Jul 2 – 6, 2018
Žofín Palace
Europe/Prague timezone

P1.1100 Complex-eikonal methods applied to geodesic acoustic modes

Jul 2, 2018, 2:00 PM
2h
Mánes

Mánes

Masarykovo nábřeží 1, 110 00 Praha 1

Speaker

Francesco Palermo

Description

See the full Abstract at http://ocs.ciemat.es/EPS2018ABS/pdf/P1.1100.pdf Complex-eikonal methods applied to geodesic acoustic modes F. Palermo1 , E. Poli1 , A. Bottino1 , A. Ghizzo2 1 Max-Planck-Institut für Plasmaphysik, 85748 Garching, Germany 2 Institut Jean Lamour, University of Lorraine, F-54506 Vandoeuvre les Nancy, France The tokamak represents a very complex system in which several actors such as drift waves, streamers, turbulence, zonal flow, geodesic acoustic modes (GAMs)... interact each other defining the transport properties of the plasma. GAMs represent the oscillation counterpart of the zonal flow and have received much attention for their potential role in the energy confinement in plasma fusion domain. In particular they inter- act with turbulence in an inhomogeneous envi- ronment in which plasma shape and profile gra- dients strongly affects their amplitude and their position [1, 2]. Because of the complexity of the system, it is crucial to develop and to apply Figure 1: Electric field evolution of GAM in (time, methods that allow to have simple and accurate radial) plane. Overlapped it is shown the ray paths descriptions of specific properties of plasma be- predicted by using the geometrical optics methods. havior. In this way, it is possible to distinguish in an intuitive and useful manner relevant aspects of global physical systems. To this purpose, ray method or geometrical optics provides a very powerful tool that has been applied in many important problems related to wave propagation and energy transport. By using the paraxial WKB (pWKB) method [3, 4] and a complex-eikonal approach [5], we describe several GAM properties such as amplitude, shape evolution and energy flux of GAM in homogeneous and in- homogeneous equilibria. These findings allow us to predict the GAM evolution, in simulations (see Fig. 1) performed with the particle-in-cell code ORB5 [6, 7]. References [1] F. Palermo et al., Physics of Plasmas 24, 072503, (2017) [2] F. Palermo et al., 44rd EPS Conference on Plasma Physics P4.160, (2017) [3] G. V. Pereverzev, Physics of Plasmas 5, 3529, (1999) [4] E. Poli et al., Physics of Plasmas 6, 5, (1999) [5] E. Mazzuccato, Physics of Plasmas 1, 1855 (1989) [6] S. Jolliet et al., Comput. Phys. Commun. 177, 409 (2007) [7] A. Bottino and E. Sonnendrucker, J. Plasma Phys. 81, 435810501 (2015)

Primary author

Presentation materials

There are no materials yet.