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Blast waveA blast wave in fluid dynamics is the pressure and flow resulting from the deposition of a large amount of energy in a small very localised volume. The flow field can be approximated as a lead shock wave, followed by a 'selfsimilar' subsonic flow field. Additional recommended knowledge
HistoryThe classic flow solution — the socalled "similarity solution" — was independently devised by Geoffrey Ingram Taylor^{[1]} and John von Neumann^{[2]} during World War II. After the war, the similarity solution was published by three other authors — L. I. Sedov^{[3]}, R. Latter^{[4]}, and J. LockwoodTaylor^{[5]} — who had discovered it independently^{[6]}. ApplicationsBombsIn response to an inquiry from the British MAUD Committee, G. I. Taylor estimated the amount of energy that would be released by the explosion of an atomic bomb in air. He postulated that for an idealized point source of energy, the spatial distributions of the flow variables would have the same form during a given time interval, the variables differing only in scale. (Thus the name of the "similarity solution.") This hypothesis allowed the partial differential equations in terms of r (the radius of the blast wave) and t (time) to be transformed into an ordinary differential equation in terms of the similarity variable , where ρ_{o} is the density of the air and E is the energy that's released by the explosion^{[7]}^{[8]}^{[9]}. This result allowed G. I. Taylor to estimate the yield of the first atomic explosion in New Mexico in 1945 using only photographs of the blast, which had been published in newspapers and magazines^{[6]}. The yield of the explosion was determined by using the equation: , where C is a dimensionless constant that is a function of the ratio of the specific heat of air at constant pressure to the specific heat of air at constant volume. In 1950, G. I. Taylor published two articles in which he revealed the yield E of the first atomic explosion^{[10]}, which had previously been classified and whose publication therefore caused a great todo. AstronomyThis so called SedovTaylor solution has become useful in astrophysics, i.a. for quantitative estimation of the outcome from supernovaexplosions. References
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This article is licensed under the GNU Free Documentation License. It uses material from the Wikipedia article "Blast_wave". A list of authors is available in Wikipedia. 