Study Of Titanium Emission Spectra In N2 - H2 Abnormal DC Glow Discharge

Details Study Of Titanium Emission Spectra In N2 - H2 Abnormal DC Glow Discharge Study Of Titanium Emission Spectra In N2 - H2 Abnormal DC Glow Discharge

Jul 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010pobeo..89..225o&link_type=abstract

Publications of the Astronomical Observatory of Belgrade, vol. 89, pp. 225-228

Astronomy and Astrophysics

Astronomy

Scientific paper

In this paper we tried to answer why small amount of hydrogen (3 %) in a nitrogen abnormal glow discharge so strongly reduce Ti I spectral line intensities. Decreasing of Ti I line intensities in N2 - H2 discharge are compared with less pronounced decreasing of N I line intensities. Using emission spectroscopy we have observed that line intensity changes are correlated to variations in electron energy distribution function (EEDF) and change of metastable density.

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