Mechanisms of pelleting flocculation

Basically speaking, flocculation and coagulation should be theoretically treated as a many-body problem. However, such potential energy theories of coagulation as the DLVO theory have been developed as a two-body problem, i.e., interaction between two plates or two particles in an infinite medium. The concept volume fraction of the constituent particles in the floc, i.e., voidage fraction in the floc is excluded from these theories and, therefore, the traditional theories are not applicable to the phenomenon of “pelleting flocculation”.In an effort to formulate a theory of flocculation that leads to pellet-like flocs, three possible mechanisms of flocculation process are involved, i.e., (1) perikinetic flocculation, (2) orthokinetic flocculation, and (3) an additional process of mechanical syneresis. A few hypotheses are also presented, which may become the prelude to a subsequent flocculation theory.     

Numerical analysis on seismic response of Shinkansen bridge-train interaction system under moderate earthquakes

This study is intended to evaluate the influence of dynamic bridge-train interaction (BTI) on the seismic response of the Shinkansen system in Japan under moderate earthquakes. An analytical approach to simulate the seismic response of the BTI system is developed. In this approach, the behavior of the bridge structure is assumed to be within the elastic range under moderate ground motions. A bullet train car model idealized as a sprung-mass system is established. The viaduct is modeled with 3D finite elements. The BTI analysis algorithm is verified by comparing the analytical and experimental results. The seismic analysis is validated through comparison with a general program. Then, the seismic responses of the BTI system are simulated and evaluated. Some useful conclusions are drawn, indicating the importance of a proper consideration of the dynamic BTI in seismic design.     

Nonequilibrium Processes in the Solar Corona,Transition Region,Flares, and Solar Wind <Emphasis Type="Italic">(Invited Review)</Emphasis>

We review the presence and signatures of the non-equilibrium processes, both non-Maxwellian distributions and non-equilibrium ionization, in the solar transition region, corona, solar wind, and flares. Basic properties of the non-Maxwellian distributions are described together with their influence on the heat flux as well as on the rates of individual collisional processes and the resulting optically thin synthetic spectra. Constraints on the presence of high-energy electrons from observations are reviewed, including positive detection of non-Maxwellian distributions in the solar corona, transition region, flares, and wind. Occurrence of non-equilibrium ionization is reviewed as well, especially in connection to hydrodynamic and generalized collisional-radiative modeling. Predicted spectroscopic signatures of non-equilibrium ionization depending on the assumed plasma conditions are summarized. Finally, we discuss the future remote-sensing instrumentation that can be used for the detection of these non-equilibrium phenomena in various spectral ranges.