The existence of an electron heat pinch has been experimentally investigated in ASDEX-Upgrade in plasmas with strong off-axis electron cyclotron heating (ECH). Localization of 1.6 MW of ECH power at rho_dep = 0.65 in plasmas with low Ohmic power (<100 kW) still resulted in peaked electron temperature (Te) profiles at densities ne0 =2.7x10^19 m^-3 Two out of four gyrotrons were modulated in order to study convective effects also on the Te transient response at different frequencies. Peculiar profiles of the modulation amplitude have been measured, very flat in the region just inside rho_dep (0.3 < rho_tor< 0.65) or even increasing rather than decreasing away from rho_dep on the inner side. The phase profiles instead regularly indicate the propagation of the heat wave in both directions away from rho_dep. Power balance analysis shows that the heat flux in the core region is very close to zero, but uncertainties do not allow a clear determination of its sign. Modelling steady-state and modulation results with an empirical model featuring a diffusive term characterized by a critical gradient length (L_Te = -Te/grad Te) behaviour and a constant Gaussian shaped heat pinch profile allows good reproduction of the data when the region just inside rho_dep is close to the critical threshold and oscillates around it, and a small convective term U=12 m s^-1 is present in the same region. At higher density the Te profile becomes flatter and the amplitude profiles recover the usual shape with stronger decay inside with respect to outside rho_dep. In this case no heat pinch is needed and the plasma goes below the critical threshold inside rho_dep. The results are consistent with the theoretical prediction of a turbulence regulated by a threshold in R/L_Te and a small turbulence generated electron heat pinch term. However initial attempts to perform first principle-based simulations using the quasi-linear electrostatic drift wave Weiland model have failed to reproduce the experimental results.
Investigation of electron heat pinch in ASDEX-Upgrade
Mantica P;
2006
Abstract
The existence of an electron heat pinch has been experimentally investigated in ASDEX-Upgrade in plasmas with strong off-axis electron cyclotron heating (ECH). Localization of 1.6 MW of ECH power at rho_dep = 0.65 in plasmas with low Ohmic power (<100 kW) still resulted in peaked electron temperature (Te) profiles at densities ne0 =2.7x10^19 m^-3 Two out of four gyrotrons were modulated in order to study convective effects also on the Te transient response at different frequencies. Peculiar profiles of the modulation amplitude have been measured, very flat in the region just inside rho_dep (0.3 < rho_tor< 0.65) or even increasing rather than decreasing away from rho_dep on the inner side. The phase profiles instead regularly indicate the propagation of the heat wave in both directions away from rho_dep. Power balance analysis shows that the heat flux in the core region is very close to zero, but uncertainties do not allow a clear determination of its sign. Modelling steady-state and modulation results with an empirical model featuring a diffusive term characterized by a critical gradient length (L_Te = -Te/grad Te) behaviour and a constant Gaussian shaped heat pinch profile allows good reproduction of the data when the region just inside rho_dep is close to the critical threshold and oscillates around it, and a small convective term U=12 m s^-1 is present in the same region. At higher density the Te profile becomes flatter and the amplitude profiles recover the usual shape with stronger decay inside with respect to outside rho_dep. In this case no heat pinch is needed and the plasma goes below the critical threshold inside rho_dep. The results are consistent with the theoretical prediction of a turbulence regulated by a threshold in R/L_Te and a small turbulence generated electron heat pinch term. However initial attempts to perform first principle-based simulations using the quasi-linear electrostatic drift wave Weiland model have failed to reproduce the experimental results.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
