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<article language="en">
	<journal>
		<journal_title>Geoscientific Model Development Discussions</journal_title>
		<journal_url>www.geosci-model-dev-discuss.net</journal_url>
		<issn>1991-9611</issn>
		<eissn>1991-962X</eissn>
		<volume_number>3</volume_number>
		<issue_number>3</issue_number>
		<publication_year>2010</publication_year>
	</journal>
	<doi>10.5194/gmdd-3-1359-2010</doi>
	<article_url>http://www.geosci-model-dev-discuss.net/3/1359/2010/</article_url>
	<abstract_html>http://www.geosci-model-dev-discuss.net/3/1359/2010/gmdd-3-1359-2010.html</abstract_html>
	<fulltext_pdf>http://www.geosci-model-dev-discuss.net/3/1359/2010/gmdd-3-1359-2010.pdf</fulltext_pdf>
	<start_page>1359</start_page>
	<end_page>1421</end_page>
	<publication_date>2010-09-01</publication_date>
	<article_title content_type="html">The global middle-atmosphere aerosol model MAECHAM5-SAM2: comparison with satellite and in-situ observations</article_title>
	<authors>
		<author numeration="1" affiliations="1,3">
			<name>R. Hommel</name>
			<email>rene.hommel@atm.ch.cam.ac.uk</email>
		</author>
		<author numeration="2" affiliations="1">
			<name>C. Timmreck</name>
		</author>
		<author numeration="3" affiliations="2">
			<name>H. F. Graf</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Max Planck Institute für Meteorologie, Hamburg, Germany</affiliation>
		<affiliation numeration="2" content_type="html">Centre for Atmospheric Science, Department of Geography, Cambridge University, Cambridge, UK</affiliation>
		<affiliation numeration="3" content_type="html">now at: Centre for Atmospheric Science, Department of Chemistry, Cambridge University, Cambridge, UK</affiliation>
	</affiliations>
	<abstract content_type="html">In this paper we investigate results from a middle-atmosphere aerosol-climate
model which has been developed to study the evolution of stratospheric
aerosols. Here we focus on the stratospheric background period and evaluate
several key quantities of the global dispersion of stratospheric aerosols and
their precursors with observations and other model studies. It is shown that
the model fairly well reproduces in situ observations of the aerosol size and
number concentrations in the upper troposphere and lower stratosphere
(UT/LS). Compared to measurements from the limb-sounding SAGE II
satellite instrument, modelled integrated aerosol quantities are more biased
the lower the moment of the aerosol population. Both findings are consistent
with earlier work analysing the quality of SAGE II retrieved e.g.
aerosol surface area densities from the volcanically unperturbed stratosphere
(SPARC/ASAP, 2006; Thomason et al.,
2008; Wurl et al., 2010).
&lt;br&gt;&lt;br&gt;
The model suggests that new particles are formed over large areas of the LS,
albeit nucleation rates in the upper troposphere are at least one order of
magnitude larger than those in the stratosphere. Hence, we suggest that both
tropospheric sulphate aerosols and particles formed in situ in the LS are
maintaining the stability of the stratospheric aerosol layer also in the
absence of direct stratospheric emissions from volcanoes. Particle size
distributions are clearly bimodal, except in the upper branches of the
stratospheric aerosol layer where aerosols evaporate. Modelled concentrations
of condensation nuclei (CN) are lesser than measured in regions of the
aerosol layer where aerosol mixing ratios are largest, due to an
overpredicted particle growth by coagulation.
&lt;br&gt;&lt;br&gt;
Transport regimes of tropical stratospheric aerosol have been identified from
modelled aerosol mixing ratios and correspond to those deduced from satellite
extinction measurements. We found that convective updraft in the Asian
Monsoon region significantly contributes to both stratospheric aerosol load
and size. The timing of formation and descend of layers of fine mode
particles in the winter and spring polar stratosphere (CN layer) are
reproduced by the model. Far above the tropopause where nucleation is
inhibited due to with height increasing stratospheric temperatures, planetary
wave mixing transports significant amounts of fine mode particles from the
polar stratosphere to mid-latitudes. In those regions enhanced condensation
rates of sulphuric acid vapour counteracts the evaporation of aerosols, hence
prolonging the aerosol lifetime in the upper branches of the stratospheric
aerosol layer.
&lt;br&gt;&lt;br&gt;
Measurements of the aerosol precursors SO&lt;sub&gt;2&lt;/sub&gt; and sulphuric acid vapour are
fairly well reproduced by the model throughout the stratosphere.</abstract>
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