Published May 2010 | Version v1
Journal article

Probing plasma turbulence by modulating the electron temperature gradient

  • 1. General Atomics, P.O. Box 85608, San Diego, California 92186-5608 (United States)
  • 2. University of California-San Diego, 9500 Gilman Drive, La Jolla, California 92093 (United States)
  • 3. University of California-Los Angeles, 405 Hilgard Avenue, Los Angeles, California 90095 (United States)
  • 4. Oak Ridge Institute for Science and Education, 130 Badger Avenue, Oak Ridge, Tennessee 37830-6218 (United States)
  • 5. University of Texas-Austin, P.O. Box 8028, Austin, Texas 78713 (United States)
  • 6. University of Wisconsin at Madison, 337 Engineering Research Building, 1500 Engineering Drive, Madison, Wisconsin 53706 (United States)

Description

The local value of a/LTe, a turbulence drive term, was modulated with electron cyclotron heating in L-mode discharges on DIII-D [J. L. Luxon, Nucl. Fusion 42, 614 (2002)] and the density and electron temperature fluctuations in low, intermediate, and high-k regimes were measured and compared with nonlinear gyrokinetic turbulence simulations using the GYRO code [J. Candy and R. E. Waltz, J. Comput. Phys. 186, 545 (2003)]. The local drive term at ρ∼0.6 was reduced by up to 50%, which produced comparable reductions in electron temperature fluctuations at low-k. At intermediate k, kθ∼4 cm-1 and kθρs∼0.8, a very interesting and unexpected result was observed where density fluctuations increased by up to 10% when the local drive term was decreased by 50%. Initial comparisons of simulations from GYRO with the thermal diffusivity from power balance analysis and measured turbulence response are reported. Simulations for the case with the lowest drive term are challenging as they are near the marginal value of a/LTe for trapped electron mode activity.

Additional details

Identifiers

Publishing Information

Journal Title
Physics of Plasmas
Journal Volume
17
Journal Issue
5
Journal Page Range
p. 056105-056105.10
ISSN
1070-664X
CODEN
PHPAEN

Optional Information

Notes
(c) 2010 American Institute of Physics