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Measurements of the effective electron density in an electron beam ion trap using extreme ultraviolet spectra and optical imaging

DOI:10.1063/1.5036758 期刊:Review of Scientific Instruments 出版年份:2018 更新时间:2025-09-09 09:28:46
摘要: In an electron beam ion trap (EBIT), the ions are not con?ned to the electron beam, but rather oscillate in and out of the beam. As a result, the ions do not continuously experience the full density of the electron beam. To determine the effective electron density, ne,eff, experienced by the ions, the electron beam size, the nominal electron density ne, and the ion distribution around the beam, i.e., the so-called ion cloud, must be measured. We use imaging techniques in the extreme ultraviolet (EUV) and optical to determine these. The electron beam width is measured using 3d → 3p emission from Fe xii and xiii between 185 and 205 ?. These transitions are fast and the EUV emission occurs only within the electron beam. The measured spatial emission pro?le and variable electron current yield a nominal electron density range of ne ~ 1011–1013 cm?3. We determine the size of the ion cloud using optical emission from metastable levels of ions with radiative lifetimes longer than the ion orbital periods. The resulting emission maps out the spatial distribution of the ion cloud. We ?nd a typical electron beam radius of ~60 μm and an ion cloud radius of ~300 μm. These yield a spatially averaged effective electron density, ne,eff, experienced by the ions in EBIT spanning ~ 5 × 109–5 × 1011 cm?3.
作者: T. P. Arthanayaka,P. Beiersdorfer,G. V. Brown,M. Hahn,N. Hell,T. E. Lockard,D. W. Savin
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To determine the effective electron density, ne,eff, experienced by the ions in an electron beam ion trap (EBIT) by measuring the electron beam size, the nominal electron density ne, and the ion distribution around the beam.

The study successfully measured the electron beam and ion cloud profiles in EBIT-I and derived ne,eff. The results provide an important exploration of potential systematic issues related to electron beam and ion cloud measurements in an EBIT. The spatially averaged effective electron densities of ne,eff ~ 5 × 109 to 5 × 1011 cm?3, which are typical of the solar corona, can be generated in EBIT-I.

The asymmetry and broad base of the ion cloud image may be due to aberrations in the lens as well as a slight misalignment of the lens plane relative to the object plane. Additional contributions to the asymmetry and broad base of the image may be due to reflection from the drift tube and emission from metastable levels in Fe iii, vi, and vii.

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