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<article language="en">
	<journal>
		<journal_title>Atmospheric Chemistry and Physics</journal_title>
		<journal_url>www.atmos-chem-phys.net</journal_url>
		<issn>1680-7316</issn>
		<eissn>1680-7324</eissn>
		<volume_number>6</volume_number>
		<issue_number>8</issue_number>
		<publication_year>2006</publication_year>
	</journal>
	<doi>10.5194/acp-6-2073-2006</doi>
	<article_url>http://www.atmos-chem-phys.net/6/2073/2006/</article_url>
	<abstract_html>http://www.atmos-chem-phys.net/6/2073/2006/acp-6-2073-2006.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys.net/6/2073/2006/acp-6-2073-2006.pdf</fulltext_pdf>
	<start_page>2073</start_page>
	<end_page>2090</end_page>
	<publication_date>2006-06-20</publication_date>
	<article_title content_type="html">Modelling the budget of middle atmospheric water vapour isotopes</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>A. Zahn</name>
			<email>andreas.zahn@imk.fzk.de</email>
		</author>
		<author numeration="2" affiliations="2,3">
			<name>P. Franz</name>
		</author>
		<author numeration="3" affiliations="4">
			<name>C. Bechtel</name>
		</author>
		<author numeration="4" affiliations="6">
			<name>J.-U. GrooÃŸ</name>
		</author>
		<author numeration="5" affiliations="2,5">
			<name>T. RÃ¶ckmann</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Institute of Meteorology and Climate Research, Forschungszentrum Karlsruhe, Germany</affiliation>
		<affiliation numeration="2" content_type="html">Max-Planck-Institute for Nuclear Physics, Heidelberg, Germany</affiliation>
		<affiliation numeration="3" content_type="html">National Institute for Water and Atmospheric Research (NIWA), Wellington, New Zealand</affiliation>
		<affiliation numeration="4" content_type="html">Robert Bosch GmbH, BÃ¼hl, Germany</affiliation>
		<affiliation numeration="5" content_type="html">Institute for Marine and Atmospheric Research Utrecht, Utrecht University, The Netherlands</affiliation>
		<affiliation numeration="6" content_type="html">Institute of Chemistry and Dynamics of the Geosphere, Forschungszentrum JÃ¼lich, Germany</affiliation>
	</affiliations>
	<abstract content_type="html">A one-dimensional chemistry model is applied to study the stable hydrogen (D) and stable
oxygen isotope (&lt;sup&gt;17&lt;/sup&gt;O, &lt;sup&gt;18&lt;/sup&gt;O) composition of water vapour in stratosphere and mesosphere.
In the troposphere, this isotope composition is determined by &quot;physical&apos;&apos; fractionation
effects, that are phase changes (e.g. during cloud formation), diffusion processes
(e.g. during evaporation from the ocean), and mixing of air masses. Due to these
processes water vapour entering the stratosphere first shows isotope depletions in D/H
relative to ocean water, which are ~5 times of those in &lt;sup&gt;18&lt;/sup&gt;O/&lt;sup&gt;16&lt;/sup&gt;O, and
secondly is mass-dependently fractionated (MDF), i.e. changes in the isotope ratio
&lt;sup&gt;17&lt;/sup&gt;O/&lt;sup&gt;16&lt;/sup&gt;O are ~0.52 times of those of &lt;sup&gt;18&lt;/sup&gt;O/&lt;sup&gt;16&lt;/sup&gt;O. In contrast, in the
stratosphere and mesosphere &quot;chemical&apos;&apos; fractionation mechanisms, that are the
production of H&lt;sub&gt;O&lt;/sub&gt; due to the oxidation of methane, re-cycling of H&lt;sub&gt;2&lt;/sub&gt;O via the HO&lt;sub&gt;x&lt;/sub&gt;
family, and isotope exchange reactions considerably enhance the isotope ratios in the
water vapour imported from the troposphere. The model reasonably predicts overall
enhancements of the stable isotope ratios in H&lt;sub&gt;2&lt;/sub&gt;O by up to ~25% for D/H, ~8.5%
for &lt;sup&gt;17&lt;/sup&gt;O/&lt;sup&gt;16&lt;/sup&gt;O, and ~14% for &lt;sup&gt;18&lt;/sup&gt;O/&lt;sup&gt;16&lt;/sup&gt;O in the mesosphere relative to the tropopause
values. The &lt;sup&gt;17&lt;/sup&gt;O/&lt;sup&gt;16&lt;/sup&gt;O and &lt;sup&gt;18&lt;/sup&gt;O/&lt;sup&gt;16&lt;/sup&gt;O ratios in H&lt;sub&gt;2&lt;/sub&gt;O are shown to be a
measure of the relative fractions of HO&lt;sub&gt;x&lt;/sub&gt; that receive the O atom either from the
reservoirs O&lt;sub&gt;2&lt;/sub&gt; or O&lt;sub&gt;3&lt;/sub&gt;. Throughout the middle atmosphere, MDF O&lt;sub&gt;2&lt;/sub&gt; is the major
donator of oxygen atoms incorporated in OH and HO&lt;sub&gt;2&lt;/sub&gt; and thus in H&lt;sub&gt;2&lt;/sub&gt;O. In the
stratosphere the known mass-independent fractionation (MIF) signal in O&lt;sub&gt;3&lt;/sub&gt; is in a first
step transferred to the NO&lt;sub&gt;x&lt;/sub&gt; family and only in a second step to HO&lt;sub&gt;x&lt;/sub&gt; and
H&lt;sub&gt;2&lt;/sub&gt;O. In contrast to CO&lt;sub&gt;2&lt;/sub&gt;, O(&lt;sup&gt;1&lt;/sup&gt;D) only plays a minor role in this MIF transfer. The
major uncertainty in our calculation arises from poorly quantified isotope exchange
reaction rate coefficients and kinetic isotope fractionation factors.</abstract>
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</article>

