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  2. 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 .

  3. Solar radio emission - Wikipedia

    en.wikipedia.org/wiki/Solar_radio_emission

    Solar radio emission refers to radio waves that are naturally produced by the Sun, primarily from the lower and upper layers of the atmosphere called the chromosphere and corona, respectively. The Sun produces radio emissions through four known mechanisms, each of which operates primarily by converting the energy of moving electrons into ...

  4. Atmospheric diffraction - Wikipedia

    en.wikipedia.org/wiki/Atmospheric_diffraction

    Radio wave diffraction is the scattering of radio frequency or lower frequencies from the Earth's ionosphere, resulting in the ability to achieve greater distance radio broadcasting. Sound wave diffraction is the bending of sound waves, as the sound travels around edges of geometric objects. This produces the effect of being able to hear even ...

  5. Why The World Seems To Fall Silent After A Fresh Snow - AOL

    www.aol.com/why-world-seems-fall-silent...

    Fresh snowflakes continue to dampen sound even once they reach the ground, turning the world into a sort of soundbooth with padding on every surface to prevent sound waves from bouncing around the ...

  6. Astronomical radio source - Wikipedia

    en.wikipedia.org/wiki/Astronomical_radio_source

    As Io moves through this torus, the interaction generates Alfvén waves that carry ionized matter into the polar regions of Jupiter. As a result, radio waves are generated through a cyclotron maser mechanism, and the energy is transmitted out along a cone-shaped surface. When Earth intersects this cone, the radio emissions from Jupiter can ...

  7. The Sun is really loud — but if we could hear it, what would ...

    www.aol.com/news/2018-02-26-the-sun-is-really...

    The Sun is said to be extremely noisy, but we can’t hear it since sound doesn’t travel through space. Scientists at the University of Sheffield decided to use vibrations within our star's ...

  8. Parabolic reflector - Wikipedia

    en.wikipedia.org/wiki/Parabolic_reflector

    An oblique projection of a focus-balanced parabolic reflector. It is sometimes useful if the centre of mass of a reflector dish coincides with its focus.This allows it to be easily turned so it can be aimed at a moving source of light, such as the Sun in the sky, while its focus, where the target is located, is stationary.

  9. Alfvén surface - Wikipedia

    en.wikipedia.org/wiki/Alfvén_surface

    Researchers were unsure exactly where the Alfvén critical surface of the Sun lay. Based on remote images of the corona, estimates had put it somewhere between 10 and 20 solar radii from the surface of the Sun. [5] On April 28, 2021, during its eighth flyby of the Sun, NASA's Parker Solar Probe (PSP) encountered the specific magnetic and particle conditions at 18.8 solar radii that indicated ...