ON SOLUTIONS IN THE HYDRODYNAMIC APPROXIMATION OF SOLAR AND STELLAR WINDS WITH VISCOSITY
Panagiotis N. Koumantos1, Panaiotis K. Pavlakos2 & Xenophon D. Moussas1 Show affiliations
- Department of Physics, National and Kapodistrian University of Athens, Panepistimiopolis GR-15783 Athens, Greece
- Department of Mathematics, National and Kapodistrian University of Athens, Panepistimiopolis GR-15784 Athens, Greece
Physics International, Volume 5, Issue 2, pp. 136–139 · doi.org/10.3844/pisp.2014.136.139
Abstract
In this article we present some results in existence and uniqueness of strong and classical solutions of the hydrodynamic equations modeling solar and stellar winds. The system of Navier-Stokes equations for solar and stellar winds is considered in its corresponding differential evolution equation form (d/dt+A)υ(t) = F(υ(t), t), where F is a given non-linear function and -A is the infinitesimal generator of the analytic semigroup arises by the hydrodynamic Stokes operator.
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Koumantos, P. N., Pavlakos, P. K. & Moussas, X. D. (2014). ON SOLUTIONS IN THE HYDRODYNAMIC APPROXIMATION OF SOLAR AND STELLAR WINDS WITH VISCOSITY. Physics International, 5(2), 136–139. https://doi.org/10.3844/pisp.2014.136.139
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