative to
prior fluxes, with the correlation coefficients (&lt;i&gt;r&lt;/i&gt;&lt;sup&gt;2&lt;/sup&gt;) increasing by a mean
of 0.04 (range: −0.17 to 0.23) and the biases decreasing by a mean of
0.4 ppb (range: −8.9 to 8.4 ppb).</description><pubDate>Thu, 13 Jun 2013 00:00:00 +0200</pubDate></item><item><title>Analysis of a winter regional haze event and its formation mechanism in the North China Plain</title><link>http://www.atmos-chem-phys.net/13/5685/2013/</link><description>&lt;b&gt;Analysis of a winter regional haze event and its formation mechanism in the North China Plain&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Chemistry and Physics, 13, 5685-5696, 2013&lt;br /&gt;&lt;br /&gt;Author(s): X. J. Zhao, P. S. Zhao, J. Xu, W. Meng,, W. W. Pu, F. Dong, D. He, and Q. F. Shi&lt;br /&gt;&lt;br /&gt;A regional haze episode occurred in the Beijing, Tianjin and Hebei province
(BTH) area in the North China Plain (NCP) from 16 to 19 January 2010. Data
were collected and analyzed during the time frame of 14 through 23 January
2010 to include the haze event. The increase of secondary inorganic
pollutants (SO&lt;sub&gt;4&lt;/sub&gt;&lt;sup&gt;2&amp;minus;&lt;/sup&gt;, NO&lt;sub&gt;3&lt;/sub&gt;&lt;sup&gt;&amp;minus;&lt;/sup&gt;, NH&lt;sub&gt;4&lt;/sub&gt;&lt;sup&gt;+&lt;/sup&gt;) in PM&lt;sub&gt;2.5&lt;/sub&gt;
was observed simultaneously at four sites, especially in the plain area of
the BTH, which could be identified as a common characteristic of pollution haze
in east China. The sulfate and nitrate in PM&lt;sub&gt;2.5&lt;/sub&gt; were mainly formed
through the heterogeneous reaction process in the urban area. The organic
matter (OM) increased more significantly at the Chengde (CD) site than the other
three sites in the plain area. The secondary organic aerosols only existed
during haze days at CD but in both haze and non-haze days at the other three
sites, which suggested the greater regional impact of secondary formation
process during the haze episode. The secondary formation of aerosol was one
important formation mechanism of haze. The strong temperature inversion and
descending air motions in the planetary boundary layer (PBL) allowed
pollutants to accumulate in a shallow layer. The weak surface wind speed
produced high pollutants concentration within source regions. The
accumulation of pollutants was one main factor in the haze formation. The
enhanced southwest wind in the last period of this episode transported
pollutants to the downwind area and expanded the regional scope of the haze.</description><pubDate>Thu, 13 Jun 2013 00:00:00 +0200</pubDate></item><item><title>Newly observed peroxides and the water effect on the formation and removal of hydroxyalkyl hydroperoxides in the ozonolysis of isoprene</title><link>http://www.atmos-chem-phys.net/13/5671/2013/</link><description>&lt;b&gt;Newly observed peroxides and the water effect on the formation and removal of hydroxyalkyl hydroperoxides in the ozonolysis of isoprene&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Chemistry and Physics, 13, 5671-5683, 2013&lt;br /&gt;&lt;br /&gt;Author(s): D. Huang, Z. M. Chen, Y. Zhao, and H. Liang&lt;br /&gt;&lt;br /&gt;The ozonolysis of alkenes is considered to be an
important source of atmospheric peroxides, which serve as oxidants,
reservoirs of HO&lt;sub&gt;x&lt;/sub&gt; radicals, and components of secondary organic
aerosols (SOAs). Recent laboratory investigations of this reaction
identified hydrogen peroxide (H&lt;sub&gt;2&lt;/sub&gt;O&lt;sub&gt;2&lt;/sub&gt;) and hydroxymethyl
hydroperoxide (HMHP) in ozonolysis of isoprene. Although larger hydroxyalkyl
hydroperoxides (HAHPs) were also expected, their presence is not currently
supported by experimental evidence. In the present study, we investigated
the formation of peroxides in the gas phase ozonolysis of isoprene at
various relative humidities on a time scale of tens of seconds, using a
quartz flow tube reactor coupled with the online detection of peroxides. We
detected a variety of conventional peroxides, including H&lt;sub&gt;2&lt;/sub&gt;O&lt;sub&gt;2&lt;/sub&gt;,
HMHP, methyl hydroperoxide, bis-hydroxymethyl hydroperoxide, and ethyl
hydroperoxide, and interestingly found three unknown peroxides. The molar
yields of the conventional peroxides fell within the range of values
provided in the literature. The three unknown peroxides had a combined molar
yield of ~ 30% at 5% relative humidity (RH), which was
comparable with that of the conventional peroxides. Unlike H&lt;sub&gt;2&lt;/sub&gt;O&lt;sub&gt;2&lt;/sub&gt;
and HMHP, the molar yields of these three unknown peroxides were inversely
related to the RH. On the basis of experimental kinetic and box model
analysis, we tentatively assigned these unknown peroxides to C2−C4 HAHPs,
which are produced by the reactions of different Criegee intermediates with
water. Our study provides experimental evidence for the formation of large
HAHPs in the ozonolysis of isoprene (one of the alkenes). These large HAHPs
have a sufficiently long lifetime, estimated as tens of minutes, which
allows them to become involved in atmospheric chemical processes, e.g., SOA
formation and radical recycling.</description><pubDate>Wed, 12 Jun 2013 00:00:00 +0200</pubDate></item><item><title>Megacity impacts on regional ozone formation: observations and WRF-Chem modeling for the MIRAGE-Shanghai field campaign</title><link>http://www.atmos-chem-phys.net/13/5655/2013/</link><description>&lt;b&gt;Megacity impacts on regional ozone formation: observations and WRF-Chem modeling for the MIRAGE-Shanghai field campaign&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Chemistry and Physics, 13, 5655-5669, 2013&lt;br /&gt;&lt;br /&gt;Author(s): X. Tie, F. Geng, A. Guenther, J. Cao, J. Greenberg, R. Zhang, E. Apel, G. Li, A. Weinheimer, J. Chen, and C. Cai&lt;br /&gt;&lt;br /&gt;The MIRAGE-Shanghai experiment was designed to characterize the factors
controlling regional air pollution near a Chinese megacity (Shanghai) and was
conducted during September 2009. This paper provides information on the
measurements conducted for this study. In order to have some deep analysis of
the measurements, a regional chemical/dynamical model (version 3 of Weather
Research and Forecasting Chemical model – WRF-Chemv3) is applied for this
study. The model results are intensively compared with the measurements to
evaluate the model capability for calculating air pollutants in the Shanghai
region, especially the chemical species related to ozone formation. The
results show that the model is able to calculate the general distributions
(the level and the variability) of air pollutants in the Shanghai region, and
the differences between the model calculation and the measurement are mostly
smaller than 30%, except the calculations of HONO (nitrous acid) at PD
(Pudong) and CO (carbon monoxide) at DT (Dongtan).
&lt;br&gt;&lt;br&gt;
The main scientific focus is the study of ozone chemical formation not only
in the urban area, but also on a regional scale of the surrounding area of
Shanghai. The results show that during the experiment period, the ozone
photochemical formation was strongly under the VOC (volatile organic
compound)-limited condition in the urban area of Shanghai. Moreover, the
VOC-limited condition occurred not only in the city, but also in the larger
regional area. There was a continuous enhancement of ozone concentrations in
the downwind of the megacity of Shanghai, resulting in a significant
enhancement of ozone concentrations in a very large regional area in the
surrounding region of Shanghai. The sensitivity study of the model suggests
that there is a threshold value for switching from VOC-limited condition to
NO&lt;sub&gt;x&lt;/sub&gt; (nitric oxide and nitrogen dioxide)-limited condition. The
threshold value is strongly dependent on the emission ratio of NO&lt;sub&gt;x&lt;/sub&gt; / VOCs. 
When the ratio is about 0.4, the Shanghai region is under a
strong VOC-limited condition over the regional scale. In contrast, when the
ratio is reduced to about 0.1, the Shanghai region is under a strong
NO&lt;sub&gt;x&lt;/sub&gt;-limited condition. The estimated threshold value (on the
regional scale) for switching from VOC-limited to NO&lt;sub&gt;x&lt;/sub&gt;-limited
condition ranges from 0.1 to 0.2. This result has important implications for
ozone production in this region and will facilitate the development of
effective O&lt;sub&gt;3&lt;/sub&gt; control strategies in the Shanghai region.</description><pubDate>Mon, 10 Jun 2013 00:00:00 +0200</pubDate></item><item><title>Estimate of surface direct radiative forcing of desert dust from atmospheric modulation of the aerosol optical depth</title><link>http://www.atmos-chem-phys.net/13/5647/2013/</link><description>&lt;b&gt;Estimate of surface direct radiative forcing of desert dust from atmospheric modulation of the aerosol optical depth&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Chemistry and Physics, 13, 5647-5654, 2013&lt;br /&gt;&lt;br /&gt;Author(s): A. di Sarra, D. Fuà, and D. Meloni&lt;br /&gt;&lt;br /&gt;Measurements carried out on the island of Lampedusa, in the central
Mediterranean, on 7 September 2005, show the occurrence of a quasi-periodic
oscillation of aerosol optical depth, column water vapour, and surface
irradiance in different spectral bands. The oscillation has a period of
about 13 min and is attributed to the propagation of a gravity wave able
to modify the vertical structure of the planetary boundary layer, as also
confirmed by satellite images. The wave occurred during a Saharan dust
event. The oscillation amplitude is about 0.1 for the aerosol optical depth,
and about 0.4 cm for the column water vapour. The modulation of the downward
surface irradiances is in opposition of phase with respect to aerosol
optical depth and water vapour column variations. The perturbation of the
downward irradiance produced by the aerosols is determined by comparing the
measured irradiances with estimated irradiances at a fixed value of the
aerosol optical depth, and by correcting for the effect of the water vapour
in the shortwave spectral range. The direct radiative forcing efficiency,
i.e., the radiative perturbation of the net surface irradiance produced by a
unit of optical depth aerosol layer, is determined at different solar zenith
angles as the slope of the irradiance perturbation versus the aerosol
optical depth. The estimated direct surface forcing efficiency at about
60° solar zenith angle is −(181 ± 17) W m&lt;sup&gt;−2&lt;/sup&gt; in the
shortwave, and −(83 ± 7) W m&lt;sup&gt;−2&lt;/sup&gt; in the photosynthetic spectral
range. The estimated daily average forcing efficiencies are of about −79 and
−46 W m&lt;sup&gt;−2&lt;/sup&gt; for the shortwave and photosynthetic spectral range,
respectively.</description><pubDate>Mon, 10 Jun 2013 00:00:00 +0200</pubDate></item><item><title>Large-eddy simulation of organized precipitating trade wind cumulus clouds</title><link>http://www.atmos-chem-phys.net/13/5631/2013/</link><description>&lt;b&gt;Large-eddy simulation of organized precipitating trade wind cumulus clouds&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Chemistry and Physics, 13, 5631-5645, 2013&lt;br /&gt;&lt;br /&gt;Author(s): A. Seifert and T. Heus&lt;br /&gt;&lt;br /&gt;Trade wind cumulus clouds often organize in along-wind cloud streets and
across-wind mesoscale arcs. We present a benchmark large-eddy simulation
which resolves the individual clouds as well as the mesoscale organization on
scales of O(10 km). Different methods to quantify
organization of cloud fields are applied and discussed. Using perturbed
physics large-eddy simulation experiments, the processes leading to the
formation of cloud clusters and the mesoscale arcs are revealed. We find that
both cold pools as well as the sub-cloud layer moisture field are crucial to
understand the organization of precipitating shallow convection. Further
sensitivity studies show that microphysical assumptions can have a pronounced
impact on the onset of cloud organization.</description><pubDate>Mon, 10 Jun 2013 00:00:00 +0200</pubDate></item><item><title>Corrigendum to &quot;Tropospheric NO&lt;sub&gt;2&lt;/sub&gt; vertical column densities over Beijing: results of the first three years of ground-based MAX-DOAS measurements (2008–2011) and satellite validation&quot; published in Atmos. Chem. Phys., 13, 1547&amp;ndash;1567, 2013</title><link>http://www.atmos-chem-phys.net/13/5629/2013/</link><description>&lt;b&gt;Corrigendum to &quot;Tropospheric NO&lt;sub&gt;2&lt;/sub&gt; vertical column densities over Beijing: results of the first three years of ground-based MAX-DOAS measurements (2008–2011) and satellite validation&quot; published in Atmos. Chem. Phys., 13, 1547&amp;ndash;1567, 2013&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Chemistry and Physics, 13, 5629-5629, 2013&lt;br /&gt;&lt;br /&gt;Author(s): J. Z. Ma, S. Beirle, J. L. Jin, R. Shaiganfar, P. Yan, and T. Wagner&lt;br /&gt;&lt;br /&gt;No abstract available.</description><pubDate>Mon, 10 Jun 2013 00:00:00 +0200</pubDate></item><item><title>State transformations and ice nucleation in amorphous (semi-)solid organic aerosol</title><link>http://www.atmos-chem-phys.net/13/5615/2013/</link><description>&lt;b&gt;State transformations and ice nucleation in amorphous (semi-)solid organic aerosol&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Chemistry and Physics, 13, 5615-5628, 2013&lt;br /&gt;&lt;br /&gt;Author(s): K. J. Baustian, M. E. Wise, E. J. Jensen, G. P. Schill, M. A. Freedman, and M. A. Tolbert&lt;br /&gt;&lt;br /&gt;Amorphous (semi-)solid organic aerosol particles have the potential to serve
as surfaces for heterogeneous ice nucleation in cirrus clouds. Raman
spectroscopy and optical microscopy have been used in conjunction with a
cold stage to examine water uptake and ice nucleation on individual
amorphous (semi-)solid particles at atmospherically relevant temperatures
(200–273 K). Three organic compounds considered proxies for atmospheric
secondary organic aerosol (SOA) were used in this investigation: sucrose,
citric acid and glucose. Internally mixed particles consisting of each
organic and ammonium sulfate were also investigated.
&lt;br&gt;&lt;br&gt;
Results from water uptake experiments followed the shape of a
humidity-induced glass transition (&lt;i&gt;T&lt;/i&gt;&lt;sub&gt;g&lt;/sub&gt;(RH)) curve and were used to
construct state diagrams for each organic and corresponding mixture.
Experimentally derived &lt;i&gt;T&lt;/i&gt;&lt;sub&gt;g&lt;/sub&gt;(RH) curves are in good agreement with
theoretical predictions of &lt;i&gt;T&lt;/i&gt;&lt;sub&gt;g&lt;/sub&gt;(RH) following the approach of
Koop et al. (2011). A unique humidity-induced glass transition point
on each state diagram, &lt;i&gt;T&lt;/i&gt;&lt;sub&gt;g&lt;/sub&gt;'(RH), was used to quantify and
compare results from this study to previous works. Values of &lt;i&gt;T&lt;/i&gt;&lt;sub&gt;g&lt;/sub&gt;'(RH)
 determined for sucrose, glucose and citric acid glasses were 236,
230 and 220 K, respectively. Values of &lt;i&gt;T&lt;/i&gt;&lt;sub&gt;g&lt;/sub&gt;'(RH) for internally
mixed organic/sulfate particles were always significantly lower; 210, 207
 and 215 K for sucrose/sulfate, glucose/sulfate and citric acid/sulfate,
respectively.
&lt;br&gt;&lt;br&gt;
All investigated SOA proxies were observed to act as heterogeneous ice
nuclei at tropospheric temperatures. Heterogeneous ice nucleation on pure
organic particles occurred at &lt;i&gt;S&lt;/i&gt;&lt;sub&gt;ice&lt;/sub&gt;  = 1.1–1.4 for temperatures below
235 K. Particles consisting of 1:1 organic-sulfate mixtures took up water
over a greater range of conditions but were in some cases also observed to
heterogeneously nucleate ice at temperatures below 202 K (&lt;i&gt;S&lt;/i&gt;&lt;sub&gt;ice&lt;/sub&gt;= 1.25–1.38).
&lt;br&gt;&lt;br&gt;
Polynomial curves were fitted to experimental water uptake data and then incorporated into the Community Aerosol Radiation Model for Atmospheres (CARMA) along
with the predicted range of humidity-induced glass transition temperatures
for atmospheric SOA from Koop et al. (2011). Model results suggest
that organic and organic/sulfate aerosol could be glassy more than 60%
of the time in the midlatitude upper troposphere and more than 40% of
the time in the tropical tropopause region (TTL). At conditions favorable
for ice formation (&lt;i&gt;S&lt;/i&gt;&lt;sub&gt;ice&lt;/sub&gt; &gt; 1), particles in the TTL are
expected to be glassy more than 50% of the time for temperatures below
200 K. Results from this study suggests that amorphous (semi-)solid organic
particles are often present in the upper troposphere and that heterogeneous
ice formation on this type of particle may play an important role in cirrus
cloud formation.</description><pubDate>Fri, 07 Jun 2013 00:00:00 +0200</pubDate></item><item><title>Observations of peroxyacetyl nitrate (PAN) in the upper troposphere by the Atmospheric Chemistry Experiment-Fourier Transform Spectrometer (ACE-FTS)</title><link>http://www.atmos-chem-phys.net/13/5601/2013/</link><description>&lt;b&gt;Observations of peroxyacetyl nitrate (PAN) in the upper troposphere by the Atmospheric Chemistry Experiment-Fourier Transform Spectrometer (ACE-FTS)&lt;/b&gt;&lt;br /&gt;&lt;br /&gt;Atmospheric Chemistry and Physics, 13, 5601-5613, 2013&lt;br /&gt;&lt;br /&gt;Author(s): K. A. Tereszchuk, D. P. Moore, J. J. Harrison, C. D. Boone, M. Park, J. J. Remedios, W. J. Randel, and P. F. Bernath&lt;br /&gt;&lt;br /&gt;Peroxyacetyl nitrate (CH&lt;sub&gt;3&lt;/sub&gt;CO·O&lt;sub&gt;2&lt;/sub&gt;NO&lt;sub&gt;2&lt;/sub&gt;, abbreviated as PAN)
is a trace molecular species present in the troposphere and lower
stratosphere due primarily to pollution from fuel combustion and the
pyrogenic outflows from biomass burning. In the lower troposphere, PAN has a
relatively short lifetime and is principally destroyed within a few hours
through thermolysis, but it can act as a reservoir and carrier of
NO&lt;sub&gt;x&lt;/sub&gt; in the colder temperatures of the upper troposphere, where UV
photolysis becomes the dominant loss mechanism. Pyroconvective updrafts from
large biomass burning events can inject PAN into the upper troposphere and
lower stratosphere (UTLS), providing a means for the long-range transport of
NO&lt;sub&gt;x&lt;/sub&gt;. Given the extended lifetimes at these higher altitudes, PAN is
readily detectable via satellite remote sensing.
&lt;br&gt;&lt;br&gt;
A new PAN data product is now available for the Atmospheric Chemistry
Experiment Fourier Transform Spectrometer (ACE-FTS) version 3.0
data set. We report observations of PAN in boreal biomass burning plumes
recorded during the BORTAS
(quantifying the impact of BOReal forest fires on
Tropospheric oxidants over the Atlantic using Aircraft and Satellites) campaign (12 July to 3 August 2011). The retrieval
method employed by incorporating laboratory-recorded absorption
cross sections into version 3.0 of the ACE-FTS forward model
and retrieval software is described in full detail. The estimated detection
limit for ACE-FTS PAN is 5 pptv, and the total systematic error contribution
to the ACE-FTS PAN retrieval is ~ 16%.
&lt;br&gt;&lt;br&gt;
The retrieved volume mixing ratio (VMR) profiles are compared to coincident
measurements made by the Michelson Interferometer for Passive Atmospheric
Sounding (MIPAS) instrument on the European Space Agency (ESA) Environmental
Satellite (ENVISAT). The MIPAS measurements demonstrated good agreement with
the ACE-FTS VMR profiles for PAN, where the measured VMR values
are well within the associated measurement errors for both instruments and
comparative measurements differ no more than 70 pptv.
&lt;br&gt;&lt;br&gt;
The ACE-FTS PAN data set is used to obtain zonal mean
distributions of seasonal averages from ~ 5–20 km. A strong
seasonality is clearly observed for PAN concentrations in the global UTLS.
Since the principal source of PAN in the UTLS is due to lofted biomass
burning emissions from the pyroconvective updrafts created by large fires,
the observed seasonality in enhanced PAN coincides with fire activity in
different geographical regions throughout the year.</description><pubDate>Thu, 06 Jun 2013 00:00:00 +0200</pubDate></item></channel></rss>