Astronomy and Astrophysics – Astronomy
Scientific paper
Jul 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008pobeo..84...39k&link_type=abstract
Publications of the Astronomical Observatory of Belgrade, vol 84, pp. 39-44
Astronomy and Astrophysics
Astronomy
Scientific paper
The flowing afterglow study of recombination of D_3^+ ions with electrons and measurements of recombination rate coefficients in He-Ar-D_2 plasma at several temperatures and buffer gas pressures, and over a wide range of deuterium number densities are reported. The influence of helium number density on overall recombination rate coefficient was observed. The results indicate the multicollision character of the recombination process in D_3^+ dominated low temperature plasma. The obtained binary and ternary recombination rate coefficients are: alpha_bin (250 K)=(4.1 +- 1.2) x 10^-8 cm^3 s^-1, K_He (250 K)=(2.1 +- 0.7) x 10^-25 cm^6 s^-1.
Dohnal P.
Glosik Juraj
Korolov I.
Kotrik T.
Plasil Radek
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