proton velocity
distribution, proton outflow
velocity, electron temperature,
and O VI, Si XII,
and Mg X outflow velocities and densitiesUVCS makes measurements of the solar corona between 2 and 10 solar radii from sun center with high spectral and spatial resolution. From the spectroscopic measurements at ultraviolet wavelengths, the
proton velocity
distribution, proton outflow
velocity, electron temperature,
and O VI, Si XII,
and Mg X outflow velocities and densities O VI, Si XII,
and Mg X velocity distributions, electron density,
and minor ions
densitiesSee also