Role of Impurity Cyclotron Damping in Ion Heating and RFP Turbulence

نویسندگان

  • P. W. Terry
  • V. Tangri
  • J. S. Sarff
  • G. Fiksel
  • A. F. Almagri
  • Y. Ren
  • S. C. Prager
چکیده

In the reversed field pinch ions are heated anomalously relative to collisional energy exchange with Ohmically heated electrons. The process channels electron energy to ions in a way that is still not understood. Recent observations suggest that impurities are preferentially heated. A theory for ion heating via impurity ioncyclotron-resonant damping of the turbulent energy cascaded from unstable global tearing modes is presented. The theory treats the magnetic turbulence as an Alfvén wave cascade and calculates the rate of damping to impurity ions via cyclotron resonances. The transient temperature rise in sawtooth crashes is modeled from a 0D transport model that accounts for the resonant cyclotron heating, anomalous heat losses, and collisional equipartition between impurities, bulk ions, electrons, and parallel and perpendicular temperatures. The larger fluctuation level at lower impurity cyclotron frequencies and the multiplicity of impurity resonances lead to heating rates that are consistent with experiment. Dependencies on temperature, density, and magnetic fluctuation level are described. The magnetic fluctuation spectrum is modeled for dissipation associated with viscosity, resistivity and cyclotron resonances. When Visco-resistive dissipation range spectra derived for MHD turbulence are fit to the MST spectrum, the viscosity and resistivity inferred are much larger than the experimental values. Analysis of asymmetry in the toroidal wavenumber spectrum suggests that additional dissipation is coming from the cyclotron resonance with impurity ions.

برای دانلود رایگان متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

A Model of Turbulence in Magnetized Plasmas: Implications for the Dissipation Range in the Solar Wind

This paper studies the turbulent cascade of magnetic energy in weakly collisional magnetized plasmas. A cascade model is presented, based on the assumptions of local nonlinear energy transfer in wavenumber space, critical balance between linear propagation and nonlinear interaction times, and the applicability of linear dissipation rates for the nonlinearly turbulent plasma. The model follows t...

متن کامل

The role of damped Alfvén waves on magnetospheric accretion models of young stars

We examine the role of Alfvén wave damping in heating the plasma in the magnetic funnels of magnetospheric accretion models of young stars. We study four different damping mechanisms of the Alfvén waves: nonlinear, turbulent, viscous-resistive and collisional. Two different possible origins for the Alfvén waves are discussed: 1) Alfvén waves generated at the surface of the star by the shock pro...

متن کامل

Alfvénic Turbulence in the Extended Solar Corona: Kinetic Effects and Proton Heating

We present a model of magnetohydrodynamic (MHD) turbulence in the extended solar corona that contains the effects of collisionless dissipation and anisotropic particle heating. Recent observations have shown that preferential heating and acceleration of positive ions occur in the first few solar radii of the high-speed solar wind. Measurements made by the Ultraviolet Coronagraph Spectrometer ab...

متن کامل

Poloidal variation of high-Z impurity density due to hydrogen minority ICRH on Alcator C-Mod

In the Alcator C-Mod tokamak, strong, steady-state variations of molybdenum density within a flux surface are routinely observed in plasmas using hydrogen minority ion cyclotron resonant heating. In/out asymmetries, up to a factor of 2, occur with both inboard and outboard accumulation depending on the major radius of the minority resonance layer. These poloidal variations can be attributed to ...

متن کامل

Fast Compressional Alfven Waves in a Tokamak

Enhancement of cyclotron damping is theoretically evaluated based upon the wave E-field polarization which is modified by the two-ion hybrid resonance. The degree of enhancement and its asymmetry about the plasma center is consistent with experimental observations. The enhancement factor is very large at low plasma densities at which most of the past damping strength measurements have been repo...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

عنوان ژورنال:

دوره   شماره 

صفحات  -

تاریخ انتشار 2010