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Fluid dynamics is the study of fluids in motion. Velocity vectors are often used to illustrate fluid motion in applications like meteorology. For example, wind—the fluid motion of air in the atmosphere—can be represented by vectors indicating the speed and direction of the wind at any given point on a map. Another method for representing fluid motion is a streamline. A streamline represents the path of a small volume of fluid as it flows. When the flow pattern changes with time, the...
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Circular Orbits and Critical Velocity for Satellites01:16

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The Moon orbits around the Earth. In turn, the Earth (and other planets) orbit the Sun. The space directly above our atmosphere is filled with artificial satellites in orbit. One can examine the circular orbit, the simplest kind of orbit, to understand the relationship between the speed and the period of planets and satellites with respect to their positions and the bodies that they orbit.
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Torque Free Motion01:15

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The torque-free motion refers to the movement of a rigid body in space when no external torques are acting upon it. This type of motion can be observed in environments where there are no external forces or frictions, like in outer space. For example, a rotation of Mars in space is a torque-free motion. Mars is an axisymmetric object, meaning it has an axis of symmetry along which it rotates, designated as the z-axis. The rotating frame of reference is defined such that the center of mass of...
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Navier–Stokes Equations01:28

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For incompressible Newtonian fluids, where density remains constant, stresses show a linear relationship with the deformation rate, defined by normal and shear stresses. Normal stresses depend on the pressure exerted on the fluid and the rate of deformation in specific directions, which determines how fluid flows under varying pressures. Shear stresses, on the other hand, act tangentially across fluid layers. They explain how adjacent fluid layers slide relative to one another, connecting...
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Conservation of Angular Momentum: Application01:18

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A system's total angular momentum remains constant if the net external torque acting on the system is zero. Examples of such systems include a freely spinning bicycle tire that slows over time due to torque arising from friction, or the slowing of Earth's rotation over millions of years due to frictional forces exerted on tidal deformations. However in the absence of a net external torque, the angular momentum remains conserved. The conservation of angular momentum principle requires a...
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Eulerian and Lagrangian Flow Descriptions01:22

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Fluid flow analysis is critical in many scientific and engineering disciplines, and two principal approaches are used to describe this flow: the Eulerian and Lagrangian methods. These methods offer different perspectives on monitoring and analyzing the motion of fluids, each with distinct advantages depending on the scenario.
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Related Experiment Video

Updated: Aug 14, 2025

Preparation of Free-Surface Hyperbolic Water Vortices
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Preparation of Free-Surface Hyperbolic Water Vortices

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Vortex Motions in the Solar Atmosphere: Definitions, Theory, Observations, and Modelling.

K Tziotziou1, E Scullion2, S Shelyag3

  • 1Institute for Astronomy, Astrophysics, Space Applications and Remote Sensing, National Observatory of Athens, GR-15236 Penteli, Greece.

Space Science Reviews
|January 11, 2023
PubMed
Summary
This summary is machine-generated.

Solar vortex flows, crucial for energy transfer, are abundant on the Sun. This review synthesizes recent research on their dynamics, observations, and modeling, guiding future solar physics studies.

Keywords:
Magnetohydrodynamic wavesSolar atmosphereSunVortex flows

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Area of Science:

  • Solar physics
  • Plasma physics
  • Fluid dynamics

Background:

  • Vortex flows are prevalent on the solar surface and atmosphere.
  • They play a key role in solar convective turbulent dynamics and magnetic field interactions.
  • These flows facilitate mass, momentum, and energy transfer across solar atmospheric layers.

Purpose of the Study:

  • To provide a comprehensive review of solar vortex flows at granular scales.
  • To synthesize recent advancements in theory, observation, and modeling.
  • To identify future research directions in solar vortex dynamics.

Main Methods:

  • Review of documented research spanning theory, observations, and modeling.
  • Inclusion of recent observational data and innovative detection techniques.
  • Analysis of magnetohydrodynamic simulations and hydrostatic wave modeling.

Main Results:

  • Vortical flows exhibit complex dynamics and excite various waves.
  • They couple different layers of the solar atmosphere.
  • This review offers the first systematic overview of these granular-scale solar phenomena.

Conclusions:

  • Solar vortex flows are fundamental to understanding energy transport in the solar atmosphere.
  • New observational facilities and advanced simulations are crucial for future research.
  • Further investigation is needed to fully grasp the interconnected physics of these phenomena.