Forbidden lines arising from magnetic dipole(M l)transitions among fine-structure levels of highly charged ions have been observed for Al,Ar, Ti, Fe,Kr, Mo and Xe in Large Helical Device(LHD). A space-resolved 3m normal incidence VUV spectrometer and newly designed double-structure impurity pellets for an impurity pellets injector have been developed for this purpose. The Ml transitions are identified by analyzing their Doppler broademing, temporal intensity behavior and spatial intensity distribution. Wavelengths of these M l transitions are determined with high accuracy and compared with previous experimental and calculated values with detailed spectroscopic analysis of C,Ne and Ar emission lines in range of 250 to 2300Å. The Ml tr...
Two-dimensional (2-D) distribution of edge impurity line emissions has been measured for CIV, CVI, F...
International audienceThis paper is devoted to the analysis of transition arrays of magnetic-dipole ...
In dilute astrophysical plasmas, such as planetary nebulae and H ii regions, strong lines appear tha...
We measured extreme ultraviolet spectra of plasmas in the Large Helical Device after an Fe pellet wa...
A space-resolved spectroscopy using a 3m normal incidence vacuum ultraviolet (VUV) spectrometer was ...
Space-resolved vacuum ultraviolet (VUV) spectroscopy using a 3 m normal incidence spectrometer has b...
Vacuum ultraviolet (VUV) spectra of emissions released from tungsten ions at lower ionization stages...
A variety of density profiles observed in the Large Helical Device (LHD) have suggested an interesti...
Aims. Accurate and reliable atomic data for lowly ionized Fe-peak species (Sc, Ti, V, Cr, Mn, Fe, Co...
Numerous optically forbidden lines resulting from magnetic dipole transitions in low-lying electron ...
We have systematically observed extreme ultraviolet (EUV) spectra from highly charged ions of nine l...
Tungsten spectra in visible, vacuum ultra-violet (VUV) and extreme ultra-violet (EUV) wavelength ran...
An impurity powder dropper was installed in the 21st campaign of the Large Helical Device experiment...
Visible emission lines of tungsten ions are useful for analysis of tungsten ion distributions at ITE...
Extreme ultraviolet (EUV) spectra emitted from aluminum in the 5-340 A wavelength range were observe...
Two-dimensional (2-D) distribution of edge impurity line emissions has been measured for CIV, CVI, F...
International audienceThis paper is devoted to the analysis of transition arrays of magnetic-dipole ...
In dilute astrophysical plasmas, such as planetary nebulae and H ii regions, strong lines appear tha...
We measured extreme ultraviolet spectra of plasmas in the Large Helical Device after an Fe pellet wa...
A space-resolved spectroscopy using a 3m normal incidence vacuum ultraviolet (VUV) spectrometer was ...
Space-resolved vacuum ultraviolet (VUV) spectroscopy using a 3 m normal incidence spectrometer has b...
Vacuum ultraviolet (VUV) spectra of emissions released from tungsten ions at lower ionization stages...
A variety of density profiles observed in the Large Helical Device (LHD) have suggested an interesti...
Aims. Accurate and reliable atomic data for lowly ionized Fe-peak species (Sc, Ti, V, Cr, Mn, Fe, Co...
Numerous optically forbidden lines resulting from magnetic dipole transitions in low-lying electron ...
We have systematically observed extreme ultraviolet (EUV) spectra from highly charged ions of nine l...
Tungsten spectra in visible, vacuum ultra-violet (VUV) and extreme ultra-violet (EUV) wavelength ran...
An impurity powder dropper was installed in the 21st campaign of the Large Helical Device experiment...
Visible emission lines of tungsten ions are useful for analysis of tungsten ion distributions at ITE...
Extreme ultraviolet (EUV) spectra emitted from aluminum in the 5-340 A wavelength range were observe...
Two-dimensional (2-D) distribution of edge impurity line emissions has been measured for CIV, CVI, F...
International audienceThis paper is devoted to the analysis of transition arrays of magnetic-dipole ...
In dilute astrophysical plasmas, such as planetary nebulae and H ii regions, strong lines appear tha...