Table A.1
Summary of the model atoms used and sources for the atomic data.
Element | Levels | Highest state | Energies and A-values | Tot. rr. | Spec. rr. | Coll. strengths |
|
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H I | 210/465 | n = 20/n = 30 | 23 | 18 | 4 (all) | 1, 5 (all) |
He I | 29/29 | 5p(1P) | 23 | 6 | 3 (all) | 25 (all) |
C I | 90/90 | 5d(1D) | 23 | 11 | 11 (first 17) | 16 (first 6) |
C II | 7/77 | 8g(2G) | 23 | 10 | – | 16 (first 5) |
N I | 68/68 | 5s(2P) | 23 | 19 | – | 16 (first 5) |
|
||||||
N II | 10/148 | 2p3(5S)/3p(3D) | 23 | 19 | – | 16 (all) |
O I | 135/135 | 8d(3D*) | 23 | 10 | 10 (first 49) | 16 (first 7) |
O II | 16/16 | 2p4(2S) | 23 | 10 | – | 16 (first 5) |
Ne I | 3/3 | 3s(2[3/2]) | 23 | 19 | – | – |
Ne II | 3/3 | 2p6(2S) | 23 | 19 | – | 16 (first 1) |
|
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Na I | 66/66 | 9f(2F) | 23 | 14 | 24 (first 60) | 20 (first 2) |
Mg I | 200/371 | 37d(3D)/80d(3D) | 7 | 14, 19 | 24 (first 18) | 8 (first 21) |
Mg II | 35/35 | 7p(2P) | 23 | 21 | – | 16 (first 2) |
Al I | 50/86 | 10d(2D)/21s(2S) | 7 | 14 | – | –c |
Al II | 10/154 | 3p2(3P)/3pd(3D) | 7 | –b | – | –c |
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Si I | 200/494 | 10s(3P)/21s(1P) | 7 | 11 | 11 (first 49) | –c |
Si II | 77/77 | 9p(2P) | 23 | 10 | – | 16 (all) |
S I | 125/125 | 8f(3F) | 7 | 14, 19 | – | –c |
S II | 5/5 | 3p3(2P) | 23 | 10 | – | 16 (all with gs) |
Ar I | 3/3 | 3p5(4S) | 23 | 19 | – | –c |
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Ar II | 2/2 | 3p5(2P) | 23 | 19 | – | 16 |
Ca I | 198/198 | 6d(3D) | 7 | 14 | 24 (first 11) | –c |
Ca II | 69/69 | 16d(2D) | 23 | 14 | – | 9 (all) |
Sc I | 50/254 | 4p(4F)/7p(2P) | 7 | –a | – | –c |
Sc II | 10/165 | 3d2(3P)/6f(1H) | 7 | –b | – | –c |
|
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Ti I | 50/394 | 4s(c3P)/4p2(1P) | 7 | 14 | – | –c |
Ti II | 10/212 | 4s(a2F)/5d(4H) | 7 | –b | – | –c |
V I | 50/502 | sp(z6D)/4p2(r2H) | 7 | –a | – | –c |
V II | 10/323 | 4s(a5F)/4f(2(11/2)) | 7 | –b | – | –c |
Cr I | 50/392 | sp(z7D)/21p(e5F) | 7 | –a | – | –c |
|
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Cr II | 10/500 | 4s(a4D)/4f(4H) | 7 | –b | – | –c |
Mn I | 50/293 | 4s(b4G)/4p(z2I) | 7 | 14 | – | –c |
Mn II | 10/509 | 4s(a5G)/9h(7H) | 7 | –b | – | –c |
Fe I | 496/496 | 4p(1P0)(3F) | 7 | 10 | 10 (first 356) | 2, 15 (first 120) |
Fe II | 578/578 | (7S)4d(8D) | 12, 23 | 10 | 10 (first 381) | 22 (first 372) |
|
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Fe III | 168/168 | 4p(3I) | 7 | –b | – | –c |
Co I | 50/317 | d9(c2D)/5s(370) | 7 | –a | – | –c |
Co II | 10/108 | 4s(b3F)/7d(5H) | 7, 17 | –b | – | –c |
Ni I | 50/136 | 4p(F*)/4d(2[1/2]) | 23 | 19 | – | –c |
Ni II | 10/500 | 4s(2D)/sp(4D) | 7 | 19 | – | –c |
Notes. Column 1: element, Col. 2: number of fine-structure levels solved for and the number included in the radiative transfer, Col. 3: highest state included, Col. 4: source for level energies and transition A-values, Col. 5: source for the total radiative recombination rate, Col. 6: source for the specific radiative recombination rates, and the number of levels for which these rates are included in parenthesis, Col. 7: source for the (thermal) collision strengths, and the number of levels with collision strength included in parenthesis.
References. (1) Anderson et al. (2000); (2) Axelrod (1980); (3) Benjamin et al. (1999); (4) Brocklehurst (1971); (5) Johnson (1972); (6) Hummer & Storey (1998); (7) R. Kurucz (http://www.cfa.harvard.edu/amp/ampdata/kurucz23/sekur.html); (8) Mauas et al. (1988); (9) Meléndez et al. (2007); (10) S. Nahar (www.astronomy.ohio-state.edu/ nahar/nahar_radiativeatomicdata/index.html); (11) Nahar (1995); (12) Fuhr & Wiese (2006); (13) Nahar (1997); (14) Pequignot & Aldrovandi (1986); (15) Pelan & Berrington (1997); (16) A. Pradhan (www.astronomy.ohio-state.edu/ pradhan/table2.ps); (17) Quinet (1998); (18) Seaton (1959); (19) Shull & van Steenberg (1982); (20) Trail et al. (1994); (21) Verner et al. (1996); (22) Zhang & Pradhan (1995); (23) NIST (www.nist.gov); (24) TOPBASE (http://cdsweb.u-strasbg.fr/topbase/xsections.html); (25) Almog & Netzer (1989).
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