Results 161 to 170 of about 859 (172)
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Atomic data needed for analysis of EUV and X-Ray spectra

2006
Given high resolution X-ray spectra, one can derive the temperature structure, elemental abundances, density, and in some cases heating or cooling rate of a hot astrophysical plasma. The accuracy of various atomic rate coefficients limits the accuracy of the inferred plasma parameters. The important rates are typically collisional ionization, radiative
openaire   +1 more source

Calibration of Empirical EUV Spectra for the Regular E-Region Modeling

Bulletin of the Russian Academy of Sciences: Physics, 2022
V. D. Nikolaeva   +3 more
openaire   +1 more source

Line analysis of EUV spectra of molybdenum laser-produced plasmas using a comparison method

Journal of Quantitative Spectroscopy and Radiative Transfer, 2021
A P Shevelko, S N Andreev
exaly  

Line analysis of EUV Spectra from Molybdenum and Tungsten Injected with Impurity Pellets in LHD

Plasma and Fusion Research, 2007
M B Chowdhuri   +2 more
exaly  

EUV spectra of highly-charged ions W54+–W63+relevant to ITER diagnostics

Journal of Physics B: Atomic, Molecular and Optical Physics, 2008
Yu Ralchenko, J N Tan, J D Gillaspy
exaly  

Temperature-Dependent EUV Spectra of Xenon Plasmas Observed in the Compact Helical System

Journal of Plasma and Fusion Research, 2005
Hiroaki Nishimura   +2 more
exaly  

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