Abstract
The ordinary-extraordinary (O-X) mode conversion is modeled with the aid of a 2D full-wave code in the Pegasus toroidal experiment as a function of the launch angles. It is shown how the shape of the plasma density profile in front of the antenna can significantly influence the mode conversion efficiency and, thus, the generation of electron Bernstein waves (EBWs). It is therefore desirable to control the density profile in front of the antenna for successful operation of an EBW heating and current drive system. On the other hand, the conversion efficiency is shown to be resilient to vertical displacements of the plasma as large as 10 cm.
Original language | English |
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Article number | 082501 |
Journal | Physics of Plasmas |
Volume | 18 |
Issue number | 8 |
DOIs | |
State | Published - Aug 2011 |
Externally published | Yes |
Funding
Authors A. Köhn and J. Jacquot wish to express their gratitude towards the Erasmus Mundus program for financial support during their visit to the University of Wisconsin–Madison.
Funders | Funder number |
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Erasmus Mundus | |
University of Wisconsin–Madison |