Structure and dynamics of coronal plasmas

Physics

Scientific paper

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Solar Corona, Chromosphere, Plasma Dynamics, Solar Magnetic Field, Solar Physics, Absorption Spectra, X Rays, Magnetic Flux

Scientific paper

Progress for the period July 1995 - June 1996 included work on the differential magnetic field shear in an active region; observations and modeling of the solar chromosphere seen in soft X-ray absorption by NIXT; and modeling magnetic flux emergence. These were the subjects of three papers. The plans for the current year include projects on a converging flux model for point-like brightenings around sunspots, and difficulties in observing coronal structure.

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