rock has been advantageously employed in hydraulic structures such as rockfill dams, gabion weirs and drain works. one rockfill dam applications can be flood control in wa-tershed management. the objectives of building rockfill detention dams are flow storage for a specific period and lowering of the outflow hydrograph. as this type of dam consists of coarse particles, seepage flow will deviate...

ABSTRACT We use the 30 simulations of Auriga Project to estimate temporal dependency inflow, outflow, and net accretion rates onto discs Milky Way-like galaxies. The are found be similar for all galaxies at early times, increasing rapidly up $\sim 10~\mathrm{M}_\odot \, \mathrm{yr}^{-1}$. After ∼6 Gyr evolution, however, diverse: in most galaxies, these exhibit an exponential-like decay, but so...

Intrasplenic pH in vivo was deduced from measurements on blood drained from cat spleen during contraction with the inflow occluded. The pH of blood in the red pulp is normally 7.20, but stasis or reduced flow through the pulp causes pH to fall toward 6.8. The splenic pulp contains blood of high hematocrit. To evaluate the role of buffering by the red cells themselves, intrasplenic p/ in red cel...

LEVESQUE, M. J. AND A. C. GROOM. pH environment of red ceLLs in the spleen. Am. J, Physiol. 231(6): 1672-1678. 1976. Intrasplenic pH in vivo was deduced from measurements on blood drained from cat spleen during contraction with the inflow occluded. The pH of blood in the red pulp is normally 7.20, but stasis or reduced flow through the pulp causes pH to fall toward 6.8. The splenic pulp contain...

We consider smali perturbations of plane parallel flow be&veer. a wail and a moving free surface. The problem is posed on a rectangle with inflow and out!low bout?dariss. The ~sua! boundary conditions are posed at the wall and the free surface, and the fluid satisfies the Navier-Stokes equations. We examine the nature of boundary conditions which car. be imposed at the inflow and outflow bounda...

We study the effect of surface brightness on the mass–metallicity relation using nearby galaxies whose gas content and metallicity profiles are available. Previous studies using fiber spectra indicated that lower surface brightness galaxies have systematically lower metallicities for their stellar mass, but the results were uncertain because of aperture effects. With stellar masses and surface ...