Abstract
The effect of a diluted Planckian radiation field on a Xe gas at the electron temperature of 100 eV is investigated within the framework of a Collisional Radiative Model, using the HULLAC code. The atomic model spans 19 charge states, includes 20,375 configurations and contains more than 2 × 106 levels. We have simulated detailed spectra comprising more than 109 transitions with the Mixed UTA model. The radiation temperature Tr is varied from 0 to 1.5 Te. The dilution factor, D, applied to decrease the radiation field, is varied independently from 0 to 3 at fixed Tr = Te. In both cases, the average charge state Z* increases from 15 to 27, but in different ways. It is shown that even a dilution D = 0.01 changes Z* by more than 1.5. Different combinations of Tr and D yielding exactly the same Z*, may give line ratios sufficiently different to be observed. This fact is explained by the interplay of the shape of the radiation field and the atomic structure.
| Original language | English |
|---|---|
| Pages (from-to) | 98-104 |
| Number of pages | 7 |
| Journal | High Energy Density Physics |
| Volume | 7 |
| Issue number | 2 |
| DOIs | |
| State | Published - Jun 2011 |
| Externally published | Yes |
Keywords
- Laboratory astrophysics
- Non-LTE
- Radiation driven plasmas
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