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Prime pagine RA2010FUS:Copia di Layout 1 - ENEA - Fusione

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Contents<br />

006 Preface<br />

008 Anniversary<br />

010 Magnetic Confinement<br />

010 Introduction<br />

011 FTU Facility<br />

011 Summary of the machine operation<br />

013 FTU Experimental Activity<br />

013 Lower hybrid<br />

016 Alfvén eigenmodes: modeling, experimental results<br />

and future plans<br />

017 Electron cyclotron<br />

021 Liquid lithium experiments<br />

023 Diagnostic developments<br />

029 Plasma–wall interaction<br />

Euratom–<strong>ENEA</strong><br />

Association<br />

2010annual<br />

fusion<br />

activities<br />

030 Plasma Theory<br />

030 Alfvén modes in the presence of a magnetic island<br />

031 Nonlocal theory of energetic–particle–induced<br />

geodesic acoustic mode<br />

032 Kinetic structures of shear Alfvén and acoustic wave<br />

spectra in burning plasmas<br />

032 ITPA benchmarking activity using HMGC<br />

033 TAE eigenfunctions for ITER magnetic <strong>di</strong>agnostics<br />

033 ITM–TF activities<br />

033 The new hybrid MHD–gyrokinetic code: HYMAGYC<br />

034 Applications and further implementation of the<br />

eXtended HMGC hybrid code<br />

035 Parametric form of equilibrium particle <strong>di</strong>stribution<br />

functions for implementations in HMGC<br />

035 Design of energetic particle equilibrium <strong>di</strong>stribution<br />

functions<br />

036 A new model for self–organized critical dynamics, with<br />

implication of the fishbone–like instability cycle<br />

037 Asymptotic techniques in the study of the propagation<br />

of high frequency (lower hybrid range) electromagnetic<br />

waves<br />

037 Analytical and numerical stu<strong>di</strong>es of the cold<br />

electromagnetic LH wave equation in the mode<br />

conversion regimev<br />

037 Hamiltonian perturbation theory in studying the LH<br />

wave propagation in burning plasmas<br />

038 The propagation and absorption of lower hybrid<br />

waves in H–mode plasma with very sharp density<br />

gra<strong>di</strong>ent at the pedestal<br />

038 Tritium minority heating with mode conversion of fast<br />

waves<br />

038 Stellar winds or matter–jet seeds from <strong>di</strong>sk plasma<br />

configuration

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