EUV emission lines and diagnostics observed with Hinode/EIS

By Peter R. Young, Del Zanna, Helen E. Mason, K. Dere, E. Landi, M. Landini, G. Doschek, Charles M. Brown, L. Culhane, L. Harra and 2 more. 2007

170 citations recorded by the source corpus.

Quiet Sun and active region spectra from the Hinode/EIS instrument are presented, and the strongest lines from different temperature regions discussed. A list of emission lines recommended to be included in EIS observation studies is presented based on analysis of blending and diagnostic potential using the CHIANTI atomic database. In addition we identify the most useful density diagnostics from the ions covered by EIS.

Subfields: Astronomy and Astrophysics, Atomic and Molecular Physics, and Optics, Mechanics of Materials

View Paper: https://www.semanticscholar.org/paper/c1420b057249b756c87e31608b0f75c005a4b835

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Citations in the corpus

VELOCITY CHARACTERISTICS OF EVAPORATED PLASMA USING HINODE/EUV IMAGING SPECTROMETER (2009, background): “The Fe XXIII and Fe XXIV velocity maps were formed using a different method, as true velocity maps become distorted by blended lines in regions where cooler emission begins to dominate.”
High-precision density measurements in the solar corona I. Analysis methods and results for Fe XII and Fe XIII (2008, methodology): “18 was suggested as a possible cause of this (Young et al. 2007b).”
The multi-thermal emission in solar active regions (2013, background): “Note that the Caxvii 192.8 Å line has instead at 3 MK a predicted emissivity of only 1% its peak value at 6 MK.”