A model for the formation of solar prominences

• 1 September 1991
• journal article
• Published by American Astronomical Society in The Astrophysical Journal
• Vol. 378, 372-377
• https://doi.org/10.1086/170437

Abstract

Keywords

• CHROMOSPHERE
• SOLAR ACTIVITY
• SOLAR CORONA
• SOLAR PROMINENCES
• STELLAR MODELS
• FINE STRUCTURE
• H ALPHA LINE
• SOLAR WIND