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Plasma Waves

Plasma Waves

Source: Department of Science and Technology

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Overview

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  1. News in Brief
  2. What is Plasma Waves?
  3. Martian Plasma Waves

Why in the News?  

Scientists have detected high-frequency plasma waves in the Martian Upper Atmosphere with novel narrowband and broadband features that can help understand plasma processes in the Martian plasma environment.

News in Brief

  • The researchers at the Indian Institute of Geomagnetism (IIG), an autonomous institute of the Department of Science and Technology have examined the existence of high-frequency plasma waves in the Martian plasma environment.
  • This is done using the high-resolution electric field data from the Mars Atmosphere and Volatile Evolution Mission (MAVEN) spacecraft of NASA.
  • These waves could be either electron oscillations that propagate parallel to the background magnetic field (Langmuir waves) or electron oscillations that propagate perpendicular to the background magnetic field (upper-hybrid type waves) in the magnetosheath region of Mars.
What is Plasma Waves?

  • Plasma waves are oscillations or fluctuations in the density and electric field of a plasma.
  • A plasma is a state of matter that exists when a gas is heated to high temperatures, causing its atoms to ionize and form charged particles, such as ions and electrons.
  • This results in a mixture of positively and negatively charged particles that can conduct electrical currents and respond to electric and magnetic fields.
  • Plasma waves play a crucial role in various astrophysical and laboratory plasma phenomena.

They can be classified into different types based on their characteristics and the physical mechanisms driving them. Some common types of plasma waves include:

  • Electrostatic Waves: These waves involve oscillations in the electric field of the plasma without any associated magnetic field variations. Examples include Langmuir waves, ion acoustic waves, and electron acoustic waves.
  • Electromagnetic Waves: These waves involve coupled oscillations in both the electric and magnetic fields. Common examples include whistler waves, upper hybrid waves, and lower hybrid waves.
  • Alfven Waves: Named after Hannes Alfvén, these are magnetohydrodynamic waves that propagate in magnetized plasmas. They involve oscillations in the magnetic field and are important in the context of space plasmas and astrophysical phenomena.
  • Ion Cyclotron Waves: These waves are associated with the gyration of ions in a magnetic field and are commonly observed in magnetized plasmas.
Applications
  • They have various applications and are important in understanding and studying phenomena such as the behaviour of the solar wind, magnetic confinement in fusion devices, astrophysical plasmas, and space weather.
  • They also play a role in communication systems and plasma-based technologies.
  • Studying and characterizing these waves are essential for gaining insights into the complex dynamics of plasmas in different environments.
Martian Plasma Waves

  • Two distinct wave modes with frequency below and above the electron plasma frequency in the Mars magnetosphere.
  • These waves are either broadband- or narrowband-type with distinguishable features in the frequency domain.
  • The broadband waves were consistently found to have periodic patchy structures with a periodicity of 8–14 milliseconds.
  • Observations of such waves provide a tool to explore how electrons gain or dissipate energy in the Martian plasma environment.
  • The physical mechanism responsible for the generation of broadband-type waves and its modulation remains unexplained and further investigation is required.

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