Showing papers by "T. W. Phillips published in 1995"
TL;DR: Good agreement between the predicted and measured intensities of the strong dielectronic satellites is found, demonstrating the utility of {ital K}{beta} spectra as a diagnostic of the electron temperature of low-density plasmas, such as those found in the Sun or magnetic fusion facilities.
Abstract: High-resolution crystal spectrometer measurements of the {ital K}{beta} spectrum of heliumlike Ar{sup 16+} covering the wavelength region from 3.34 to 3.50 A are presented and compared with detailed theoretical analyses. The measurements were made on the Princeton Large Torus tokamak and test the theoretical atomic data in the low-density limit at an electron density {ital n}{sub {ital e}}{le}2{times}10{sup 13} cm{sup {minus}3} and temperature {ital T}{sub {ital e}}=2.3 keV. Satellite transitions of the type 1{ital s}{sup 2}2{ital l}-1{ital s}2{ital l}3{ital l}{prime} and 1{ital s}{sup 2}3{ital l}-1{ital s}3{ital l}3{ital l}{prime} from lithiumlike Ar{sup 15+} and 1{ital s}{sup 2}2{ital l}2{ital l}{prime}-1{ital s}2{ital l}2{ital l}{prime}3{ital l}{prime}{prime} from berylliumlike Ar{sup 14+} are identified that are produced by either dielectronic recombination or electron-impact excitation. Good agreement between the predicted and measured intensities of the strong dielectronic satellites is found. The agreement demonstrates the utility of {ital K}{beta} spectra as a diagnostic of the electron temperature of low-density plasmas, such as those found in the Sun or magnetic fusion facilities. Poorer agreement is found for the weaker dielectronic satellite transitions, including the 1{ital s}3{ital l}3{ital l}{prime} satellites that play an important role in the analysis of high-density plasma produced in laser fusion. Their intensity is underestimated bymore » the calculations by about 50%. And it is shown that direct electron-impact excitation rates underestimate the relative intensity of the 1{ital s}{sup 2} {sup 1}{ital S}{sub 0}--1{ital s}2{ital p} {sup 3}{ital P}{sub 1} transition in heliumlike Ar{sup 16+} by a factor of 2, indicating the need for including additional excitation processes and possible blends with high-lying dielectronic satellites of the type 1{ital s}{sup 2}{ital nl}{prime}-1{ital s}3{ital lnl}{prime} with {ital n}{ge}4 in the theoretical models.« less
34 citations