The innermost corona observed at the 1973 June 30 eclipse

Abstract

Slitless flash spectrograms in heights below 8000 km above the solar limb were obtained by the

V. Solar Maximun Analysis

“…A study of growing loops at various temperatures (Ha to X-rays) has revealed that the (post-) flare loops must be shrinking and their density must be increasing during their cooling (Svestka et al, 1987). Indeed, Hanaoka et al (1986) found electron densities of 8 x 10» and 10"-cm-3 in the hot and cold loops, respectively. According to Sakurai (1985), potential-field modeling gives a reasonable fitting in the case of two-ribbon flares ; but other kinds of flares, and The largest number of spacecraft observational studies were related to solar flares.…”