Evolution of solar magnetic flux

Technical Report · Fri Jun 01 00:00:00 EDT 1984

OSTI ID:5925749

The appearance of solar magnetic flux is discussed both the mechanisms and phenomena associated with flux emergence are considered. The dynamics of solar surface magnetic flux are addressed, including both the transport and structure of magnetic-flux-carrying elements as seen in the chromosphere and corona. The disappearance of magnetic flux from the surface of the Sun is also discussed. Standard solar models representing generally accepted views are considered along with observations which seem to fall outside the scope of these models.

• Research Organization: Maryland Univ., College Park (USA)
• OSTI ID: 5925749
• Report Number(s): N-84-34335
• Country of Publication: United States
• Language: English

Related Subjects

71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
SUN
MAGNETIC FLUX
CHROMOSPHERE
SKYLAB
SOLAR CORONA
SOLAR CYCLE
STAR MODELS
SUNSPOTS
ATMOSPHERES
MAIN SEQUENCE STARS
MATHEMATICAL MODELS
SATELLITES
SOLAR ACTIVITY
SOLAR ATMOSPHERE
STARS
STARSPOTS
STELLAR ACTIVITY
STELLAR ATMOSPHERES
STELLAR CORONAE
640104* - Astrophysics & Cosmology- Solar Phenomena