Caramulo, Portugal, August 31 - September 6 , 2003.

Invited Speakers

Name	Location	Email	Lecture
Pr. Friedrich Busse	Bayreuth	busse@uni-bayreuth.de	Rotating convection
Dr. Philippe Cardin	U.J.F.	Philippe.Cardin@obs.ujf-grenoble.fr	Survey of experimental results
Pr. Fausto Cattaneo	Chicago	cattaneo@math.uchicago.edu	Introduction to MHD turbulence
Pr. David Fearn	Glasgow	D.Fearn@maths.gla.ac.uk	Introduction to the Geodynamo
Dr. Andrew Gilbert	Exeter	A.D.Gilbert@ex.ac.uk	Introduction to Fast Dynamos
Pr. Christopher Jones	Exeter	C.A.Jones@ex.ac.uk	Introduction to Planetary dynamos
Pr. Michael Proctor	Cambridge	mrep@damtp.cam.ac.uk	Introduction to self-excited dynamo action
Pr. Paul Roberts	U.C.L.A.	roberts@math.ucla.edu	Turbulence in the Earth core
Dr. Anvar Shukurov	Newcastle	Anvar.Shukurov@newcastle.ac.uk	Introduction to Galactic dynamos
Pr. Andrew Soward	Exeter	soward@noether.ex.ac.uk	Asymptotic results on rotating and MHD flows
Pr. Nigel Weiss	Cambridge	now@damtp.cam.ac.uk	Introduction to Stellar dynamos

Organisers

Name	Institute	Email
Dr. Emmanuel Dormy	Institut de Physique du Globe de Paris	dormy@ipgp.jussieu.fr
Dr. Alexandra Pais	Center for Computational Physics, Coimbra	pais@teor.fis.uc.pt

Co-organisers

Dr. Benoît Desjardins	Ecole Normale Supérieure de Paris	desjardi@dma.ens.fr
Pr. Emmanuel Grenier	Ecole Normale Supérieure de Lyon	egrenier@umpa.ens-lyon.fr
Dr. Fernando Nogueira	Center for Computational Physics, Coimbra	fnog@teor.fis.uc.pt
Dr. Orlando Oliveira	Center for Computational Physics, Coimbra	orlando@teor.fis.uc.pt

Participants

Name	Institute	Position	Email	Presentation
Thierry Alboussiere	University of Cambridge	Lecturer	ta209@eng.cam.ac.uk	Experimental transition to turbulence of Hartmann layers
Alexander Anufriev	Geophysical Institute of Bulgarian Academy of Sciences	Senior scentist worker	anufriev@geophys.bas.bg	Amplitudes of the solution at the compressible convection in the Earth's core.
Raul Avalos-Zuniga	Laboratoire des Ecoulements Géophysiques et Industriels	PhD student	Raul.Avalos@hmg.inpg.fr	Influence of electromagnetic boundary conditions onto the onset of dynamo action in laboratory experiments
Manuel Baptista	DMA-FCUP	Ph.D student	mbaptist@fc.up.pt	Stability oF MHD flow steady states to perturbations in a large spatial scale of a 3D periodic domain
Alberto Bigazzi	Jet Propulsion Laboratory, Californaia Institute of Technology	NRC post-doctoral researcher.	alberto.bigazzi@jpl.nasa.gov	Non-axisymmetric dynamo modeling of solar preferred longitudes
Francois Bouchut	CNRS	Researcher	fbouchut@dma.ens.fr	Numerical simulation of rotating shallow water flows
Mickael Bourgoin	ENS-Lyon	PhD	mbourgoi@ens-lyon.fr	MHD induction in swirling flows
Axel Brandenburg	Nordita	Professor	brandenb@nordita.dk	What is the energy-carrying scale of a solar surface dynamo?
Jozef Brestensky	Dept of Physics of the Earth and Planets, Faculty of Maths, Physics and Informatics, Comenius University, Bratislava	Associate Professor	brestensky@fmph.uniba.sk	- Magnetic Instabilities Catalysed by Viscosity in the Earth's Core - Rotating Convection with Soret Effect in the Earth's Core
Martin Breuer	University of Münster	PhD student	breuerm@earth.uni-muenster.de	The influence of inertia on convection in a rotating spherical shell
Nic Brummell	JILA, University of Colorado, USA	Research Assistant Professor	brummell@solarz.colorado.edu	A dynamo driven by the interaction of shear and magnetic buoyancy
Allan Sacha Brun	CEA Saclay/Service d'Astrophysique	permanent researcher	sacha.brun@cea.fr	The Turbulent Magnetic Sun: A 3-D MHD Approach
Alice Courvoisier	University of Leeds	PhD student	alice@maths.leeds.ac.uk	Modulated dynamos in cellular flows
Stéphane Descombes	Ecole normale supérieure de Lyon	Assistant professor	sdescomb@umpa.ens-lyon.fr	Order reduction of numerical schemes in the presence of small parameters
Antonio Ferriz-Mas	Universidad de Vigo	Lecturer	antonio.ferriz@oulu.fi	Where does the solar dynamo operate?
Peter Frick	Institute of Continuous Media Mechanics	Head of Laboratory	frick@icmm.ru	P.Frick and D.Sokoloff "A simple model of multiscale dynamo"
Agris Gailitis	Institute of Physics University of Latvia	leading researcher	gailitis@sal.lv	New results of Riga dynamo experiment and its mathematical background
Sílvio Gama	DMA-FCUP	Assistent Professor	smgama@fc.up.pt	Stability oF MHD flow steady states to perturbations in a large spatial scale of a 3D periodic domain
David Gerard-Varet	ENS-Lyon	PhD student	dgerardv@umpa.ens-lyon.fr	Ekman Layers near rough boundaries
Nicolas Gillet	LGIT, Grenoble	PhD student	Nicolas.Gillet@obs.ujf-grenoble.fr	Experimental and numerical study of developped magneto-convection in a rapidly rotating sphere
Renato Guedes	CFC-FCTUC	student	renato@malaposta.fis.uc.pt
Uwe Guenther	Research Center Rossendorf, Dresden, Germany	researcher	u.guenther@fz-rossendorf.de	A no-go theorem for isospectral alpha2-dynamos
Pavel Hejda	Geophysical Institute	Deputy-Director	ph@ig.cas.cz	Numerical modelling of geodynamo by finite volume method
Peter Hoyng	SRON Laboratory for Space Research	Senoir scientist	p.hoyng@sron.nl	Ab initio calculation of the mean reversal time of a geodynamo model
David Hughes	University of Leeds	Professor	dwh@maths.leeds.ac.uk	Dynamo Action in the Presence of a Background Field
Alexey Iskakov	I.P.G.P., Paris	post-doc researcher	iskakov@ipgp.jussieu.fr	A mixed finite Volume - Boundary element formulation for magnetic induction in b ounded domain
Evy Kersalé	Applied Mathematics, Leeds	Postdoctorate	kersale@maths.leeds.ac.uk	Global MRI and dynamo in accretion discs
Nathan Kleeorin	Ben-Gurion University of the Negev	Associate Professor	nat@menix.bgu.ac.il	Magnetic Helicity Transport and Solar and Galactic Dynamos
Maarit Korpi	Laboratoire d'Astrophysique, Observatoire Midi-Pyrenees, Toulouse	Visiting postdoctoral researcher	Maarit.Korpi@oulu.fi	Sources of interstellar turbulence and their relation to dynamo action: a numerical investigation
Kirill Kuzanyan	IZMIRAN, Russian Academy of Sciences	senior researcher	kuzanyan@dnttm.ru	Helicity and the alpha-effect in solar dynamo: theory and observations(tentative title)
Gedeon Legaut	LGIT, Grenoble	PhD student	Gedeon.Legaut@obs.ujf-grenoble.fr	Secular variation of the Earth's magnetic field
Nicolas Leprovost	SPEC - CEA Saclay	PhD Student	nicolas.leprovost@cea.fr	Turbulent diffusion with ambipoar drift
Philip Livermore	School of Earth Sciences, Leeds University	Graduate student	p.livermore@earth.leeds.ac.uk	Magnetic energy stability in spherical flows
Joanne Mason	University of Leeds, UK.	PhD student	joanne@maths.leeds.ac.uk	Models of the Solar Dynamo incorporating Magnetic Pumping
Stéphane Mathis	Observatoire de Paris-Section de Meudon, L.U.T.H.	PHD student	stephane.mathis@obspm.fr	Transport in stellar radiation zones with magnetic field
Xu Mingtian	Forschungszentrum Rossendorf, Germany	Doctor	M.Xu@fz-rossendorf.de	An integral equation approach to unsteady kinematic dynamos
Krzysztof Mizerski	Warsaw University, Institute of Geophysics	Student	kamiz@igf.fuw.edu.pl	Couette flow
Vincent Morin	I.P.G.P., Paris	PhD student	morin@ipgp.jussieu.fr	Convection in rapidly rotating fluid sphere
Manuel Nunez	Universidad de Valladolid	Professor	mnjmhd@am.uva.es	Dynamics of the stretching of magnetic fields
Franck Plunian	Laboratoire des Ecoulements Géophysiques et Industriels	Maître de Conferences	Franck.Plunian@hmg.inpg.fr	Influence of electromagnetic boundary conditions onto the onset of dynamo action in laboratory experiments
Yannick Ponty	Laboratoire G.D Cassini / Observatoire de la Cote d'Azur	Charge de Recherche	ponty@obs-nice.fr	Dynamo action at low magnetic Prandtl number using Large Eddies Simulation
Florent Ravelet	cea saclay / spec	PhD student	ravelet@drecam.saclay.cea.fr	What happens in a conducting shell surrounding a kinematic cylindrical dynamo ?
Karl-Heinz Raedler	Astrophysical Institute Potsdam	Retired	khraedler@aip.de	A remark on kinetic helicity, alpha-effect and dynamo action
Igor Rogachevskii	Ben-Gurion University of the Negev	Associate Professor	gary@bgumail.bgu.ac.il	Electromotive Force in Turbulent Convection and Magnetic Dynamos
Jon Rotvig	University of Exeter	Research, post.doc.	J.Rotvig@ex.ac.uk	Dynamos and convection: mean flow generation
Alexander Ruzmaikin	JPL, Caltech	Research Scientist	Alexander.Ruzmaikin@jpl.nasa.gov	The Non-Axisymmetric Solar Dynamo
Alexander Schekochihin	Imperial College London	Research Associate	a.schekochihin@ic.ac.uk	- Linear and nonlinear small-scale turbulent dynamo - From Small-Scale Dynamo to Isotropic MHD Turbulence: Folded Fields and Alfven Waves
Martin Schrinner	Max Planck Institute for Aeronomy	PhD student	schrinne@linmpi.mpg.de	Mean-field coefficients for geodynamo models
Radostin Dimov Simitev	Institute of Physics , University of Bayreuth, Gernamy	Doctoral Student (Advisor: Prof. F.H. Busse)	radostin.simitev@uni-bayreuth.de	Dynamical Processes and Parameter Dependences of Convection Driven Spherical Dynamos
Stephan Stellmach	University of Münster	PHD student	stellma@earth.uni-muenster.de	Cartesian small Ekman number dynamos
Andreas Tilgner	Institute of Geophysics, University of Goettingen	Professor	andreas.tilgner@physik.uni-goettingen.de	Mode selection in experimental dynamos
Steve Tobias	University of Leeds	Lecturer	smt@maths.leeds.ac.uk	The role of spectra in turbulent dynamos
Romain Volk	Ecole Normale Superieure de Lyon	PhD student	rvolk@ens-lyon.fr	Induction mechanisms in a von karman flow of liquid gallium

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