Sentence examples for shock flow from inspiring English sources

The unidirectional shock flow has been observed from currency market to equity market for Japan, India, US, Korea and Canada only.

This is also known as first-order Fermi acceleration, in which the cosmic rays gain energy as they are scattered by turbulence upstream and downstream of the shock, repeatedly cross the shock, and are effectively compressed by shock flow Blandford and Eichler (1987).

The model includes the determination of the particle's injection energy, the maximum energy of particles accelerated at the shock, energetic particle spectra at all spatial and temporal locations, and the dynamical distribution of particles that are trapped in the post shock flow and those that escape upstream and downstream of the evolving shock complex.

To assess the clinical relevance of the increase in PD-1-related molecule expressions after septic shock, flow cytometric measurements were correlated with clinical parameters and usual biomarkers of sepsis-induced immunosuppression.

Our work demonstrates the feasibility of VMS methods for highly transient shock flows, an area of research for which the VMS literature is extremely scarce.

Numerical simulations of non-linear CR acceleration at converging shock flows have revealed that these accelerators can provide very hard spectra of protons up to 1016 1017 eV which is well above the "knee" in the all-particle CR spectrum at about 3×1015 eV.

In the immediate post-shock flow, Venus has a magnetosheath region just like that of any other magnetized planet.

The validation process proposed by Babuška et al. [1] is applied to thermochemical models describing post-shock flow conditions.

This optimal geometry bifurcates the shock-wave and carefully manages the recovering post-shock flow to maximise pressure-smearing in the shock-region with only a small penalty in L/D for the aerofoil.

The trapping and channeling of their stellar winds in closed magnetic loops leads to magnetically confined wind shocks (MCWS), with pre-shock flow speeds that are some fraction of the wind terminal speed.

The steady-state inviscid and nearly inviscid Burgers' equations and the Euler equations for steady-state shocked flow in a quasi-1-dimensional nozzle are discretized by cell-centered finite differences on the cells of an arbitrarily spaced grid.