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Velocity and Acceleration of a Wave00:51

Velocity and Acceleration of a Wave

A wave propagates through a medium with a constant speed, known as a wave velocity. It is different from the speed of the particles of the medium, which is not constant. In addition, the velocity of the medium is perpendicular to the velocity of the wave. The variable speed of the particles of the medium implies that there must be acceleration associated with it. 
The velocity of the particles can be obtained by taking the partial derivative of the position equation with respect to time. We can...
Travelling Waves01:04

Travelling Waves

A wave is a disturbance that propagates from its source, repeating itself periodically, and is typically associated with simple harmonic motion. Mechanical waves are governed by Newton's laws and require a medium to travel. A medium is a substance in which a mechanical wave propagates, and the medium produces an elastic restoring force when it is deformed.
Water waves, sound waves, and seismic waves are some examples of mechanical waves. For water waves, the wave propagation medium is water;...
Propagation of Waves01:07

Propagation of Waves

When a wave propagates from one medium to another, part of it may get reflected in the first medium, and part of it may get transmitted to the second medium. In such a case, the interface of the two mediums can be considered as a boundary that is neither fixed nor free.
Consider a scenario where a wave propagates from a string of low linear mass density to a string of high linear mass density. In such a case, the reflected wave is out of phase with respect to the incident wave, however the...
Equations of Wave Motion01:02

Equations of Wave Motion

Mathematically, the motion of a wave can be studied using a wavefunction. Consider a string oscillating up and down in simple harmonic motion, having a period T. The wave on the string is sinusoidal and is translated in the positive x-direction as time progresses. Sine is a function of the angle θ, oscillating between +A and −A and repeating every 2π radians. To construct a wave model, the ratio of the angle θ and the position x is considered.
Euler's Equations of Motion01:28

Euler's Equations of Motion

In fluid mechanics, shear stresses arise from viscosity, which represents a fluid's internal resistance to deformation. For low-viscosity fluids, like water, these stresses are minimal, simplifying flow analysis by allowing the fluid to be treated as inviscid, or frictionless. In an inviscid fluid, shear stresses are absent, leaving only normal stresses, which act perpendicularly to fluid elements. Notably, pressure — defined as the negative of the normal stress — remains uniform across...
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Standing Waves in a Cavity

A household microwave and lasers are examples of standing electromagnetic waves in a cavity. When two conducting metal plates are placed parallel at the nodal planes, it creates a cavity where standing waves are formed. The cavity between the two planes is analogous to a stretched string held at the points x = 0 and x = L. Here, the distance 'L' between the two planes must be an integer multiple of half of the wavelength. The wavelengths that satisfy this condition are given by:

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Related Experiment Video

Updated: Jun 5, 2026

An Analog Macroscopic Technique for Studying Molecular Hydrodynamic Processes in Dense Gases and Liquids
11:03

An Analog Macroscopic Technique for Studying Molecular Hydrodynamic Processes in Dense Gases and Liquids

Published on: December 4, 2017

Simple waves in relativistic fluids.

Maxim Lyutikov1

  • 1Department of Physics, Purdue University, 525 Northwestern Avenue, West Lafayette, Indiana 47907-2036, USA.

Physical Review. E, Statistical, Nonlinear, and Soft Matter Physics
|January 15, 2011
PubMed
Summary

This study presents exact analytical solutions for the Riemann problem in magnetized plasmas, simplifying the understanding of relativistic fluid flows and plasma expansion into vacuum.

Area of Science:

  • Relativistic fluid dynamics
  • Plasma physics
  • Magnetohydrodynamics

Background:

  • The Riemann problem is crucial for understanding wave propagation in fluid dynamics.
  • Relativistic flows of polytropic fluids present complex behaviors, especially under magnetic field influence.
  • Magnetized plasmas exhibit unique properties influencing their dynamic evolution.

Purpose of the Study:

  • To analyze the Riemann problem for relativistic flows of polytropic fluids.
  • To derive exact analytical solutions for magnetized plasma expansion into vacuum.
  • To investigate the behavior of magnetized plasma under various boundary conditions and dimensionalities.

Main Methods:

  • Applying the Riemann problem framework to relativistic polytropic fluid dynamics.

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Microparticle Manipulation by Standing Surface Acoustic Waves with Dual-frequency Excitations
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Microparticle Manipulation by Standing Surface Acoustic Waves with Dual-frequency Excitations

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Last Updated: Jun 5, 2026

An Analog Macroscopic Technique for Studying Molecular Hydrodynamic Processes in Dense Gases and Liquids
11:03

An Analog Macroscopic Technique for Studying Molecular Hydrodynamic Processes in Dense Gases and Liquids

Published on: December 4, 2017

Measurements of Waves in a Wind-wave Tank Under Steady and Time-varying Wind Forcing
08:54

Measurements of Waves in a Wind-wave Tank Under Steady and Time-varying Wind Forcing

Published on: February 13, 2018

Microparticle Manipulation by Standing Surface Acoustic Waves with Dual-frequency Excitations
06:51

Microparticle Manipulation by Standing Surface Acoustic Waves with Dual-frequency Excitations

Published on: August 21, 2018

  • Deriving explicit analytical solutions for one-dimensional plasma expansion.
  • Analyzing self-similar structures in three-dimensional magnetized outflows.
  • Investigating wave reflection phenomena in magnetized plasmas.
  • Main Results:

    • Found simplified evolution of physical quantities for cold magnetized plasmas.
    • Obtained exact explicit analytical solutions for 1D magnetized plasma expansion into vacuum.
    • Analyzed plasma expansion into unmagnetized media and rarefaction wave reflection.
    • Determined self-similar structure of 3D magnetized outflows near the plasma-vacuum interface.

    Conclusions:

    • The study provides exact analytical solutions for key problems in magnetized relativistic plasma flows.
    • The findings simplify the understanding of plasma dynamics, particularly expansion into vacuum.
    • The derived solutions are applicable to various astrophysical and laboratory plasma scenarios.