Exploration of the Solar-Stellar Connection at High Spectral Resolution with the Ultraviolet Spectrometer and Polarimeter,and Studies of Thermal Bifurcation at the Photosphere-Chromosphere Interface.

摘要

The dynamics of high-excitation plasma in the 100,000 K transition zones of stars of late spectral type, as observed with the International Ultraviolet Explorer, was compared with the radial gas velocities of individual structural features of the solar TZ, as observed with high spatial resolution by the UVSP on the Solar Maximum Mission. The 4th-positive system of carbon monoxide in the quiet sun and in active regions was studied in order to explore the properties of thermal inhomogeneities at the critical interface between the photosphere and chromosphere.