1. RADIO-FREQUENCY HEATING IN STRAIGHT FIELD LINE MIRROR NEUTRON SOURCE V.E.Moiseenko 1,2, O.Ågren 2, K.Noack 2 1 Kharkiv Institute of Physics and Technology, Ukraine 2 Uppsala University, Sweden

2. OUTLINE SFLM FDS Scenarios for ICRH Numerical model Parameters of calculations Calculation results Conclusions

3. SFLM FDS Usage of a SFLM is beneficial to localize the fusion neutron flux to the SFLM part of the device which is surrounded by a fission mantle. The device would be capable to operate continuously. It is expected that full control on plasma could be achieved. The device is relatively simple.

4. Scenarios for ICRH Minority heating: Wave is launched by antenna near ut-off Wave does not propagates to high field side reflecting from cut-off FMSW then converts to FAW Alfven resonances are also excited FAW is absorbed owing to cyclotron damping Second harmonic heating: The same, but no conversion to FAW and no Alfven resonances Conversion to IBW is possible RF field forms a standing wave in radial direction and propagates along magnetic field towards midplane V.E. MOISEENKO, O. AGREN, Phys. Plasmas 12, ID 102504 (2005). V.E. MOISEENKO, O. AGREN, Phys. Plasmas 14, ID 022503 (2007).

5. Scenarios for ICRH (cont.) Power Re Ex Im Ex Re Ey Im Ey The SFLM neutron source has a substantially smaller size than a fusion reactor machine. In this situation the fast magnetosonic wave which is excited by the antenna makes fewer oscillations across the magnetic field. The width of the ion cyclotron zone becomes smaller owing to the sharper gradients of the magnetic field magnitude along magnetic field lines. The last factor is softened by a smaller mirror ratio. Reactor Neutron source Second harmonic calculation

6. Numerical model Zero electron mass approximation is chosen in which the parallel component of the electric field is neglected in Maxwell’s operator WKB formulas for cyclotron damping: fundamental harmonic, Second harmonic V.E. MOISEENKO, O. AGREN, Phys. Plasmas 14, ID 022503 (2007). Boundary conditions

7. Parameters of calculations

8. Calculation results (minority heating) Dependence of the absorption (solid line) and shine-through (dashed line) resistances on RF heating frequency. Dependence of the absorption and shine- through resistances on plasma density.

9. Calculation results (minority heating) Dependence of the absorption and shine-through resistances on antenna location.

10. Calculation results (second harmonic heating) Dependence of the absorption (solid line) and shine-through (dashed line) resistances on RF heating frequency. Dependence of the absorption and shine- through resistances on plasma density.

11. Calculation results (second harmonic heating) Dependence of the absorption and shine-through resistances on antenna location. Dependence of the absorption and shine-through resistances on tritium thermal velocity.

12. CONCLUSIONS The calculations indicate good performance of deuterium minority heating at fundamental ion cyclotron frequency. The heating is weakly sensitive to the ion temperature and, therefore, has no start-up problem. The sensitivity to other factors, e.g. plasma density, antenna location etc., is not critical. The second harmonic heating of tritium is more delicate. It is every time accompanied by a noticeable shine-through of the wave energy to the middle part of the trap where the wave would be absorbed by the deuterium at the second harmonic ion cyclotron zone. Most of the remaining wave energy may also be absorbed at the second harmonic tritium resonance zone near the opposite mirror. The calculations predict relatively sensitive dependence on plasma density, antenna location and tritium temperature. However, if the necessary conditions are provided this heating is satisfactorily efficient.