@article {10.3844/pisp.2014.136.139,
article_type = {journal},
title = {ON SOLUTIONS IN THE HYDRODYNAMIC APPROXIMATION OF SOLAR AND STELLAR WINDS WITH VISCOSITY},
author = {Koumantos, Panagiotis N. and Pavlakos, Panaiotis K. and Moussas, Xenophon D.},
volume = {5},
year = {2014},
month = {May},
pages = {136-139},
doi = {10.3844/pisp.2014.136.139},
url = {https://thescipub.com/abstract/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.},
journal = {Physics International},
publisher = {Science Publications}
}