Author Institution: General Atomic Division, General Dynamics CorporationA preliminary theoretical study of an explosive-driven argon shock, using measured shock velocities, indicated shock temperatures of $23,000^{\circ}K$. Opacity calculations showed the precursor radiant flux in a tube of 60 cm length should be that of a blackbody of the above temperature up to photon energies near that of the first excited state of argon $(h\nu = 11.5 ev)$. This total calculated flux is 1.4 megawatts. Flux measurements using ablation and bolometer detectors showed 0.2-0.3 megawatts with little or none of this in the ultraviolet. This low flux can be explained by a high ultraviolet opacity of the cool argon ahead of the shock due to the absorption of res...
NOTE: Text or symbols not renderable in plain ASCII are indicated by [...]. Abstract is included in ...
X-ray Thomson scattering has enabled us to measure the temperature of a shocked layer, produced in t...
Entering the atmosphere of a planet is one of the key phases of many space missions, being significa...
The plasmas produced in electromagnetic shock tubes have previously been studied in this laboratory ...
The preionization of a shock tube's gas before the shock passes through it is called the precursor e...
The aim of this project was to investigate the effect of radiation loss on the various flows associ...
Abstract. Strong shock waves propagating in argon gas exhibit a variety of precursor effects. The ma...
At signifcantly large pressures, shock waves can be driven that are so energetic that radiation star...
A chemical kinetic model describing photochemical reactions that are likely to be important in "co...
The paper describes shock-tube data on radiative cooling of an argon plasma, the electron density gr...
The radiative energy loss from an argon plasma in a shock tube has been investigated, with emphasis ...
Absorption coefficients of high temperature air have been measured photoelectrically over the temper...
Converging shock waves have been studied experimentally in a shock tube, and numerically using invis...
Abstract-Measurement o f optical properties of plasmas is de-scribed as an important application o f...
Results from spectral radiance measurements using optical multi-channel analyzer over the visible an...
NOTE: Text or symbols not renderable in plain ASCII are indicated by [...]. Abstract is included in ...
X-ray Thomson scattering has enabled us to measure the temperature of a shocked layer, produced in t...
Entering the atmosphere of a planet is one of the key phases of many space missions, being significa...
The plasmas produced in electromagnetic shock tubes have previously been studied in this laboratory ...
The preionization of a shock tube's gas before the shock passes through it is called the precursor e...
The aim of this project was to investigate the effect of radiation loss on the various flows associ...
Abstract. Strong shock waves propagating in argon gas exhibit a variety of precursor effects. The ma...
At signifcantly large pressures, shock waves can be driven that are so energetic that radiation star...
A chemical kinetic model describing photochemical reactions that are likely to be important in "co...
The paper describes shock-tube data on radiative cooling of an argon plasma, the electron density gr...
The radiative energy loss from an argon plasma in a shock tube has been investigated, with emphasis ...
Absorption coefficients of high temperature air have been measured photoelectrically over the temper...
Converging shock waves have been studied experimentally in a shock tube, and numerically using invis...
Abstract-Measurement o f optical properties of plasmas is de-scribed as an important application o f...
Results from spectral radiance measurements using optical multi-channel analyzer over the visible an...
NOTE: Text or symbols not renderable in plain ASCII are indicated by [...]. Abstract is included in ...
X-ray Thomson scattering has enabled us to measure the temperature of a shocked layer, produced in t...
Entering the atmosphere of a planet is one of the key phases of many space missions, being significa...