Add to ORKGThe electron temperature structure in a weakly ionized plasma is studied allowing the degree of ionization to vary across the shock wave. The values of the electron temperature and the downstream equilibrium temperature obtained with variable ionization are less than those for frozen ionization. The electron temperature rises sharply behind the shock for variable ionization while a gradual increase is predicted by frozen ionization
Comparison of appropriate theoretically derived line ratios with observational data can yield estima...
Astrophysical shocks are often collisionless shocks, in which the changes in plasma flow and tempera...
Astrophysical shocks are often collisionless shocks, in which the changes in plasma flow and tempera...
The electron temperature structure in a weakly ionized plasma is studied allowing the degree of ioni...
The response of complex ionized gas systems to the presence of nonuniform distribution of charged gr...
Electron temperature is reconsidered for weakly-ionized oxygen and nitrogen plasmas with its dischar...
Photoelectric measurements were made of the shock-excited spectrum of a mixture of helium and argon....
In this thesis, the effect of the step ionizations on the high and low energy electron temperature p...
The exact value of the electron-atom collisional ionization cross section for argon is not accuratel...
The paper presents a unified picture of the structure of steady one-dimensional shock waves in parti...
The paper describes shock-tube data on radiative cooling of an argon plasma, the electron density gr...
An investigation of the dynamics of shock waves in weakly ionized argon plasmas has been performed u...
An analysis and assessment of three mechanisms describing plasma/shock wave interactions was conduct...
Weakly ionized plasmas at or near 1 atm pressure, or atmospheric-pressure plasmas, have received inc...
In our attempt to find analytical solutions for breakdown waves, we employ a set of three-component ...
Comparison of appropriate theoretically derived line ratios with observational data can yield estima...
Astrophysical shocks are often collisionless shocks, in which the changes in plasma flow and tempera...
Astrophysical shocks are often collisionless shocks, in which the changes in plasma flow and tempera...
The electron temperature structure in a weakly ionized plasma is studied allowing the degree of ioni...
The response of complex ionized gas systems to the presence of nonuniform distribution of charged gr...
Electron temperature is reconsidered for weakly-ionized oxygen and nitrogen plasmas with its dischar...
Photoelectric measurements were made of the shock-excited spectrum of a mixture of helium and argon....
In this thesis, the effect of the step ionizations on the high and low energy electron temperature p...
The exact value of the electron-atom collisional ionization cross section for argon is not accuratel...
The paper presents a unified picture of the structure of steady one-dimensional shock waves in parti...
The paper describes shock-tube data on radiative cooling of an argon plasma, the electron density gr...
An investigation of the dynamics of shock waves in weakly ionized argon plasmas has been performed u...
An analysis and assessment of three mechanisms describing plasma/shock wave interactions was conduct...
Weakly ionized plasmas at or near 1 atm pressure, or atmospheric-pressure plasmas, have received inc...
In our attempt to find analytical solutions for breakdown waves, we employ a set of three-component ...
Comparison of appropriate theoretically derived line ratios with observational data can yield estima...
Astrophysical shocks are often collisionless shocks, in which the changes in plasma flow and tempera...
Astrophysical shocks are often collisionless shocks, in which the changes in plasma flow and tempera...