Astronomy and Astrophysics – Astrophysics
Scientific paper
Mar 1978
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978a%26a....64..111k&link_type=abstract
Astronomy and Astrophysics, vol. 64, no. 1-2, Mar. 1978, p. 111-113.
Astronomy and Astrophysics
Astrophysics
23
Line Spectra, Oscillators, Plasma Resonance, Titanium, Absorption Spectra, Arc Generators, Doppler Effect, Light Sources, Plasma Density
Scientific paper
A method combining emission measurements of lines from a common upper level with hook measurements of lines from a common lower level has been applied to obtain 24 relative f-values of Ti I resonance lines without any assumption concerning the state of the plasma used. Modified cascaded arcs in titanium chloride vapor with argon as the carrier gas were employed for both the emission and the hook measurements. Starting from the 24 hooked resonance lines, 11 sets of relative f-values with a total of 33 additional lines in the wavelength region from 3900 to 7900 A were determined and then normalized by using the f-values of the resonance lines. The accuracies are estimated to be within 13% to 33%, and the method employed to measure the f-values is compared with a method that requires an LTE plasma. The f-values determined are compared with the results of two previous experimental investigations.
Danzmann Karsten
Kock Manfred
Kuehne Martin
No associations
LandOfFree
Oscillator strengths of TI I from hook and emission measurements 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 Oscillator strengths of TI I from hook and emission measurements, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Oscillator strengths of TI I from hook and emission measurements will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1078387