Restricted three-dimensional stellar wind modeling. I - Polytropic case

• 1 March 1975
• journal article
• Published by American Astronomical Society in The Astrophysical Journal
• Vol. 196, 837
• https://doi.org/10.1086/153474

Abstract

Keywords

• RADIAL VELOCITY
• ENERGY
• THREE DIMENSIONAL
• PRESSURE GRADIENT
• MAGNETOHYDRODYNAMICS
• MAGNETIC FIELDS
• MAGNETIC FIELD
• SYMMETRY
• SECULAR VARIATION
• MATHEMATICAL MODEL
• SOLAR WIND
• CONTINUITY EQUATION