J/A+A/565/A77       Atomic data for FeIX                      (Del Zanna+, 2014)

Atomic data for astrophysics: Fe IX. Del Zanna G., Storey P.J., Badnell N.R., Mason H.E. <Astron. Astrophys. 565, A77 (2014)> =2014A&A...565A..77D 2014A&A...565A..77D
ADC_Keywords: Atomic physics Keywords: atomic data - line: identification - techniques: spectroscopic Abstract: We present the results of a new large-scale intermediate-coupling frame transformation R-matrix scattering calculation for electron collisional excitation of Fe IX. The target includes all the main configurations up to n=5, to improve our earlier R-matrix and distorted-wave (DW) calculations for the n=3,4 levels. Unlike similar calculations which we carried out for the other coronal iron ions, in this case the larger target does not significantly affect the collision strengths of the strongest transitions to the n=3,4 levels. Some differences are however present for a few transitions, in particular for the 3d-4p line at 197.86Å. For the weaker transitions, significant enhancements due to extra resonances resulting from this much bigger target are found. Several new line identifications are suggested. We find excellent agreement between predicted and observed line intensities in the EUV (Hinode EIS) showing that Fe IX lines provide a reliable temperature diagnostic. We also show that the visible forbidden lines are a good diagnostic to measure electron densities. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 51 865 Level energies of the RM4 calculation table2.dat 117 373680 Transition probabilities and thermally averaged collision strengths for the RM4 calculation -------------------------------------------------------------------------------- See also: J/A+A/541/A90 : Fe X soft X-ray lines (Del Zanna+, 2012) J/A+A/543/A139 : Fe XII soft X-ray lines (Del Zanna+, 2012) J/A+A/543/A144 : Fe XIII soft X-ray lines (Del Zanna+, 2012) J/A+A/549/A42 : Fe XI soft X-ray lines (Del Zanna+, 2013) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 3- 5 I3 --- Index [1/865] Level index 7- 24 A18 --- Level Electronic level description 25 A1 --- --- [(] 26 I1 --- 2S+1 [1/7] 2S+1 multiplicity 27 A1 --- --- [)] 28 I1 --- L [0-7] L value 29 A1 --- --- [(] 30- 33 F4.1 --- J [0/8] J value 34 A1 --- --- [)] 43- 51 F9.1 cm-1 E Target energy (ab initio) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 2- 4 I3 --- i [2/865] Upper level index of the transition 6- 8 I3 --- j [1/864] Lower level index of the transition 10- 17 E8.3 s-1 A Einstein A coefficient 19- 26 E8.3 --- CS1 Averaged collision strength at T=1.62x104K 28- 35 E8.3 --- CS2 Averaged collision strength at T=4.05x104K 37- 44 E8.3 --- CS3 Averaged collision strength at T=8.1x104K 46- 53 E8.3 --- CS4 Averaged collision strength at T=1.62x105K 55- 62 E8.3 --- CS5 Averaged collision strength at T=4.05x105K 64- 71 E8.3 --- CS6 Averaged collision strength at T=8.1x105K 73- 80 E8.3 --- CS7 Averaged collision strength at T=1.62x106K 82- 89 E8.3 --- CS8 Averaged collision strength at T=4.05x106K 91- 98 E8.3 --- CS9 Averaged collision strength at T=8.1x106K 100-107 E8.3 --- CS10 Averaged collision strength at T=1.62x107K 109-117 E9.3 --- Elim High-energy limit -------------------------------------------------------------------------------- Acknowledgements: Giulio Del Zanna, gdelzanna(at)spd.aas.org
(End) Patricia Vannier [CDS] 25-Apr-2014
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line