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- W1570994906 abstract "The Solar Ultraviolet Measurements of Emitted Radiation (SUMER) spectrometer aboard the Solar and Heliospheric Observatory (SOHO) recorded a large number of spectra in the 500-1600 A region. Many of the detected spectral lines have been identified as transitions in ions from elements with low-to-moderate atomic numbers (Z ≤ 20). However, a substantial number of lines remained unidentified. We postulated that some of the unidentified lines are transitions between excited configurations in Fe+7. Unfortunately, Cr+5 was the last ion in the K I isoelectronic sequence where the envisioned types of transitions were previously identified. In this paper we report new identifications, in laboratory-generated spectra, of transitions between excited configurations in Mn+6 and Fe+7, two additional ions along the K I isoelectronic sequence. Since the elemental abundance of manganese in the solar atmosphere is very low, no Mn VII lines were identified in the SUMER spectra; however, the laboratory-identified Fe VIII lines were found to be present in the SUMER quiet-Sun spectra recorded above the solar limb and in sunspot spectra recorded on the solar disk." @default.
- W1570994906 created "2016-06-24" @default.
- W1570994906 creator A5064460256 @default.
- W1570994906 creator A5075817846 @default.
- W1570994906 date "2003-09-20" @default.
- W1570994906 modified "2023-10-14" @default.
- W1570994906 title "New Identifications of Mn<scp>vii</scp>and Fe<scp>viii</scp>Lines Belonging to Transitions of the Type 3<i>p</i><sup>6</sup>4<i>p</i>–3<i>p</i><sup>6</sup>4<i>d</i>and 3<i>p</i><sup>5</sup>3<i>d</i><sup>2</sup>–3<i>p</i><sup>6</sup>4<i>d</i>" @default.
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- W1570994906 doi "https://doi.org/10.1086/377300" @default.
- W1570994906 hasPublicationYear "2003" @default.
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