
Rate of change of position of a fluid element, measured along or transverse to flow.Velocity in fluid dynamics is the rate of change of position of a fluid element, measured along or transverse to the flow direction. It is a fundamental field variable that describes how fluid particles move through space and time. Understanding velocity is crucial for analyzing fluid behavior, from laminar flows in porous media to turbulent eddies in oceans and atmospheres.
The concept of velocity in fluids was formalized by Leonhard Euler in the 18th century, who introduced the idea of a velocity field. Later, Claude-Louis Navier and George Gabriel Stokes developed the equations that bear their names, providing a mathematical framework for velocity in viscous flows.
Velocity is a vector quantity, meaning it has both magnitude and direction. In fluid dynamics, it is often described by a velocity field, which assigns a velocity vector to every point in the fluid. This field is governed by equations like the Navier-Stokes equations, which relate velocity to pressure, density, and external forces. Measurements of velocity can be made using techniques like particle image velocimetry or Doppler anemometry.
Velocity measurements are used in weather forecasting to track wind patterns, in oceanography to monitor currents, and in engineering to design pipelines and aircraft.
In turbulent flows, velocity fluctuates chaotically, and even the most powerful supercomputers cannot fully simulate the smallest eddies.
| Δz | variable | redshift change — redshift |
| v | variable | line-of-sight velocity — velocity metre per second |
| c | variable | speed of light — speed of light metre per second |
| v | variable | orbital speed — velocity metre per second |
| M | variable | central mass — mass kilogram |
| r | variable | orbital radius — radius metre |
| G | constant | Universal constant of gravitation, determining the strength of gravitational force. — gravitational constant = 6.67430e-11 cubic metre per kilogram per second squared |
| z | variable | redshift parameter — redshift |
| v | variable | relative velocity between source and observer — velocity metre per second |
| θ | variable | angle between velocity vector and line of sight — angle radian |
| c | constant | speed of light in vacuum — speed of light = 299792458 metre per second |
| cos | operator | trigonometric cosine function — cosine |
| F | variable | Force on the sail — force newton |
| A | variable | Area of the sail — area square metre |
| s | variable | Poynting flux (power per unit area) of incident light — irradiance watt per square metre |
| v | variable | Speed of the sail relative to the light source — velocity metre per second |
| c | constant | Universal constant, speed of light in vacuum — speed of light = 299792458 metre per second |
| \cdot | operator | Product of quantities — multiplication |
| \frac{1 - v/c}{1 + v | operator | Ratio of reflected to incident photon energy and rate — doppler factor squared |
| \nu_{\text{out}} | variable | Observed frequency of reflected light — frequency hertz |
| \nu_{\text{in}} | variable | Frequency of incident light in the source frame — frequency hertz |
| v | variable | Speed of the mirror relative to the source — velocity metre per second |
| c | constant | Universal constant, speed of light in vacuum — speed of light = 299792458 metre per second |
| \frac{1 - v/c}{1 + v | operator | Ratio of observed to emitted frequency for a receding source — doppler factor |






















