scholarly journals Explanation of the memory effect in argon

2005 ◽  
Vol 3 (2) ◽  
pp. 95-107 ◽  
Author(s):  
Vidosav Markovic ◽  
Sasa Gocic ◽  
Suzana Stamenkovic

Memory effect - the long time variation of the electrical breakdown time delay on the relaxation time td (?) was observed in argon 24 hours after relaxation times and explained by the long-lived metastable states remaining from the preceding glow. However, the quenching processes reducing the effective lifetime of metastable states several orders of magnitude below that relevant for the time scale of observation were neglected. By applying approximate gas phase models it was found that the early afterglow kinetics up to hundreds of milliseconds is dominated by the decay of molecular argon ions Ar2+ and the approximate value of their ambipolar diffusion coefficient is determined. After that, nitrogen atoms present as impurities and recombined on the cathode surface and/or field emission determine the breakdown time delay down to the cosmic rays and natural radioactivity level.

2006 ◽  
Vol 13 (8) ◽  
pp. 083502 ◽  
Author(s):  
Čedomir A. Maluckov ◽  
Jugoslav P. Karamarković ◽  
Miodrag K. Radović ◽  
Momčilo M. Pejović

2004 ◽  
Vol 11 (11) ◽  
pp. 5328-5334 ◽  
Author(s):  
Čedomir A. Maluckov ◽  
Jugoslav P. Karamarković ◽  
Miodrag K. Radović ◽  
Momčilo M. Pejović

2007 ◽  
Vol 5 (1) ◽  
pp. 33-44 ◽  
Author(s):  
Vidosav Markovic ◽  
Sasa Gocic ◽  
Suzana Stamenkovic

The homogeneous gas phase models of relaxation kinetics (application of the gas phase effective coefficients to represent surface losses) are applied for the study of charged and neutral active particles decay in neon afterglow. The experimental data obtained by the breakdown time delay measurements as a function of the relaxation time td (?) (memory curve) is modeled in early, as well as in late afterglow. The number density decay of metastable states can explain neither the early, nor the late afterglow kinetics (memory effect), because their effective lifetimes are of the order of milliseconds and are determined by numerous collision quenching processes. The afterglow kinetics up to hundreds of milliseconds is dominated by the decay of molecular neon Ne2 + and nitrogen ions N2 + (present as impurities) and the approximate value of N2 + ambipolar diffusion coefficient is determined. After the charged particle decay, the secondary emitted electrons from the surface catalyzed excitation of nitrogen atoms on the cathode determine the breakdown time delay down to the cosmic rays and natural radioactivity level. Due to the neglecting of number density spatial profiles, the homogeneous gas phase models give only the approximate values of the corresponding coefficients, but reproduce correctly other characteristics of afterglow kinetics from simple fits to the experimental data.


Author(s):  
Milic Pejovic ◽  
Sasa Dekic ◽  
Bojan Jovanovic ◽  
Irfan Fetahovic ◽  
Predrag Osmokrovic

2010 ◽  
Vol 81 (10) ◽  
pp. 105104 ◽  
Author(s):  
Milić M. Pejović ◽  
Dragan B. Denić ◽  
Momčilo M. Pejović ◽  
Nikola T. Nešić ◽  
Nikola Vasović

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