Spectra of Ni- and Co-like ions of Xe in an electron-beam ion trap

2008 ◽  
Vol 86 (3) ◽  
pp. 467-475 ◽  
Author(s):  
E Träbert ◽  
P Beiersdorfer ◽  
M F Gu

High-resolution soft X-ray observations of Ni- and Co-like Xe ions in an electron-beam ion trap are compared with the predictions of various calculations. Calculated energy levels up to the 4p levels are presented alongside experimental determinations. PACS Nos.: 32.30.Rj; 34.50.Fa; 34.80.Dp

1999 ◽  
Vol 70 (1) ◽  
pp. 280-283 ◽  
Author(s):  
G. V. Brown ◽  
P. Beiersdorfer ◽  
K. Widmann

1999 ◽  
Vol 70 (3) ◽  
pp. 1658-1664 ◽  
Author(s):  
N. Nakamura ◽  
A. Ya. Faenov ◽  
T. A. Pikuz ◽  
E. Nojikawa ◽  
H. Shiraishi ◽  
...  

1997 ◽  
Vol 68 (1) ◽  
pp. 1077-1079 ◽  
Author(s):  
P. Beiersdorfer ◽  
J. R. Crespo López-Urrutia ◽  
E. Förster ◽  
J. Mahiri ◽  
K. Widmann

1990 ◽  
Vol 61 (9) ◽  
pp. 2338-2342 ◽  
Author(s):  
P. Beiersdorfer ◽  
R. E. Marrs ◽  
J. R. Henderson ◽  
D. A. Knapp ◽  
M. A. Levine ◽  
...  

2004 ◽  
Vol 75 (10) ◽  
pp. 3723-3726 ◽  
Author(s):  
P. Beiersdorfer ◽  
E. W. Magee ◽  
E. Träbert ◽  
H. Chen ◽  
J. K. Lepson ◽  
...  

2001 ◽  
Vol 79 (2-3) ◽  
pp. 153-162 ◽  
Author(s):  
E Träbert ◽  
P Beiersdorfer ◽  
K B Fournier ◽  
S B Utter ◽  
K L Wong

Systematic variation of the electron-beam energy in an electron-beam ion trap has been employed to produce soft-X-ray spectra (20 to 60 Å) of Au with well-defined maximum charge states ranging from Br- to Co-like ions. Guided by large-scale relativistic atomic structure calculations, the strongest Δn = 0 (n = 4 to n' = 4) transitions in Rb- to Cu-like ions (Au42+ – Au50+) have been identified. PACS Nos.: 32.30Rj, 39.30+w, 31.50+w, 32.20R


2019 ◽  
Vol 49 (1) ◽  
pp. 21-24 ◽  
Author(s):  
Peter Beiersdorfer ◽  
Natalie Hell ◽  
Dmytro Panchenko ◽  
Greg V. Brown ◽  
Elmar Träbert ◽  
...  

2008 ◽  
Vol 86 (1) ◽  
pp. 199-208 ◽  
Author(s):  
G V Brown

X-ray emission from neon-like Fe XVII has been measured with high-resolution spectrometers from laboratory or celestial sources for nearly seven decades. Two of the strongest lines regularly identified in these spectra are the 1P1 → 1S0 resonance and the 3D1 → 1S0 intercombination line, known as 3C and 3D, respectively. This paper gives a brief overview of measurements of the intensities of the lines 3C and 3D from laboratory and celestial sources and their comparison to model calculations, with an emphasis on measurements completed using an electron beam ion trap. It includes a discussion of the measured absolute cross sections compared with results from modern atomic theory calculations as well as the diagnostic utility of the relative intensity, R = I3C/I3CD, as it applies to the interpretation of spectra measured from the Sun and extra-solar sources. PACS Nos.: 32.30.Rj, 32.30.–r, 32.70.Cs, 52.72.+v, 95.85.Nv, 96.60.P–, 97.10.Ex


2003 ◽  
Vol 74 (3) ◽  
pp. 1947-1950 ◽  
Author(s):  
A. S. Shlyaptseva ◽  
D. A. Fedin ◽  
S. M. Hamasha ◽  
S. B. Hansen ◽  
C. Harris ◽  
...  

1997 ◽  
Vol T73 ◽  
pp. 400-402 ◽  
Author(s):  
D Paterson ◽  
C T Chantler ◽  
C Q Tran ◽  
L T Hudson ◽  
F G Serpa ◽  
...  

Sign in / Sign up

Export Citation Format

Share Document