The Astrophysical Journal Supplement Series · 2008 · 161 citations · 21 references
Natural SciencesAstronomyPhysicsSolar AstronomySpectroscopyUltraviolet AstronomySolar Active RegionsSolar ObservationsSolar PhysicsSolar SpectroscopySpectral Line AstronomyUltraviolet SpectroscopyExtreme Ultraviolet EmissionExtreme Ultraviolet Solar ObservationsExtreme Ultraviolet SpectroscopyLine List ConstructionSolar Emission LinesSolar Plasma PhysicsSolar Ultraviolet Emission Lines
We present spectral line wavelengths, identifications, and intensities in the 171-211 and 245-291 Å ranges from five solar plasma regions recorded by the Extreme-Ultraviolet Imaging Spectrometer (EIS) on Hinode. The recorded data were emitted from a quiet region, two active areas on the solar disk, a limb region, and a region 20'' above the limb. The line list contains 500 lines of which 55% were identified with previously known transitions. Although the EIS spectral coverage is limited to two ranges approximately 40 Å wide, the identified lines belong to a total of 56 ions from 15 elements.
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CHIANTI - an atomic database for emission lines
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The Hinode (Solar-B) Mission: An Overview
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