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Titlebook: Seminar on Concurrency; Carnegie-Mellon Univ Stephen D. Brookes,Andrew William Roscoe,Glynn Win Conference proceedings 1985 Springer-Verlag

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楼主: Dopamine
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Robin Milnerly the theories for their formation and propagation. The major advances achieved in recent years are reviewed, regarding the observed morphology, kinematics and excitation properties of jets, from the parsec-scale ‘giant outflows’ down to the ‘microjets’ from T Tauri stars. High angular resolution i
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Stephen D. Brookesrstanding of stellar jets is therefore fundamental to any theory of Star Formation. The motivation of the four-year JETSET (Jet Simulations, Experiments and Theory) Marie Curie Research Training Network is to build an int- disciplinary European research community focused on the study of jets from yo
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Glynn Winskels from laser and z-pinch plasma experiments,.·  the magnetohydrodynamic theory of relativistic and non-relativistic stationary jets,.·  heating mechanisms in magnetohydrodynamic jets, from the solar magnetic reconnection to the molecular shock heating perspectives,.·  atomic and molecular microphysi
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J. A. Bergstra,J. W. Klop,J. V. Tuckerions and key questions for jet physics: • Higher resolution 3D simulations, including large-eddy or direct simulations. • Three dimensional studies of jet disruption and the transition to turbulence in jets: Norman, Burns and Sulkanen (1988) have shown that the passage of a 2D jet through a shock ca
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Ben Moszkowskiaturally formed in the rapidly rotating magnetospheres of geometrically thin accretion disks around rotating black holes. Disk fields generated by dynamo effects in the boundary layer between disk and rotating hole immerse the hole in a rotating magnetosphere which is loaded by plasma from the disk.
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Gul Agha 30° to 55° depending on the ratio of the mass flow rates of disk wind and stellar wind. The maximum speed of the outflow is about the Keplerian speed at the inner disk radius. An axial jet forms during the first decades of rotations. However, this feature does not survive on the very long time scal
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