Spectral diagnostics of an active region observed by the solar euv rocket telescope and spectrograph (serts)

Abstract

The EUV spectrum of a solar active region observed by SERTS-89 is used to estimate physical parameters such as electron density, elemental abundance and inhomogeneity in the emitting source. A total of 13 ions, namely, Ne IV-VI, Mg V-IX, Si VII-X and SX, are studied in the SERTS spectral range 170-450 A, providing plasma diagnostics at temperatures between 105 -106 K. Attention is called to results derived from ion pairs of different elements that are formed over similar temperature regimes, which allow special checks on the standard assumptions of spectral analyses. Some EUV lines, not originally reported in the SERTS-89 spectrum, are shown to have measureable intensities and are indicated for future observations.