David J. Jeffery
2013 January 1
Here yours truly puts online some useful Grotrian diagrams for which permission is obtained.
There arn't many---only 1, in fact.
What yours truly has done in other cases is simply made placeholder images to link directly to the images that are online.
Most of these come from the book Partial Grotrian Diagrams of Astrophysical Interest, 1968 (Washington, D.C.: GPO) (hereafter Moore & Merrill (1968)) by Charlotte E. Moore (1898--1990) and Paul W. Merrill (1887--1961).
This book's Grotrian diagrams have no permission to be shown it seems.
Moore & Merrill (1968) is a publication of the US Government Printing Office (GPO). GPO publications are generally public domain: see GPO: Public Domain & Copyright Notice. However, those GPO publications with the a that material has been reprinted with permission of a copyright holder require the permission of the copyright holder for that material.
Moore & Merrill (1968) has almost all material reprinted from a publication of the Carnegie Institution for Science (CIFS): see CIFS Monograph Series 610.
So the Moore & Merrill (1968) Grotrian diagrams cannot be reproduced as far as yours truly knows.
However, the diagrams are easily available and printable for free at the link Moore & Merrill (1968), but they shouldn't displayed by others online without some explict permission.
Maybe they could be displayed under fair use, but it seems unlikely.
Maybe someday there will be a general permission to display them, but until that day we can only link to Moore & Merrill (1968).
It's surprising that there seem to be no great online sources for Grotrian diagrams.
The following on the best I found so far.
Caption: H I Grotrian diagram.
Credit/Permission: Moore, C. E. & Merrill, P. W. 1968, Partial Grotrian Diagrams of Astrophysical Interest, 1968 (Washington, D.C.: GPO), 1968 / ???.
Image linked to Moore & Merrill (1968, p. 4).
Caption: H I
Grotrian diagram.
Below, we consider the
energy levels
and then the atomic line transitions
for the hydrogen atom.
For energy levels, we use ideal
hydrogen atom values.
For
atomic line transitions,
we use values tabulated by the
National Institute of
Science & Technnology (NIST)
(formerly the
National Bureau of Standards (NBS))
(Wiese et al. 1966, p. 2;
Wiese et al. 1966, p. 2, online).
The formula for energies of the
energy levels of the ideal
hydrogen atom
(i.e., the hydrogen atom calculated without
any perturbation corrections included, but using the correct
reduced mass) is
The zero point for the energies is zero energy
of the continuum of energy states available to free (i.e., unbound)
electrons.
To get the energy measured from the
ground state
of the hydrogen atom, one uses formula
E_grd_n = E_n - E_1.
To get the energy of a particular
transition,
one uses the formula
E = E_n_upper - E_n_lower.
In the table below, we show the
hydrogen atom
energy levels.
The
atomic line transitions
for the hydrogen atom are tabulated below.
Credit/Permission: ©
User:Kiko2000,
User:Cepheiden,
2000 /
Creative Commons
CC BY-SA 3.0.
Image linked to Wikipedia.
E_n = -E_ryd*(μ/m_e)/n**2
= -(13.5982 ... eV)/n**2 ,
where
the Rydberg energy = 13.60569253(30) eV,
the reduced Rydberg energy = 13.5982 ... eV,
the electron reduced mass μ=m_e/(1+m_e/m_p)=(0.9994 ...)*m_e,
the electron rest-mass energy m_e=0.510998910(13) MeV,
the proton rest-mass energy m_p=938.272046(21) MeV,
energy is in electron-volts (eV) (1 MeV=10**6 eV),
and
n is the principal quantum number
which runs 1, 2, 3, ... in order of increasing energy level energy for the hydrogen atom.
----------------------------------------------------
Table: Energy Levels of the Ideal Hydrogen Atom
----------------------------------------------------
n E_n E_grd_n
(eV) (eV)
----------------------------------------------------
1 -13.598 ... 0.0000 ...
2 -3.3995 ... 10.1987 ...
3 -1.5109 ... 12.0873 ...
4 -0.8498 ... 12.7483 ...
5 -0.5439 ... 13.0543 ...
6 -0.3777 ... 13.2205 ...
7 -0.2775 ... 13.3207 ...
∞ 0 13.5982 ...
----------------------------------------------------
Table: Atomic Hydrogen Spectral Series
Caption: He I Grotrian diagram.
Credit/Permission: Moore, C. E. & Merrill, P. W. 1968, Partial Grotrian Diagrams of Astrophysical Interest, 1968 (Washington, D.C.: GPO), 1968 / ???.
Image linked to Moore & Merrill (1968, p. 6).
Caption: Li I Grotrian diagram.
For correct orientation: /on image right click/menu/rotate clockwise.
Credit/Permission: Moore, C. E. & Merrill, P. W. 1968, Partial Grotrian Diagrams of Astrophysical Interest, 1968 (Washington, D.C.: GPO), 1968 / ???.
Image linked to Moore & Merrill (1968, p. 8).
Caption: C II Grotrian diagram.
Credit/Permission: Moore, C. E. & Merrill, P. W. 1968, Partial Grotrian Diagrams of Astrophysical Interest, 1968 (Washington, D.C.: GPO), 1968 / ???.
Image linked to Moore & Merrill (1968, p. 20).
Caption: N II Grotrian diagram.
For correct orientation: /on image right click/menu/rotate clockwise.
Credit/Permission: Moore, C. E. & Merrill, P. W. 1968, Partial Grotrian Diagrams of Astrophysical Interest, 1968 (Washington, D.C.: GPO), 1968 / ???.
Image linked to Moore & Merrill (1968, p. 24).
Caption: O I Grotrian diagram.
For correct orientation: /on image right click/menu/rotate clockwise.
Credit/Permission: Moore, C. E. & Merrill, P. W. 1968, Partial Grotrian Diagrams of Astrophysical Interest, 1968 (Washington, D.C.: GPO), 1968 / ???.
Image linked to Moore & Merrill (1968, p. 32).
Caption: Na I Grotrian diagram.
Under almost all conditions, the strongest transition lines of Na I by far are the 2 yellow ground state sodium D lines which constitute a doublet of lines with wavelengths λ=5889.95 Å and λ=5895.92 Å (Wiese et al. 1969, p. 2).
Credit/Permission: University of Wisconsin: Atomic Collisions Group, before or circa 2012 / Public domain is implicitly declared it seems ???.
Image linked to University of Wisconsin: Atomic Collisions Group: Stuff to Download.
Caption: Mg I Grotrian diagram.
For correct orientation: /on image right click/menu/rotate clockwise.
Credit/Permission: Moore, C. E. & Merrill, P. W. 1968, Partial Grotrian Diagrams of Astrophysical Interest, 1968 (Washington, D.C.: GPO), 1968 / ???.
Image linked to Moore & Merrill (1968, p. 16).
Caption: Mg II Grotrian diagram.
Credit/Permission: Moore, C. E. & Merrill, P. W. 1968, Partial Grotrian Diagrams of Astrophysical Interest, 1968 (Washington, D.C.: GPO), 1968 / ???.
Image linked to Moore & Merrill (1968, p. 10).
Caption: Si II Grotrian diagram.
Credit/Permission: Moore, C. E. & Merrill, P. W. 1968, Partial Grotrian Diagrams of Astrophysical Interest, 1968 (Washington, D.C.: GPO), 1968 / ???.
Image linked to Moore & Merrill (1968, p. 22).
Caption: S II Grotrian diagram.
Credit/Permission: Moore, C. E. & Merrill, P. W. 1968, Partial Grotrian Diagrams of Astrophysical Interest, 1968 (Washington, D.C.: GPO), 1968 / ???.
Image linked to Moore & Merrill (1968, p. 30).
Caption: Ca I Grotrian diagram.
For correct orientation: /on image right click/menu/rotate clockwise.
Credit/Permission: Moore, C. E. & Merrill, P. W. 1968, Partial Grotrian Diagrams of Astrophysical Interest, 1968 (Washington, D.C.: GPO), 1968 / ???.
Image linked to Moore & Merrill (1968, p. 18).
Caption: Ca II Grotrian diagram.
Under almost all conditions, the strongest transition lines of Ca II by far are the 2 near ultraviolet ground state Ca II H & K lines which constitute a doublet of lines with wavelengths λ=3933.66 Å (the K line) and λ=3968.47 Å (the H line) (Wiese et al. 1969, p. 252).
Credit/Permission: Moore, C. E. & Merrill, P. W. 1968, Partial Grotrian Diagrams of Astrophysical Interest, 1968 (Washington, D.C.: GPO), 1968 / ???.
Image linked to Moore & Merrill (1968, p. 12).
Caption: Sc II Grotrian diagram.
For correct orientation: /on image right click/menu/rotate clockwise.
Credit/Permission: Moore, C. E. & Merrill, P. W. 1968, Partial Grotrian Diagrams of Astrophysical Interest, 1968 (Washington, D.C.: GPO), 1968 / ???.
Image linked to Moore & Merrill (1968, p. 40).
Caption: Ti II Grotrian diagram.
For correct orientation: /on image right click/menu/rotate clockwise.
Credit/Permission: Moore, C. E. & Merrill, P. W. 1968, Partial Grotrian Diagrams of Astrophysical Interest, 1968 (Washington, D.C.: GPO), 1968 / ???.
Image linked to Moore & Merrill (1968, p. 44).
Caption: V II Grotrian diagram.
For correct orientation: /on image right click/menu/rotate clockwise.
Credit/Permission: Moore, C. E. & Merrill, P. W. 1968, Partial Grotrian Diagrams of Astrophysical Interest, 1968 (Washington, D.C.: GPO), 1968 / ???.
Image linked to Moore & Merrill (1968, p. 48).
Caption: Cr II Grotrian diagram.
Credit/Permission: Moore, C. E. & Merrill, P. W. 1968, Partial Grotrian Diagrams of Astrophysical Interest, 1968 (Washington, D.C.: GPO), 1968 / ???.
Image linked to Moore & Merrill (1968, p. 52).
Caption: Mn II Grotrian diagram.
For correct orientation: /on image right click/menu/rotate clockwise.
Credit/Permission: Moore, C. E. & Merrill, P. W. 1968, Partial Grotrian Diagrams of Astrophysical Interest, 1968 (Washington, D.C.: GPO), 1968 / ???.
Image linked to Moore & Merrill (1968, p. 56).
Caption: Fe I Grotrian diagram.
For correct orientation: /on image right click/menu/rotate clockwise.
Credit/Permission: Moore, C. E. & Merrill, P. W. 1968, Partial Grotrian Diagrams of Astrophysical Interest, 1968 (Washington, D.C.: GPO), 1968 / ???.
Image linked to Moore & Merrill (1968, p. 62).
Caption: Fe II Grotrian diagram.
For correct orientation: /on image right click/menu/rotate clockwise.
Credit/Permission: Moore, C. E. & Merrill, P. W. 1968, Partial Grotrian Diagrams of Astrophysical Interest, 1968 (Washington, D.C.: GPO), 1968 / ???.
Image linked to Moore & Merrill (1968, p. 61).
Caption: Fe III Grotrian diagram.
For correct orientation: /on image right click/menu/rotate clockwise.
Credit/Permission: Moore, C. E. & Merrill, P. W. 1968, Partial Grotrian Diagrams of Astrophysical Interest, 1968 (Washington, D.C.: GPO), 1968 / ???.
Image linked to Moore & Merrill (1968, p. 60).
Caption: Co I Grotrian diagram.
For correct orientation: /on image right click/menu/rotate clockwise.
Credit/Permission: Moore, C. E. & Merrill, P. W. 1968, Partial Grotrian Diagrams of Astrophysical Interest, 1968 (Washington, D.C.: GPO), 1968 / ???.
Image linked to Moore & Merrill (1968, p. 63).
Caption: Ni I Grotrian diagram.
For correct orientation: /on image right click/menu/rotate clockwise.
Credit/Permission: Moore, C. E. & Merrill, P. W. 1968, Partial Grotrian Diagrams of Astrophysical Interest, 1968 (Washington, D.C.: GPO), 1968 / ???.
Image linked to Moore & Merrill (1968, p. 65).
Caption: Ni II Grotrian diagram.
For correct orientation: /on image right click/menu/rotate clockwise.
Credit/Permission: Moore, C. E. & Merrill, P. W. 1968, Partial Grotrian Diagrams of Astrophysical Interest, 1968 (Washington, D.C.: GPO), 1968 / ???.
Image linked to Moore & Merrill (1968, p. 64).