Later, Chen and Guo [17] studied the existence of blow-up solutions and the strong instability of standing waves.
Considering the strong instability of TiO2 nanoparticles, the value obtained is in disagreement with the empirical limit of |30| mV, over which a nanofluid should remain stable.
One or more of the following factors can account for superlative liquid water content in the mixed-phase region, i.e., strong instability, strong updraft, greater cloud base height, and high aerosol concentration.
Mixed with the effect of third bodies (Moon and Sun), this commensurability is on the basis of a strong instability of the Galileo constellation.
Strong instability and updraft can account for the high cloud water concentrations in the mixed-phase region and are thus necessary conditions for formation of inverted polarity thunderstorms to occur.
If the solution does not depend "smoothly" on the problem data, small variations on the data could create huge variations on the solutions, resulting in strong instability which is not acceptable.
In such a case, because of this intrinsic strong instability, the main difficulty of any numerical computation is the ability of discovering at run time, only using data, what is the maximum attainable accuracy on the solution.
This comprehensive study reveals the existence of a strong instability in the loading that results from changes in sand particle reflection during dynamic evolution of the panel's surface topology.
For a sufficiently large activation energy, the strong instability appears in the propagation of the plane detonation front, a quasi-steady regime may be observed during the direct initiation for the initiation energy near the critical value.
Strong instability occurred in the vicinity of the area as a result of surface heating.
