Abstract:
Multi-slit spectra of (Fe XIV 5303) plus neon comparisons were successfully obtained on February 16, 1980 at the Japal-Rangapur site. The objective is to confirm our previous results of March 1970 and June 1973, viz. that the corona is remarkably quiescent (random velocities = 0.5 Km/s r.m.s.) and that the majority of detected flows at 0.3 - 1.0 Ro are directed towards the Sun.
