CHIANTI

An Atomic Database for Spectroscopic Diagnostics of Astrophysical Plasmas.


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George Mason University (USA) - University of Michigan (USA) - University of Cambridge (UK)

VERSION 8.0


Different colours indicate different isoelectronic sequences.

H I
He I II
Li
Be
B
C II III IV V VI
N I II III IV V VI VII
O I II III IV V VI VII VIII
F
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 III IV X XI XII XIV XVI XVII
Ar III IV V VII VIII IX X XI XII XIII XIV XV XVI XVII XVIII
K V VI IX XI XII XIII XIV XV XVI XVII XVIII XIX
Ca II V VI VII VIII IX X XI XII XIII XIV XV XVI XVII XVIII XIX XX
Sc
Ti XI XII XIV XV XVI XVII XVIII XIX XX
V
Cr VII VIII IX XIII XIV XVI XVII XVIII XIX XX XXI XXII
Mn VIII IX X XV XVII XVIII XIX XX XXI XXII XXIII
Fe II IV V 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 II XI XII XIII XIV XV XVI XVII XVIII XIX XX XXI XXII XXIII XXIV XXV XXVI XXVII XXVIII
Cu
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