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	<journal>
		<journal_title>Atmospheric Chemistry and Physics Discussions</journal_title>
		<journal_url>www.atmos-chem-phys-discuss.net</journal_url>
		<issn>1680-7367</issn>
		<eissn>1680-7375</eissn>
		<volume_number>10</volume_number>
		<issue_number>2</issue_number>
		<publication_year>2010</publication_year>
	</journal>
	<doi>10.5194/acpd-10-3189-2010</doi>
	<article_url>http://www.atmos-chem-phys-discuss.net/10/3189/2010/</article_url>
	<abstract_html>http://www.atmos-chem-phys-discuss.net/10/3189/2010/acpd-10-3189-2010.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys-discuss.net/10/3189/2010/acpd-10-3189-2010.pdf</fulltext_pdf>
	<start_page>3189</start_page>
	<end_page>3228</end_page>
	<publication_date>2010-02-05</publication_date>
	<article_title content_type="html">The impact of the 1783â€“1784 AD Laki eruption on global aerosol  formation processes and cloud condensation nuclei</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>A. Schmidt</name>
			<email>a.schmidt@see.leeds.ac.uk</email>
		</author>
		<author numeration="2" affiliations="1">
			<name>K. S. Carslaw</name>
		</author>
		<author numeration="3" affiliations="2">
			<name>G. W. Mann</name>
		</author>
		<author numeration="4" affiliations="1">
			<name>B. M. Wilson</name>
		</author>
		<author numeration="5" affiliations="1">
			<name>T. J. Breider</name>
		</author>
		<author numeration="6" affiliations="1">
			<name>S. J. Pickering</name>
		</author>
		<author numeration="7" affiliations="3">
			<name>T. Thordarson</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">School of Earth and Environment, University of Leeds, LS2 9JT, UK</affiliation>
		<affiliation numeration="2" content_type="html">NCAS, University of Leeds, LS2 9JT, UK</affiliation>
		<affiliation numeration="3" content_type="html">School of Geosciences, Grant Institute, University of Edinburgh, Edinburgh, UK</affiliation>
	</affiliations>
	<abstract content_type="html">The 1783â€“1784 AD Laki flood lava eruption commenced on 8 June 1783 and
      released 122 Tg of sulphur dioxide gas over the course of 8 months
      into the upper troposphere and lower stratosphere above
      Iceland. Previous studies have examined the impact of the Laki
      eruption on sulphate aerosol and climate using general circulation
      models. Here, we study the impact on aerosol microphysical processes,
      including the nucleation of new particles and their growth to cloud
      condensation nuclei (CCN) using a comprehensive Global Model of
      Aerosol Processes (GLOMAP). Total particle concentrations in the free
      troposphere increase by a factor ~16 over large parts of the
      Northern Hemisphere in the 3 months following the onset of the
      eruption. Particle concentrations in the boundary layer increase by
      a factor 2 to 5 in regions as far away as North America, the Middle
      East and Asia due to long-range transport of nucleated particles. CCN
      concentrations (at 0.22% supersaturation) increase by a factor 65 in
      the upper troposphere with maximum changes in 3-month zonal mean
      concentrations of ~1400 cm&lt;sup&gt;&amp;minus;3&lt;/sup&gt; at high northern
      latitudes. 3-month zonal mean CCN concentrations in the boundary layer
      at the latitude of the eruption increase by up to a factor 26, and
      averaged over the Northern Hemisphere, the eruption caused a factor 4
      increase in CCN concentrations at low-level cloud altitude. The
      simulations show that the Laki eruption would have completely
      dominated as a source of CCN in the pre-industrial atmosphere. The
      model also suggests an impact of the eruption in the Southern
      Hemisphere, where CCN concentrations are increased by up to a factor
      1.4 at 20&amp;deg; S. Our model simulations suggest that the impact
      of an equivalent wintertime eruption on upper tropospheric CCN
      concentrations is only about one-third of that of a summertime
      eruption. The simulations show that the microphysical processes
      leading to the growth of particles to CCN sizes are fundamentally
      different after an eruption when compared to the unperturbed
      atmosphere, underlining the importance of using a fully coupled
      microphysics model when studying long-lasting, high-latitude
      eruptions.</abstract>
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