Computedn=2 level populations in helium-like ions from Cv to Nixxvii |
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| Authors: | R Mewe J Schrijver |
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| Institution: | 1. Space Research Laboratory, Astronomical Institute, Utrecht, The Netherlands
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| Abstract: | The population densities of all levels with principal quantum numbern=2 in a number of helium-like ions with nuclear charge numberZ, in the range 6 to 28 have been evaluated as a function of various parameters, i.e., electron temperature,T e, electron density,N e, radiation temperature,T r, dilution factor,W, and of the state of ionization. The spectral line fluxes from all possible radiative transitions from these levels have been calculated for an optically thin plasma. The effects of cascades following collisional excitation of higher levels or radiative and dielectronic recombination have been computed in detail. Innershell ionization of the lithium-like ion to form the helium-like ion in a 23 S or 21 S state has been considered. It can have a strong influence on the forbidden line intensity in a non-equilibrium plasma. Collisional and radiative coupling of levels of the same multiplicity (e.g. 23 S 1 and 23 P 2,1,0) have been considered as a function ofT e, Ne orT r, W, respectively. The computations were performed both for stationary and time-varying plasmas. In the latter case strong departures from a stationary ionization equilibrium can significantly alter the line fluxes. A few examples of the results are shown and discussed. |
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