Published December 15, 2003 | Version v1
Journal article

Density Convection near Radiating ICRF Antennas and its Effect on the Coupling of Lower Hybrid Waves

  • 1. Association Euratom-CEA, CEA/DSM/DRFC, CEA-Cadarache, 13108 St Paul-lez-Durance (France)
  • 2. Euratom/UKAEA Fusion Association, Culham Science Centre, Abingdon, OX14 3DB (United Kingdom)
  • 3. Gent University, EESA Department, B-9000 Gent (Belgium)
  • 4. Max-Planck-Institut fuer Plasmaphysik, Euratom Association, D-85748 Garching (Germany)
  • 5. Associazione Euratom-ENEA sulla Fusione, CR Frascati, C.P. 65, 00044 Frascati, Rome (Italy)

Description

Combined operation of Lower Hybrid (LH) and Ion Cyclotron Resonance Frequency (ICRF) waves can result in a degradation of the LH wave coupling, as observed both in the Tore Supra and JET tokamaks. The reflection coefficient on the part of the LH launcher magnetically connected to the powered ICRF antenna increases, suggesting a local decrease in the electron density in the connecting flux tubes. This has been confirmed by Langmuir probe measurements on the LH launchers in the latest Tore Supra experiments. Moreover, recent experiments in JET indicate that the LH coupling degradation depends on the ICRF power and its launched k//-spectrum. The 2D density distribution around the Tore Supra ICRF antennas has been modelled with the CELLS-code, balancing parallel losses with diffusive transport and sheath induced ExB convection, obtained from RF field mapping using the ICANT-code. The calculations are in qualitative agreement with the experimental observations, i.e. density depletion is obtained, localised mainly in the antenna shadow, and dependent on ICRF power and antenna spectrum

Additional details

Identifiers

Publishing Information

Journal Title
AIP Conference Proceedings
Journal Volume
694
Journal Issue
1
Journal Page Range
p. 259-262
ISSN
0094-243X
CODEN
APCPCS

Conference

Title
15. topical conference on radio frequency power in plasmas
Dates
19-21 May 2003
Place
Moran, WY (United States)

Optional Information

Notes
(c) 2003 American Institute of Physics
Collaborations
EFDA-JET Contributors