Search results
Results from the WOW.Com Content Network
The heliospheric current sheet, or interplanetary current sheet, is a surface separating regions of the heliosphere where the interplanetary magnetic field points toward and away from the Sun. [1] A small electrical current with a current density of about 10 −10 A /m 2 flows within this surface, forming a current sheet confined to this surface.
As shown by dimensional analysis and in experiments by Sarpkaya, these coefficients depend in general on the Keulegan–Carpenter number, Reynolds number and surface roughness. [4] [5] The descriptions given below of the Morison equation are for uni-directional onflow conditions as well as body motion.
Flux F through a surface, dS is the differential vector area element, n is the unit normal to the surface. Left: No flux passes in the surface, the maximum amount flows normal to the surface. Right: The reduction in flux passing through a surface can be visualized by reduction in F or dS equivalently (resolved into components, θ is angle to ...
The surface tension σ is force per unit length of a surface element and acts tangential to the free surface. f σ = σ d l {\displaystyle f_{\sigma }=\sigma \ dl} For an infinitesimally small surface element dS , the tangential components of the surface tension forces cancel out when σ = constant , and the normal component can be expressed as ...
Atmospheric GCMs (AGCMs) model the atmosphere (and typically contain a land-surface model as well) using imposed sea surface temperatures (SSTs). [5] They may include atmospheric chemistry. AGCMs consist of a dynamical core which integrates the equations of fluid motion, typically for: surface pressure; horizontal components of velocity in layers
A geostrophic current is an oceanic current in which the pressure gradient force is balanced by the Coriolis effect. The direction of geostrophic flow is parallel to the isobars , with the high pressure to the right of the flow in the Northern Hemisphere , and the high pressure to the left in the Southern Hemisphere .
Solving the geodesic equations is a procedure used in mathematics, particularly Riemannian geometry, and in physics, particularly in general relativity, that results in obtaining geodesics. Physically, these represent the paths of (usually ideal) particles with no proper acceleration , their motion satisfying the geodesic equations.
First the system is progressed in time to a mid-time-step position, solving the above transport equations for mass and momentum using a suitable advection method. This is denoted the predictor step. At this point an initial projection may be implemented such that the mid-time-step velocity field is enforced as divergence free.