Other
Scientific paper
Jun 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987sao..reptr....w&link_type=abstract
Semiannual Progress Reports, 1 May 1986 - 30 Apr. 1987 Smithsonian Astrophysical Observatory, Cambridge, MA.
Other
Astronomical Models, Heliosphere, Magnetohydrodynamic Waves, Plasma Heating, Shock Heating, Solar Corona, Solar Wind, Boundary Value Problems, Line Spectra, Lyman Alpha Radiation, Magnetic Fields, Plasma Diagnostics, Thermal Conductivity, Time Dependence
Scientific paper
Selected problems concerned with the important physical processes that occur in the corona and solar wind acceleration region, particularly time dependent phenomena were studied. Both the physics of the phenomena and the resultant effects on observational signatures, particularly spectroscopic signatures were also studied. Phenomena under study include: wave motions, particularly Alfven and fast mode waves; the formation of standing shocks in the inner heliosphere as a result of momentum and/or heat addition to the wind; and coronal transient phenomena where momentum and/or heat are deposited in the corona to produce transient plasma heating and/or mass ejection. The development of theoretical models for the inner heliosphere, the theoretical investigation of spectroscopic plasma diagnostics for this region, and the analysis of existing skylab and other relevant data are also included.
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