CHIANTI

An Atomic Database for Spectroscopic Diagnostics of Astrophysical Plasmas.

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Naval Research Laboratory (USA) - Rutherford Appleton Laboratory (UK)
University of Cambridge (UK) - George Mason University (USA) - Universita' degli Studi di Firenze (Italy)

VERSION 5.1

Below are links to the data, references, and tables of most prominent lines.

Different colours indicate different isoelectronic sequences.

H I
He I II
C II III IV V VI
N I II III IV V VI VII
O II III IV V VI VII VIII
Ne II III IV V VI VII VIII IX X
Na III IV V VI VII VIII IX X XI
Mg II IV V VI VII VIII IX X XI XII
Al II III V VI VII VIII IX X XI XII XIII
Si II III IV V VI VII VIII IX X XI XII XIII XIV
P V VII VIII IX X XI XII XIII XIV XV
S II III IV V VI VII VIII IX X XI XII XIII XIV XV XVI
Cl II X XI XII XIV XVI XVII
Ar IV VII VIII IX X XI XII XIII XIV XV XVI XVII XVIII
K V IX XI XII XIII XIV XV XVI XVII XVIII XIX
Ca VII VIII IX X XI XII XIII XIV XV XVI XVII XVIII XIX XX
Ti XI XII XIV XV XVI XVII XVIII XIX XX
Cr XIII XIV XVI XVII XVIII XIX XX XXI XXII
Mn XV XVII XVIII XIX XX XXI XXII XXIII
Fe II VI VII VIII IX X XI XII XIII XIV XV XVI XVII XVIII XIX XX XXI XXII XXIII XXIV XXV XXVI
Co XVII XIX XX XXI XXII XXIII XXIV XXV
Ni XII XIII XV XVI XVII XVIII XIX XX XXI XXII XXIII XXIV XXV XXVI XXVII XXVIII
Zn XX XXIII XXIV XXV XXVII XXVIII

Ions that produce satellite lines

C IV V
N V VI
O VI VII
Ne VIII IX
Mg X XI
Al XI XII
Si XII XIII
S XIV XV
Ar XVI XVII
Ca XVIII XIX
Fe II III IV V VI VII VIII IX X XI XII XIII XIV XV XVI XVII XVIII XIX XX XXI XXII XXIII XXIV XXV
Ni XXVI XXVII

Page designed and last modified by Giulio Del Zanna on Wed Sep 14 15:42:55 2005
Last revised by G. Del Zanna on 4-Sep-2009