Magnetic field morphology in the upper layers

Details Magnetic field morphology in the upper layers Magnetic field morphology in the upper layers

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987nascp2483....1p&link_type=abstract

In NASA-Goddard Space Flight Center, Theoretical Problems in High Resolution Solar Physics, 2 p 1-13 (SEE N88-11609 02-92)

Physics

2

Magnetic Field Configurations, Magnetic Flux, Morphology, Sunspots, Thermodynamic Properties, Chromosphere, Gas Pressure, Magnetostatic Fields, Photosphere, Solar Gravitation, Solar Physics

Scientific paper

The authors examine some basic properties of emerged magnetic flux concentrations, with emphasis on the interplay between the magnetic and thermodynamic structure in the region between the photosphere and the transition zone. The discussion is limited to the gross behaviour of those phenomena that may be reasonably regarded as quasi-static, such as the longer-lived sunspots, pores, and some smaller magnetic flux tubes. Substructure and dynamic phenomena are not considered.

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