Astronomy and Astrophysics – Astrophysics
Scientific paper
Feb 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26as...92..517k&link_type=abstract
Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 92, no. 3, Feb. 1992, p. 517-532. Research supported by Mini
Astronomy and Astrophysics
Astrophysics
18
Argon Plasma, Dysprosium, Electron Transitions, Ferroelectricity, Metallic Plasmas, Line Spectra, Oscillator Strengths, Spectral Energy Distribution
Scientific paper
An argon-dysprosium plasma was generated at atmospheric pressure between a ceramic ferroelectric plate and a dysprosium plate. The system of plates was connected to an acoustic frequency power supply. The plasma radiation was analyzed in the spectral range from 2500 to 6700 A by using a grating spectrograph with a linear dispersion of about 1 mm/A, adapted for photoelectric measurements. The emission spectrum of dysprosium was recorded and the intensities of more than 500 DyI and DyII lines were measured. For 133 DyI-lines and 228 DyII-lines the transition probabilities, absorption oscillator strengths and log(gifik) were determined. The obtained values were compared with the literature data.
No associations
LandOfFree
Intensities and transition probabilities for selected DyI and DyII lines emitted from a ferroelectric plasma source does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Intensities and transition probabilities for selected DyI and DyII lines emitted from a ferroelectric plasma source, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Intensities and transition probabilities for selected DyI and DyII lines emitted from a ferroelectric plasma source will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1045238