Detail publikačního výsledku

Influence of Metal Traces on Kinetics of a Nitrogen Glow Discharge in Post-Discharge Period

KANICKÝ, V.; OTRUBA, V.; HRDLIČKA, A.; KRÁSENSKÝ, P.; KRČMA, F.

Originální název

Influence of Metal Traces on Kinetics of a Nitrogen Glow Discharge in Post-Discharge Period

Anglický název

Influence of Metal Traces on Kinetics of a Nitrogen Glow Discharge in Post-Discharge Period

Druh

Článek recenzovaný mimo WoS a Scopus

Originální abstrakt

The DC flowing post-discharge in nitrogen containing mercury traces of about 3.14 ppb was studied in Pyrex tube by emission spectroscopy. The relative populations of N_2 (B ^3 Pi_g), N_2 (C ^3 Pi_u) and N_2^+ (B ^2 Sigma_u^+) states were calculated in the dependence on the post-discharge time in the range of 3 - 40 ms. As the uncontrolled oxygen traces were recorded in the mercury flow the experiment with nitrogen-oxygen mixture was added. The results showed strong quenching of the nitrogen pink afterglow by mercury traces. The kinetic explanation should be done through strong depopulation of level N_2 (X ^1 Sigma_g^+,v = 20) (creation of mercury ^3 P_1 state) and levels N_2 (X ^1 Sigma_g^+, v = 28) or N_2 (A ^3 Sigma_u^+,v = 4) (creation of mercury ^1 S_0 state). Both mercury states are origins of UV light emission (254, resp. 185 nm) that could not be detected in our experimental set up.

Anglický abstrakt

The DC flowing post-discharge in nitrogen containing mercury traces of about 3.14 ppb was studied in Pyrex tube by emission spectroscopy. The relative populations of N_2 (B ^3 Pi_g), N_2 (C ^3 Pi_u) and N_2^+ (B ^2 Sigma_u^+) states were calculated in the dependence on the post-discharge time in the range of 3 - 40 ms. As the uncontrolled oxygen traces were recorded in the mercury flow the experiment with nitrogen-oxygen mixture was added. The results showed strong quenching of the nitrogen pink afterglow by mercury traces. The kinetic explanation should be done through strong depopulation of level N_2 (X ^1 Sigma_g^+,v = 20) (creation of mercury ^3 P_1 state) and levels N_2 (X ^1 Sigma_g^+, v = 28) or N_2 (A ^3 Sigma_u^+,v = 4) (creation of mercury ^1 S_0 state). Both mercury states are origins of UV light emission (254, resp. 185 nm) that could not be detected in our experimental set up.

Klíčová slova

nitrogen post-discharge, pink afterglow, post-discharge kinetics, optical spectroscopy, mercury traces

Klíčová slova v angličtině

nitrogen post-discharge, pink afterglow, post-discharge kinetics, optical spectroscopy, mercury traces

Autoři

KANICKÝ, V.; OTRUBA, V.; HRDLIČKA, A.; KRÁSENSKÝ, P.; KRČMA, F.

Vydáno

27.11.2006

Nakladatel

ICP Information Newsletter, Inc.

Místo

Amherst, USA

ISSN

0161-6951

Periodikum

ICP Information Newsletter

Svazek

32

Číslo

6S

Stát

Spojené státy americké

Strany od

159

Strany do

160

Strany počet

2

BibTex

@article{BUT43653,
  author="Viktor {Kanický} and Vítězslav {Otruba} and Aleš {Hrdlička} and Pavel {Krásenský} and František {Krčma}",
  title="Influence of Metal Traces on Kinetics of a Nitrogen Glow Discharge in Post-Discharge Period",
  journal="ICP Information Newsletter",
  year="2006",
  volume="32",
  number="6S",
  pages="159--160",
  issn="0161-6951"
}