The experiments have provided strong support for the validity of our computational approach.
Short-term experiments have provided confusing results, but a real test takes years.
Additional experiments have provided the laws for breakage, exhibiting the influence of mass transfer.
Previous experiments have provided a model of the process and values for its parameters.
The results of these experiments have provided encouraging initial evidence about the plausibility of our approach and are discussed in the paper.
These experiments have provided abundant information to aid in the development of our scientific understanding of environmental impacts of CO2 while assessing state of the art monitoring techniques.
The results of these experiments have provided insight into the causal relationships between the turbulent flow field, unsteady surface pressure, and radiated far field acoustics.
These experiments have provided a wealth of accurate data on the properties of the interplanetary plasma, on the earth's magnetosphere, and on the interaction of the solar wind with the Moon, Venus and Mercury, Mars, Jupiter, Saturn, Uranus, and Neptune.
Experiments have provided evidence that a much faster propagation of the front occurs in solutions than that predicted by reaction diffusion (RD) theories, thereby suggesting the influence of convective effects arising if A, B, and C have different densities.
Hard X-ray diffraction experiments have provided evidence of a strongly heterogeneous distribution of dislocation densities along the axis of cylindrical ice single crystals oriented for basal slip in torsion creep.
The diffraction experiments have provided characteristically asymmetric line profiles which were evaluated for the dislocation densities and arrangements and for the residual long-range internal stresses prevailing in a dislocation cell structure.
