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CHIANTI-An Atomic Database for Emission Lines. V. Comparison with an Isothermal Spectrum Observed with SUMER
DOI: 10.1086/337949 Bibcode: 2002ApJS..139..281L

Dere, K. P.; Landi, E.; Feldman, U.

CHIANTI is a database consisting of critically evaluated atomic data and transition probabilities necessary to analyze spectral observations of optically thin plasmas. Previous papers described the content of the database and compared it to a solar active region spectrum between 170 and 450 Å. The aim of the present paper is to compare CHIANTI pre…

2002 The Astrophysical Journal Supplement Series
SOHO 110