<?xml version="1.0" encoding="utf-8" standalone="no"?>
<!DOCTYPE article SYSTEM "http://www.adv-sci-res.net/inc/asr/copernicus.dtd">
<article language="en">
	<journal>
		<journal_title>Advances in Science and Research</journal_title>
		<journal_url>www.adv-sci-res.net</journal_url>
		<issn>1992-0628</issn>
		<eissn>1992-0636</eissn>
		<volume_number>3</volume_number>
		<volume_title>8th EMS Annual Meeting and 7th European Conference on Applied Climatology 2008</volume_title>
		<publication_year>2009</publication_year>
	</journal>
	<doi>10.5194/asr-3-79-2009</doi>
	<article_url>http://www.adv-sci-res.net/3/79/2009/</article_url>
	<abstract_html>http://www.adv-sci-res.net/3/79/2009/asr-3-79-2009.html</abstract_html>
	<fulltext_pdf>http://www.adv-sci-res.net/3/79/2009/asr-3-79-2009.pdf</fulltext_pdf>
	<start_page>79</start_page>
	<end_page>84</end_page>
	<publication_date>2009-04-29</publication_date>
	<article_title content_type="html">Deriving turbulence characteristics from the COSMO numerical weather prediction model for dispersion applications</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>B. Szintai</name>
			<email>balazs.szintai@meteoswiss.ch</email>
		</author>
		<author numeration="2" affiliations="1">
			<name>P. Kaufmann</name>
		</author>
		<author numeration="3" affiliations="1">
			<name>M. W. Rotach</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Federal Office of Meteorology and Climatology MeteoSwiss, Zürich, Switzerland</affiliation>
	</affiliations>
	<abstract content_type="html">At MeteoSwiss an integrated modelling system is used to simulate the
dispersion of radioactive material in emergency situations. For the
prediction of the atmospheric flow, the COSMO numerical weather prediction
model is used. The model is run operationally at 6.6 and 2.2 km horizontal
resolution, respectively and uses a 1.5 order turbulence closure with a
prognostic equation for turbulent kinetic energy. Both versions of the COSMO
model are coupled off-line with a Lagrangian particle dispersion model
(LPDM). The aim of this study is to investigate the sensitivity of the
dispersion model to different interfacing approaches between LPDM and the
COSMO model. The diagnosed turbulence variables are validated on an ideal
convective case and two measurement campaigns. Simulations of hypothetical
pollutant releases show that the different interfacing approaches can lead
to substantial changes in the forecasted concentrations.</abstract>
	<references>
		<reference numeration="1" content_type="text"> Arpagaus, M.: Verification of vertical profiles: Operational verification at MeteoSwiss, COSMO Newsletter No. 5., 102–105, available online: http://www.cosmo-model.org, 2005. </reference>
		<reference numeration="2" content_type="text"> Batchvarova, E. and Gryning, S. E.: Applied model for the growth of the daytime mixed layer, Bound.-Lay. Meteorol. 56, 261–274, 1991. </reference>
		<reference numeration="3" content_type="text"> Beyrich, F. and Mengelkamp, H. T.: Evaporation over a Heterogeneous Land Surface: EVA_GRIPS and the LITFASS-2003 Experiment – An Overview, Bound.-Lay. Meteorol., 121, 5–32, 2006. </reference>
		<reference numeration="4" content_type="text"> Buzzi, M., Rotach, M. W., Raschendorfer, M., and Holtslag, A. A. M.: Evaluation of the COSMO-SC boundary layer scheme for stable conditions, Meteorol. Z., submitted, 2009. </reference>
		<reference numeration="5" content_type="text"> Doms, G. and Schaettler, U.: The nonhydrostatic limited-area model LM – Part I: Dynamics and Numerics. Scientific Documentation, Deutscher Wetterdienst, Offenbach, Germany, available online: http://www.cosmo-model.org, 2002. </reference>
		<reference numeration="6" content_type="text"> Glaab, H., Fay B., and Jacobsen, I.: Evaluation of the emergency dispersion model at the Deutscher Wetterdienst using ETEX data, Atmos. Environ., 32, 4359–4366, 1998. </reference>
		<reference numeration="7" content_type="text"> Hanna, S. R.: Applications in air pollution modeling, in: Atmospheric Turbulence and Air Pollution Modelling, edited by: Nieuwstadt, F. T. M. and van Dop, H., D Reidel Publishing Company, Dordrecht, Holland, 275–310, 1982. </reference>
		<reference numeration="8" content_type="text"> Kaufmann, P.: Verification of aLMo with SYNOP and GPS data over Europe, COSMO Newsletter No. 5., 113–117, available online: http://www.cosmo-model.org, 2005. </reference>
		<reference numeration="9" content_type="text"> Mellor, G. L. and Yamada, T.: Development of a turbulence closure model for geophysical flow problems, Rev. Geophys. Space Phys., 20, 851–875, 1982. </reference>
		<reference numeration="10" content_type="text"> Mironov, D. V., Gryanik, V. M., Moeng, C.-H., Olbers, D. J., and Warncke, T. H.: Vertical turbulence structure and second-moment budgets in convection with rotation: A large-eddy simulation study, Q. J. Roy. Meteor. Soc., 126, 477–515, 2000. </reference>
		<reference numeration="11" content_type="text"> Legg, B. J. and Raupach, M.: Markov-chain simulation of particle dispersion in inhomogeneous flows: the mean drift velocity induced by a gradient in Eulerian velocity variance, Bound.-Lay. Meteorol., 24, 3–13, 1982. </reference>
		<reference numeration="12" content_type="text"> Stohl, A., Forster, C., Frank, A., Seibert, P., and Wotawa, G.: Technical note: The Lagrangian particle dispersion model FLEXPART version 6.2, Atmos. Chem. Phys., 5, 2461–2474, 2005. </reference>
		<reference numeration="13" content_type="text"> Szintai, B. and Kaufmann, P.: TKE as a measure of turbulence, COSMO Newsletter No. 8., 2–10, available online: http://www.cosmo-model.org, 2008. </reference>
		<reference numeration="14" content_type="text"> Thomson, D. J.: Criteria for the selection of stochastic models of particle trajectories in turbulent flows, J. Fluid Mech., 180, 529–556, 1987. </reference>
		<reference numeration="15" content_type="text"> Zilitinkevich, S., Esau, I., and Baklanov, A.: Further comments on the equilibrium height of neutral and stable planetary boundary layers, Q. J. Roy. Meteor. Soc., 133, 265–271, 2007. </reference>
	</references>
</article>

