| Comparison of observed and theoretical Fe L emission from CIE plasmas | |
| Carpenter, M ; Beiersdorfer, P ; Brown, G V ; Chen, H C ; Gu, M F ; Jernigan, J G | |
| Lawrence Livermore National Laboratory | |
| 关键词: Lawrence Livermore National Laboratory; Spectra; Photons; 99 General And Miscellaneous//Mathematics, Computing, And Information Science; Electron Beams; | |
| DOI : 10.2172/924171 RP-ID : UCRL-SR-236551 RP-ID : W-7405-ENG-48 RP-ID : 924171 |
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| 美国|英语 | |
| 来源: UNT Digital Library | |
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【 摘 要 】
We analyze data from the Lawrence Livermore National Lab (LLNL) Electron Beam Ion Trap (EBIT) that simulates a CIE plasma by sweeping the electron beam to approximate a Maxwellian velocity distribution. These results are compared to spectra of confirmed astronomical CIE plasmas (e.g. outer regions of x-ray clusters) observed by XMM/RGS. We utilize the Photon Clean Method (PCM) to quantify these spectra (EBIT and XMM/RGS) in the form of ratios of Fe L lines in the emission complex near 1 keV. The variances of line fluxes are measured with bootstrap methods (Efron 1979). Both of these observations are further compared with theoretical predictions of Fe L line fluxes from APED and similar atomic databases.
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| 924171.pdf | 961KB |
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