molike_hps95mo.dat
Resolved Specific Ion Data Collections
- Ion
- Mo0+
- Temperature Range
- 1.000 eV → 200 eV
ADF04
- Filename
- molike_hps95mo.dat
- Full Path
- adf04/molike/molike_hps95mo.dat
Download data
- Spontaneous Emission: Mo+0(i) → Mo+0(j) + hv
- Electron Impact Excitation: Mo+0(i) + e → Mo+0(j) + e
- Free Electron Recombination: Mo+1(i) + e → Mo+0(j)
| (a6s)5s(a7s) 7S3.0 | 0.0 cm-1 |
| (a6s)5s(a5s) 5S2.0 | 10768.3 cm-1 |
| (a6s)5p(z7p) 7P10.0 | 26003.0 cm-1 |
| (a6s)5p(z5p) 5P7.0 | 28853.0 cm-1 |
| (5d)5s5p(y7p) 7P10.0 | 31641.0 cm-1 |
| (5d)5s5p(y5p) 5P7.0 | 33525.0 cm-1 |
Contributors
- Hugh Summers
- Nigel Badnell
---------------------------------------------------------------------------- Energy Levels: Taken from Moore NBS tables Ionisation Potential: As energy levels A Values: Taken from strcture calculations Collision Rates: R-matrix calculations by Badnell & Gorczyca based on Superstructure and Froese-Fischer targets. Amends earlier JET unpublished work by Queen's University Belfast. Data for a7S-a5S spin change and z7P-y7P, z5P-y5P transitions included from same calculations but lower accuracy expected. ionisation cross-section calculations by Pindzola in distorted wave approximation (including exchange) H. P. Summers 8 July 1994 Added collisional transition 1-4 with same upsilons as 1-2 on recommendation of Badnell. Variation between septet and quintet structure gives uncertainties of order 2 in R-matrix calculation, justifying this. H. P. Summers 16 June 1995 Substituted 1-2, 1-4 and 1-6 upsilons from new calculations of Badnell. Calculations used the new prseudo-resonance eliminating version of the R-matrix codes. Original data from the spread shhet analysis is in 'jetshp.strath.data(exc#cr0)'. H. P. Summers 14 Aug 1995 ---------------------------------------------------------------------------- RADIATIVE RECOMBINATION DATA ADDED PROCESSED BY ADASRRC ON :/JETSHP.RADREC.NBLIKE(MO1LS) H. P. Summers 20 June 1995 ------------------------------------------------------------------------------- --------------------------------------------------------------------------------- ---------------------------------------------------------------------------------