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ISSN: 1948-9803 (Print)
ISSN: 1948-9811 (Online)
Research Article Open Access

ON SOLUTIONS IN THE HYDRODYNAMIC APPROXIMATION OF SOLAR AND STELLAR WINDS WITH VISCOSITY

Panagiotis N. Koumantos1, Panaiotis K. Pavlakos2 and Xenophon D. Moussas1
  • 1 Department of Physics, National and Kapodistrian University of Athens, Panepistimiopolis GR-15783 Athens, Greece
  • 2 Department of Mathematics, National and Kapodistrian University of Athens, Panepistimiopolis GR-15784 Athens, Greece

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.

Physics International
Volume 5 No. 2, 2014, 136-139

DOI: https://doi.org/10.3844/pisp.2014.136.139

Submitted On: 4 May 2014 Published On: 30 May 2014

How to Cite: 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

Open AccessCopyright: © 2014 Panagiotis N. Koumantos, Panaiotis K. Pavlakos and Xenophon D. Moussas. This is an open access article distributed under the terms of the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original author and source are credited.

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Keywords

  • Solar and Stellar Winds
  • Hydrodynamics
  • Navier-Stokes Equations
  • Evolution Equations