Results 71 to 80 of about 249 (184)
ABSTRACT: We study the weakly nonlinear evolution of acoustic instability of a plane‐parallel polytrope with thermal dissipation in the form of Newton's law of cooling. The most unstable horizontal wavenumbers form a band around zero and this permits the development of a nonlinear pattern theory leading to a complex Ginzburg‐Landau equation (CGLE ...
Umurhan, O. M., Tao, L., Spiegel, E. A.
openaire +3 more sources
Precise stellarator quasi-symmetry can be achieved with electromagnetic coils. [PDF]
Wechsung F +4 more
europepmc +1 more source
Ultrahigh neutral pressures in the sub-divertor of the Large Helical Device
In the Large Helical Device (LHD) a low temperature mode (LTM) of the helical divertor was discovered. It combines particle detachment and very large sub-divertor pressures up to 1.4 Pa. During the LTM, the electron temperature in the divertor was in the
U. Wenzel +8 more
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Statistical Analysis of Plasma Dynamics in Gyrokinetic Simulations of Stellarator Turbulence. [PDF]
Papadopoulos AD +4 more
europepmc +1 more source
A model for Alfvén-eigenmode-induced transport of fast ions in stellarators
A novel model for Alfvén-eigenmode-induced transport of fast ions in stellarators is introduced. A variety of reduced transport models exists for tokamaks, but nothing comparable currently exists for stellarators.
C. Slaby +4 more
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Exposure of tungsten heavy alloys at high thermal loads in LHD
Tungsten has been considered a plasma-facing material in a future fusion reactor because of its low sputtering yield and low fuel retention. It has been examined in several tokamaks.
Chandra Prakash Dhard +5 more
doaj +1 more source
MONKES is a new neoclassical code for the evaluation of monoenergetic transport coefficients in stellarators. By means of a convergence study and benchmarks with other codes, it is shown that MONKES is accurate and efficient.
F.J. Escoto +4 more
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Stellar Magnetism affects all spectral types and exists and varies throughout the evolution of stars. Magnetic fields can affect not only the interior of stars, but also their circumstellar environments. In this chapter, we concentrate on the magnetic fields that can be measured at the surface of stars through the influence of the Zeeman effect on ...
Petit, Veronique, Oksala, Mary E.
openaire +2 more sources
Physics of magnetic confinement fusion
Fusion is the energy source of the universe. The local conditions in the core of the Sun allow the transfer of mass into energy, which is finally released in the form of radiation.
Wagner F.
doaj +1 more source
Review of plasma turbulence experiments. [PDF]
Fujisawa A.
europepmc +1 more source

