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  2. Wave - Wikipedia

    en.wikipedia.org/wiki/Wave

    Electromagnetic waves propagating in free space, for instance, are transverse; they can be polarized by the use of a polarizing filter. Longitudinal waves, such as sound waves, do not exhibit polarization. For these waves there is only one direction of oscillation, that is, along the direction of travel.

  3. Cosmic noise - Wikipedia

    en.wikipedia.org/wiki/Cosmic_noise

    Cosmic noise, also known as galactic radio noise, is a physical phenomenon derived from outside of the Earth's atmosphere.It is not actually sound, and it can be detected through a radio receiver, which is an electronic device that receives radio waves and converts the information given by them to an audible form.

  4. Ion acoustic wave - Wikipedia

    en.wikipedia.org/wiki/Ion_acoustic_wave

    In plasma physics, an ion acoustic wave is one type of longitudinal oscillation of the ions and electrons in a plasma, much like acoustic waves traveling in neutral gas. However, because the waves propagate through positively charged ions, ion acoustic waves can interact with their electromagnetic fields , as well as simple collisions.

  5. Astronomical radio source - Wikipedia

    en.wikipedia.org/wiki/Astronomical_radio_source

    An astronomical radio source is an object in outer space that emits strong radio waves. Radio emission comes from a wide variety of sources. Radio emission comes from a wide variety of sources. Such objects are among the most extreme and energetic physical processes in the universe .

  6. Interstellar medium - Wikipedia

    en.wikipedia.org/wiki/Interstellar_medium

    In the ISM this is further complicated by the magnetic field, which provides wave modes such as Alfvén waves which are often faster than pure sound waves: if turbulent speeds are supersonic but below the Alfvén wave speed, the behaviour is more like subsonic turbulence.

  7. Helioseismology - Wikipedia

    en.wikipedia.org/wiki/Helioseismology

    Pressure modes are in essence standing sound waves. The dominant restoring force is the pressure (rather than buoyancy), hence the name. All the solar oscillations that are used for inferences about the interior are p modes, with frequencies between about 1 and 5 millihertz and angular degrees ranging from zero (purely radial motion) to order .

  8. Wave interference - Wikipedia

    en.wikipedia.org/wiki/Wave_interference

    Interference of right traveling (green) and left traveling (blue) waves in Two-dimensional space, resulting in final (red) wave Interference of waves from two point sources. Cropped tomography scan animation of laser light interference passing through two pinholes (side edges).

  9. Standing wave - Wikipedia

    en.wikipedia.org/wiki/Standing_wave

    In physics, a standing wave, also known as a stationary wave, is a wave that oscillates in time but whose peak amplitude profile does not move in space. The peak amplitude of the wave oscillations at any point in space is constant with respect to time, and the oscillations at different points throughout the wave are in phase .