Results 61 to 70 of about 2,917 (170)
Theory of Stellar Oscillations [PDF]
, 2017 Lecture presented at the IVth Azores International Advanced School in Space Sciences on "Asteroseismology and Exoplanets: Listening to the Stars and Searching for New Worlds" (arXiv:1709.00645), which took place in Horta, Azores Islands, Portugal in July ...
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Collisionless microinstabilities in stellarators I - analytical theory of trapped-particle modes
, 2013 This is the first of two papers about collisionless, electrostatic micro-instabilities in stellarators, with an emphasis on trapped-particle modes. It is found that, in so-called maximum-$J$ configurations, trapped-particle instabilities are absent in ...
Helander, P. +2 more
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Contributions of plasma physics to chaos and nonlinear dynamics
, 2016 This topical review focusses on the contributions of plasma physics to chaos and nonlinear dynamics bringing new methods which are or can be used in other scientific domains.
Escande, Dominique
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The theory of stellar winds [PDF]
Astrophysics and Space Science, 2011 We present a brief overview of the theory of stellar winds with a strong emphasis on the radiation-driven outflows from massive stars. The resulting implications for the evolution and fate of massive stars are also discussed. Furthermore, we relate the effects of mass loss to the angular momentum evolution, which is particularly relevant for the ...
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Statistical Analysis of Plasma Dynamics in Gyrokinetic Simulations of Stellarator Turbulence. [PDF]
Entropy (Basel), 2023 Papadopoulos AD +4 more
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Existence of weakly quasisymmetric magnetic fields without rotational transform in asymmetric toroidal domains. [PDF]
Sci Rep, 2022 Sato N.
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The case of the trapped singularities [PDF]
, 2004 A case study in bifurcation and stability analysis is presented, in which reduced dynamical system modelling yields substantial new global and predictive information about the behaviour of a complex system.
Ball, R.
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Stellar Turbulent Convection. I. Theory
The Astrophysical Journal, 1998 The description of stellar turbulent convection requires a minimum of five coupled, time-dependent, nonlocal, differential equations for the five variables: turbulent kinetic energy, turbulent potential energy, turbulent pressure, convective flux, and energy dissipation. Any fewer number of equations makes the model local. In this paper, we present the
V. M. Canuto, M. Dubovikov
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Pulsation Theory and Stellar Structure [PDF]
International Astronomical Union Colloquium, 1993 AbstractObserved periods of pulsating stars provide information about the properties of the stars. As examples I here consider double-mode pulsators, solar-like oscillations and δ Scuti stars. The ongoing expansion in the observational efforts in this area may be expected to lead to increasingly detailed tests of stellar evolution theory.
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Demonstration of reduced neoclassical energy transport in Wendelstein 7-X. [PDF]
Nature, 2021 Beidler CD +39 more
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