Publication: Dielectronic recombination data for dynamic finite-density plasmas - XIII. The magnesium isoelectronic sequence
| dc.contributor.author | YUMAK YAHŞİ, AYŞE | |
| dc.contributor.author | YAVUZ, İLHAN | |
| dc.contributor.author | ALTUN, ZİKRİ | |
| dc.contributor.authors | Altun, Z.; Yumak, A.; Yavuz, I.; Badnell, N. R.; Loch, S. D.; Pindzola, M. S. | |
| dc.date.accessioned | 2022-03-14T09:03:10Z | |
| dc.date.accessioned | 2026-01-10T17:37:42Z | |
| dc.date.available | 2022-03-14T09:03:10Z | |
| dc.date.issued | 2007-11 | |
| dc.description.abstract | We have calculated total and partial final- state level- resolved dielectronic recombination ( DR) rate coe. cients for the ground and metastable initial levels of 21 Mg- like ions between Al+ and Xe42+. This is the final part of the assembly of a levelresolved DR database necessary for modelling dynamic finite-density plasmas within the generalized collisional-radiative framework. Calculations have been performed in both LS-and intermediate coupling, allowing for. n = 0 and. n = 1 core- excitations from ground and metastable levels. Complementary partial and total radiative recombination RR coeficients have been calculated for the same ions viz. Al+ through Zn18+, as well as Kr24+, Mo30+, and Xe42+. Fitting coeficients which describe the total RR and DR rate coeficients (separately) are also presented here. Results for a selection of ions fromthis sequence are discussed, and compared with existing theoretical and experimental results. A full set of results can be accessed from the Atomic Data and Analysis Structure (ADAS) database or from the Oak Ridge Controlled Fusion Atomic Data Center (http://www-cfadc.phy.ornl.gov/data_and_codes). The complexity of further M-shell sequences, both from the atomic and modelling perspectives, renders this juncture a natural conclusion for the assemblage of the partial database. Further M-shell work, has and will, focus more on total rate coe. cients, rather than partials, at least in the medium term. | |
| dc.identifier.doi | 10.1051/0004-6361:20078238 | |
| dc.identifier.issn | 1432-0746 | |
| dc.identifier.uri | https://hdl.handle.net/11424/242226 | |
| dc.identifier.wos | WOS:000250443900043 | |
| dc.language.iso | eng | |
| dc.publisher | EDP SCIENCES S A | |
| dc.relation.ispartof | ASTRONOMY & ASTROPHYSICS | |
| dc.rights | info:eu-repo/semantics/openAccess | |
| dc.subject | atomic data | |
| dc.subject | atomic processes | |
| dc.subject | plasmas | |
| dc.subject | ELECTRON-ION RECOMBINATION | |
| dc.subject | ACTIVE GALACTIC NUCLEI | |
| dc.subject | OPTICALLY THIN PLASMAS | |
| dc.subject | X-RAY-ABSORPTION | |
| dc.subject | IONIZATION EQUILIBRIUM | |
| dc.subject | RATE COEFFICIENTS | |
| dc.subject | LOW-TEMPERATURES | |
| dc.subject | EMISSION RATES | |
| dc.subject | M-SHELL | |
| dc.subject | FE-XIV | |
| dc.title | Dielectronic recombination data for dynamic finite-density plasmas - XIII. The magnesium isoelectronic sequence | |
| dc.type | article | |
| dspace.entity.type | Publication | |
| oaire.citation.endPage | 1059 | |
| oaire.citation.issue | 3 | |
| oaire.citation.startPage | 1051 | |
| oaire.citation.title | ASTRONOMY & ASTROPHYSICS | |
| oaire.citation.volume | 474 |
Files
Original bundle
1 - 1 of 1
