Results 1 to 10 of about 5,819 (232)

Confirmation of the topology of the Wendelstein 7-X magnetic field to better than 1:100,000 [PDF]

open access: yesNature Communications, 2016
Early stellarator designs suffered from high particle losses, an issue that can be addressed by optimization of the coils. Here the authors measure the magnetic field lines in the Wendelstein 7-X stellarator, confirming that the complicated design of the
T. Sunn Pedersen   +9 more
doaj   +2 more sources

Critical gradient turbulence optimization toward a compact stellarator reactor concept

open access: yesPhysical Review Research, 2023
Integrating turbulence into stellarator optimization is achieved by targeting the onset for the ion-temperature-gradient mode, highlighting effects of field line curvature, parallel connection length, local magnetic shear, and flux surface expansion. The
G. T. Roberg-Clark   +5 more
doaj   +2 more sources

Stellar Structure [PDF]

open access: yesNature, 1931
Es wird der Meinungsaustausch zwischen Milne, Eddington und Jeans dargelegt, der am 9. Januar d. J. während der Sitzung der Royal Astronomical Society in London stattfand. Milne erklärte, daß der Hauptzweck seiner Theorie des Sterninnerns in der Befreiung der Eddingtonsehen Theorie von ad hoc-Hypothesen liege.
Russell, H. N., Atkinson, R. d'E.
  +8 more sources

Kinetic simulations of scrape-off layer physics in the DIII-D tokamak

open access: yesNuclear Materials and Energy, 2017
Simulations using the fully kinetic code XGCa were undertaken to explore the impact of kinetic effects on scrape-off layer (SOL) physics in DIII-D H-mode plasmas.
R.M. Churchill   +7 more
doaj   +1 more source

Physics-regularized neural network of the ideal-MHD solution operator in Wendelstein 7-X configurations

open access: yesNuclear Fusion, 2023
The computational cost of constructing 3D magnetohydrodynamic (MHD) equilibria is one of the limiting factors in stellarator research and design. Although data-driven approaches have been proposed to provide fast 3D MHD equilibria, the accuracy with ...
Andrea Merlo   +5 more
doaj   +1 more source

Coarse-grained gyrokinetics for the critical ion temperature gradient in stellarators

open access: yesPhysical Review Research, 2022
We present a modified gyrokinetic theory to predict the critical gradient that determines the linear onset of the ion temperature gradient (ITG) mode in stellarator plasmas.
G. T. Roberg-Clark   +2 more
doaj   +1 more source

Stellar ages from stellar rotation [PDF]

open access: yesProceedings of the International Astronomical Union, 2008
AbstractOur ability to determine stellar ages from measurements of stellar rotation, hinges on how well we can measure the dependence of rotation on age for stars of different masses. Rotation periods for stars in open clusters are essential to determine the relations between stellar age, rotation, and mass.
openaire   +2 more sources

Stellar Motions and Stellar Dynamics [PDF]

open access: yesTransactions of the International Astronomical Union, 1962
The texts of the twelve prepared contributions, often in abbreviated form, are given first; they are followed by a summary of the discussion on all the contributions considered together.
A. Blaauw   +8 more
openaire   +1 more source

Real-time wall conditioning by controlled injection of boron and boron nitride powder in full tungsten wall ASDEX Upgrade

open access: yesNuclear Materials and Energy, 2019
In ASDEX Upgrade with full-tungsten wall, boronization is an important tool to control tungsten sources and allow reliable operation at low collisionality. The duration of the beneficial effects is limited by the erosion of the boron layer, in particular
A. Bortolon   +12 more
doaj   +1 more source

Stellar Structure and the Origin of Stellar Energy* [PDF]

open access: yesNature, 1930
THE generally accepted theory of the internal conditions in stars, due to Sir A. S. Eddington, depends largely on a special solution of the fundamental equations, and according to this a definite calculable luminosity is associated with a given mass. If this were the only solution of the equations it would conflict, as I have repeatedly shown in recent
openaire   +2 more sources

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