Sep 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990runy.reptq....t&link_type=abstract
Final Technical Report, 1 Oct. 1978 - 30 Sep. 1990 Rochester Univ., NY. Dept. of Mechanical Engineering.
Physics
Magnetic Flux, Seismology, Solar Magnetic Field, Solar Physics, Sun, Sunspots, Dynamic Characteristics, Gas Flow, Mathematical Models, Oscillations, Siphons
Scientific paper
The goal of this research was the understanding of the various oscillatory, transient, and quasi-steady motions in sunspots and the basic structure of a sunspot. The research involved both theoretical modeling (based on thermohydrodynamic theory) and observations of dynamical phenomena in sunspots. The principal topics of the research were sunspot seismology (the interaction of solar p-modes with a sunspot as a probe of the subsurface structure of a sunspot); three minute umbral oscillations and their relation to the structure of the umbral atmosphere; siphon flows in isolated magnetic flux tubes and their relation to the photospheric Evershed flow and to intense magnetic elements outside of sunspots; and more general theoretical work on magneto-atmospheric waves. Here, a summary of results is given.
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