1971
DOI: 10.1103/physreva.4.2368
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Validity of the Quasisteady State and Collisional-Radiative Recombination for Helium Plasmas. I. Pure Afterglows

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Cited by 34 publications
(6 citation statements)
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“…Soon after, however, it was recognized the importance of a time dependent integration of kinetic equations which are at the basis of the c-r models for situations characterized by very short macroscopic relaxation times. Time dependent solution of c-r models have been presented by Cacciatore et al [2][3][4][5] for atomic H, O and N plasmas many years ago and more recently these plasmas [6][7][8] have been again studied for explaining new experimental situations (e.g. laser-plasmas interaction) in which a time dependent solution of c-r models seems to be necessary.…”
Section: Introductionmentioning
confidence: 99%
See 1 more Smart Citation
“…Soon after, however, it was recognized the importance of a time dependent integration of kinetic equations which are at the basis of the c-r models for situations characterized by very short macroscopic relaxation times. Time dependent solution of c-r models have been presented by Cacciatore et al [2][3][4][5] for atomic H, O and N plasmas many years ago and more recently these plasmas [6][7][8] have been again studied for explaining new experimental situations (e.g. laser-plasmas interaction) in which a time dependent solution of c-r models seems to be necessary.…”
Section: Introductionmentioning
confidence: 99%
“…laser-plasmas interaction) in which a time dependent solution of c-r models seems to be necessary. In these papers [2][3][4][5], rate coefficients of e-A collisions are calculated approximating the eedf with the Maxwell distribution at a fixed temperature (free electron kinetics have been neglected). This assumption is realistic only if the ionization degree is high enough so that electron-electron Coulomb collisions (e-e) dominates the free electron kinetics.…”
Section: Introductionmentioning
confidence: 99%
“…The intensity of the hydrogen spectral line radiation, in the case of pure hydrogen, is considerably enhanced during the perturbation, and this is followed by a drop of intensity below the stationary value immediately after. 0022-37271821040631 + 07 $02.00 0 1982 The Institute of Physics Few attempts have been made to calculate theoretically the time behaviour of level population in the nonstationary plasma (Cacciatore andCapitelli 1974, Limbaugh andMason 1972). Population relaxation was studied for various initial conditions that were chosen arbitrarily and therefore an application of this calculation requires a knowledge of instantaneous values of population at the beginning of the relaxation.…”
Section: Introductionmentioning
confidence: 99%
“…Gordiets, Gudsenko & Shelepsin (1968) used a R unge-K utta method to obtain approximate population densities for a hydrogen plasma a t various times and temperatures and included both collisional and radiative processes. On the other hand, Limbaugh & Mason (1971) were more concerned with investigating the validity of the quasi-steady-state approximation in their work on a helium plasma. Their method of integration was a modified Euler method and they obtained values for the collisional-radiative recombination coefficient as a function of time.…”
Section: Introductionmentioning
confidence: 99%