Titlebook: High Energy Density Laboratory Astrophysics; Sergey V. Lebedev Conference proceedings 2007 Springer Science+Business Media B.V. 2007 Accre

ATP861

Climate

招人嫉妒

Magnetic-Tower Jet Solution for Launching Astrophysical Jetshave been developed since 2000, the launching mechanisms of jets is somewhat controversial. Previous studies of jets have concentrated on the effect of the large-scale magnetic fields permeating accretion disks. However, the existence of such global magnetic fields is not evident in various astrophy

半導(dǎo)體

有效

defile

Jet Deflection by a Quasi-Steady-State Side Wind in the Laboratory region enables internal shocks to fully cross the jet, leading to the development of significantly more structure in the jet than in previous work with a similar setup (.). The ability to control the length of the interaction region in the laboratory allows the switch between a regime representing

ASSAY

推崇

Plasma Jet Studies via the Flow Z-Pinchof an embedded radial shear in the axial flow is correlated with the observed stability, and is in agreement with numerical predictions of the stability threshold. The case is made that using a higher-Z working gas will produce supersonic plasma jets, consistent with dimensionless similarity constra

有節(jié)制

Double-Pulse Laser-Driven Jets on OMEGAst laser experiments to generate pulsed outflow. The temporal laser-intensity profile consists of two 1-ns square pulses separated by 9.6 ns. The laser is focused on a truncated conical plug made of medium . material inserted into a high-. washer. Unloading material from the plug is collimated withi

Humble

Laboratory Modeling of Standing Shocks and Radiatively Cooled Jets with Angular Momentumetion disk. We discuss the first experiments to simulate rotating radiatively cooled, hypersonic jets in the laboratory. A modification of the conical wire array .-pinch is used to introduce angular momentum into convergent flows of plasma, a jet-forming standing shock and into the jet itself. The r