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explosive
The correlation coefficient is found to exhibit quasi-periodic variations with increasing distance to the explosive source of sound.
      
The experiments are performed in the Black Sea, on a 600-km-long path, with explosive sound sources.
      
Temporal energy fluctuations of impuse signals generated by powerful explosive sources of sound are considered by using the experimental data obtained on a long-distance stationary path in the northwestern Pacific.
      
In a close neutron star binary resulting from the collapse of the rotating iron core of a collapsing supernova, the low-mass component of mass m undergoes explosive disruption at the final evolutionary stage of this binary.
      
This indicates the dominance of explosive oxygen burning in massive type II supernovae during the synthesis of potassium in the Galactic disk.
      
Explosive evaporation simultaneously increases both the temperature and the density of the plasma at the loop top.
      
The flare and coronal mass ejection result from the explosive decay of the current sheet.
      
The motion of a small-scale CME occurs within a magnetic flux tube (ray of enhanced brightness) and leads to an explosive increase in its angular size (rapid expansion of the tube).
      
We consider the evolution of close binaries resulting in the most intensive explosive phenomena in the stellar Universe-Type Ia supernovae and gamma-ray bursts.
      
The fact such a frequent spectrum does exist supports the idea that both soft and hard protons are efficiently accelerated, probably by a single mechanism that operates during the explosive phases of the flares.
      
Thus, there are two sources of the particle acceleration operating at low and high altitudes during the explosive and post-eruptive phases of the solar flares, respectively.
      
In the problem of explosive crystallization of amorphous films, the sources have the same sign.
      
Analysis of the experimental atomic radial distribution functions for thin amorphous films of zinc phosphides obtained by explosive laser sputtering has been performed within a fragmentary model.
      
Explosive regime of the development of instability leading to vapor-film collapse on a heated solid hemispherical surface
      
Explosive crystallization initiated in nanocrystalline iron-carbon films by an electron beam
      
Shock wave processes and cumulation in a steel ball under quasi-spherical explosive loading with perturbation
      
The initial stage of explosive volcanic eruption: The dynamics of the magma state in depression waves
      
The argon was compressed by a cylindrical shell accelerated by the detonation products of an explosive.
      
A range of parameters is found in which four-wave interactions saturate the explosive instability, which explains the appearance of stable hexagons in the experiment.
      
Outside this region, nonlinearities of higher order saturate the explosive instability, and the process of hexagon generation must be studied numerically.
      
 

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