Identifications of Fe XVII and Ni XIX in solar flares based on isoelectronic extrapolations-Reference-Cited by-同舟云学术

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Identifications of Fe XVII and Ni XIX in solar flares based on isoelectronic extrapolations

Published:1984-05-01 Issue:1 Volume:208 Page:1P-5P
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:Monthly Notices of the Royal Astronomical Society

Author:

Jupen C.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/208/1/1P/2812260/mnras208-001P.pdf

Cited by 56 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Solar UV and X-ray spectral diagnostics;Living Reviews in Solar Physics;2018-08-31

2. Implementation and application of the relativistic equation-of-motion coupled-cluster method for the excited states of closed-shell atomic systems;Physical Review A;2014-06-19

3. Benchmarking atomic data for astrophysics: Fe XVII EUV lines;Astronomy & Astrophysics;2009-10-27

4. Electron-impact excitation of 2p53l→ 2p53l' line emission of Fe XVII;Journal of Physics: Conference Series;2009-04-01

5. Solar Observations of High‐Temperature Emission with the Extreme‐Ultraviolet Imaging Spectrometer onHinode;The Astrophysical Journal;2008-10

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