Issue |
A&A
Volume 601, May 2017
|
|
---|---|---|
Article Number | A111 | |
Number of page(s) | 7 | |
Section | Atomic, molecular, and nuclear data | |
DOI | https://doi.org/10.1051/0004-6361/201630199 | |
Published online | 15 May 2017 |
Measurements of density dependent intensity ratios of extreme ultraviolet line emission from Fe X, XI, and XII
1 Institute for Laser Science, The University of Electro-Communications, Tokyo 182-8585, Japan
e-mail: safdaruetian@gmail.com
2 National Institute for Fusion Science, Gifu 509-5292, Japan
3 Department of Fusion Science, SOKENDAI, Gifu 509-5292, Japan
4 National Astronomical Observatory of Japan, Tokyo 181-8588, Japan
5 Department of Astronomical Science, SOKENDAI, Tokyo 181-8588, Japan
Received: 6 December 2016
Accepted: 25 March 2017
We report high-resolution density dependent intensity ratio measurements for middle charge states of iron in the extreme ultraviolet (EUV) spectral wavelength range of 160−200 Å. The measurements were performed at the Tokyo EBIT laboratory by employing a flat-field grazing incidence spectrometer installed on a low energy compact electron beam ion trap. The intensity ratios for several line pairs stemming from Fe X, Fe XI and Fe XII were extracted from spectra collected at the electron beam energies of 340 and 400 eV by varying the beam current between 7.5 and 12 mA at each energy. In addition, the effective electron densities were obtained experimentally by imaging the electron beam profile and ion cloud size with a pinhole camera and visible spectrometer, respectively. In this paper, the experimental results are compared with previous data from the literature and with the present calculations performed using a collisional-radiative model. Our experimental results show a rather good agreement with the calculations and previous reported results.
Key words: ultraviolet: planetary systems / Sun: corona / methods: laboratory: atomic / techniques: spectroscopic / atomic processes / atomic data
© ESO, 2017
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