Results 121 to 130 of about 1,497,004 (325)
Turbulent pair dispersion in the presence of gravity
Turbulent pair dispersion of heavy particles is strongly altered when particles of two different Stokes numbers (bidisperse) are considered, and this is further compounded when a uniform gravitational acceleration is present.
Kelken Chang+2 more
doaj +1 more source
Numerical simulation of gluey particles [PDF]
We propose here a model and a numerical scheme to compute the motion of rigid particles interacting through the lubrication force. In the case of a particle approaching a plane, we propose an algorithm and prove its convergence towards the solutions to the gluey particle model proposed by B. Maury.
openaire +3 more sources
An Analysis for IDH‐Mutant Grade 4 Astrocytoma Based on WHO CNS 5: Implication of Clinical Practice
ABSTRACT Purpose There is ongoing debate regarding the therapeutic approach and prognosis for IDH‐mutant grade 4 astrocytoma, a newly defined subtype of diffuse glioma in the 2021 WHO classification system for central nervous system tumors (WHO CNS 5). The aim of this study was to explore the clinical outcome and prognosticators for newly diagnosed IDH‐
Xianxin Qiu+13 more
wiley +1 more source
Bioinspired composite segmented armour: Numerical simulations
Nature has evolved ingenious armour designs, like the flexible carapaces of armadillo and boxfish consisting of hexagonal segments connected by collagen fibres, that serve as bioinspiration for modern ballistic armours.
Pedro Miranda+2 more
doaj
Numerical Simulation of Stationary and Non-Stationary Gaussian Random Processes [PDF]
Joel Franklin
openalex +1 more source
Numerical simulations of quasar absorbers [PDF]
The physical state of the intergalactic medium can be probed in great detail with the intervening absorption systems seen in quasar spectra. The properties of the Hydrogen absorbers depend on many cosmological parameters, such as the matter-power spectrum, reionisation history, ionising background and the nature of the dark matter.
openaire +4 more sources
Numerical Simulations of Driven Relativistic MHD Turbulence
A wide variety of astrophysical phenomena involve the flow of turbulent magnetized gas with relativistic velocity or energy density. Examples include gamma-ray bursts, active galactic nuclei, pulsars, magnetars, micro-quasars, merging neutron stars, X ...
Andrew I. MacFadyen+26 more
core +2 more sources
Simulation of Heat Flow in Porous Media Using Numerical Models [PDF]
F.R. Nicholson+2 more
openalex +1 more source
Numerical simulations of galactic wakes [PDF]
We have performed a series of numerical simulations which examine the simple but realistic case of a galaxy with a smooth potential corresponding to a King profile, and with no interstellar medium.
Lufkin, Eric A.
core +1 more source
Direct numerical simulations of aeolian sand ripples
Aeolian sand beds exhibit regular patterns of ripples resulting from the interaction between topography and sediment transport. Their characteristics have been so far related to reptation transport caused by the impacts on the ground of grains entrained ...
Andreotti, Bruno+2 more
core +1 more source