1949
DOI: 10.1103/physrev.76.662
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Interferometric Studies of Faster than Sound Phenomena. Part II. Analysis of Supersonic Air Jets

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Cited by 66 publications
(25 citation statements)
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“…In the late stages of a star's evolution, jets arising as a result of magneto-rotational stellar collapse 10 may play an important role in the explosion of some types of supernovae. 11 Laboratory studies of supersonic jets [12][13][14] have until recently been limited to relatively low pressure and Mach number, and to temperatures for which radiation transport is not an important mechanism. Consequently, detailed understanding of many phenomena for high Mach-number and radiative jets has been founded solely in numerical simulation using radiation hydrodynamic codes employing a variety of different algorithms for approximate solution of the fundamental nonlinear hydrodynamic equations.…”
Section: Introductionmentioning
confidence: 99%
“…In the late stages of a star's evolution, jets arising as a result of magneto-rotational stellar collapse 10 may play an important role in the explosion of some types of supernovae. 11 Laboratory studies of supersonic jets [12][13][14] have until recently been limited to relatively low pressure and Mach number, and to temperatures for which radiation transport is not an important mechanism. Consequently, detailed understanding of many phenomena for high Mach-number and radiative jets has been founded solely in numerical simulation using radiation hydrodynamic codes employing a variety of different algorithms for approximate solution of the fundamental nonlinear hydrodynamic equations.…”
Section: Introductionmentioning
confidence: 99%
“…where the mixture density of a two-phase dust-gas flow must be, mix Ladenburg et al [1949] and Lewis and Carlson [1964] have experimentally showed that the higher the value of K, the further downstream (i.e., the further away from the nozzle) the position of the first Mach disk. The higher the value of χ, the further upstream (i.e., the closer to the nozzle) the position of the first Mach disk.…”
Section: Validation Against Under-expanded Jetsmentioning
confidence: 99%
“…In a typical plinian cloud, the lower, thrusting, momentum-driven part has all the properties of underexpanded jets expanding into the atmosphere [Kieffer and Sturtevant, 1984;Valentine, 1998]; while the upper, turbulent, buoyantly-driven part is controlled by the atmospheric drag and the dissipation is induced by multiphase turbulence [Dartevelle, 2005]. As a matter of fact, the physics of underexpanded jets [e.g., Ladenburg et al, 1949;Lewis and Carlson, 1964;Kieffer and Sturtevant, 1984] and multiphase turbulent jets [e.g., Hishida et al, 1987;Violet et al, 1992] is well known and documented with accurate measurements to be used for validation purposes.…”
Section: Figurementioning
confidence: 99%
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