The effect of metastable level populations on the ionization fraction of Li-like ions

Lines from Li-like ions have been known to produce theoretical intensities under-estimated compared to lines of a similar formation temperature. Here we investigate this anomalous behaviour whereby the ionization fractions are calculated using the ADAS code considering the electron density dependenc...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:Astronomy and astrophysics (Berlin) 2005-02, Vol.430 (2), p.L29-L32
Hauptverfasser: Doyle, J. G., Summers, H. P., Bryans, P.
Format: Artikel
Sprache:eng
Schlagworte:
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
Beschreibung
Zusammenfassung:Lines from Li-like ions have been known to produce theoretical intensities under-estimated compared to lines of a similar formation temperature. Here we investigate this anomalous behaviour whereby the ionization fractions are calculated using the ADAS code considering the electron density dependence of dielectronic recombination coupled with collisional ionization from metastable levels. For the lines investigated, the line contribution functions show a clear dependence with increasing electron density. For example, C iv 1548 Å  shows over a factor of three enhancement for $N_{\rm e} = 10^{12}~{\rm cm}^{-3}$. The increase in the higher temperature lines is lower, but are still in the range of 30 to 60%. Furthermore, all the lines have their peak contribution shifted to lower temperature. Calculating the total radiative power output at an electron density of $10^{11}~{\rm cm}^{-3}$, we find that the difference in the transition region is 10–15% while above 106 K the difference is around 30% compared to the low density value.
ISSN:0004-6361
1432-0746
DOI:10.1051/0004-6361:200400125