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  2. Radio noise - Wikipedia

    en.wikipedia.org/wiki/Radio_noise

    Radio noise near in frequency to a received radio signal (in the receiver's passband) interferes (RFI) with the operation of the receiver's circuitry.The level of noise determines the maximum sensitivity and reception range of a radio receiver; if no noise were picked up with radio signals, even weak transmissions could be received at virtually any distance by making a radio receiver that had ...

  3. Extremely low frequency - Wikipedia

    en.wikipedia.org/wiki/Extremely_low_frequency

    The rise of the noise at low frequencies (left side) is radio noise caused by slow processes in the Earth's magnetosphere. Due to their extremely long wavelength, ELF waves can diffract around large obstacles, are not blocked by mountain ranges or the horizon, and can travel around the curvature of the Earth .

  4. Magnetosphere of Saturn - Wikipedia

    en.wikipedia.org/wiki/Magnetosphere_of_Saturn

    The spectrum of Saturn's radio emissions compared with spectra of four other magnetized planets. Saturn is the source of rather strong low frequency radio emissions called Saturn kilometric radiation (SKR). The frequency of SKR lies in the range 10–1300 kHz (wavelength of a few kilometers) with the maximum around 400 kHz. [7]

  5. Saturn's hexagon - Wikipedia

    en.wikipedia.org/wiki/Saturn's_hexagon

    Saturn's Hexagon Comes to Light, APOD January 22, 2012; In the Center of Saturn's North Polar Vortex, Astronomy Picture of the Day – December 4, 2012; Video of hexagon's rotation from NASA; NASA's Cassini Spacecraft Obtains Best Views of Saturn Hexagon (December 4, 2013) Animated vortex view (TPS) Hexagon image; Saturn's Hexagon Replicated In ...

  6. Cosmic noise - Wikipedia

    en.wikipedia.org/wiki/Cosmic_noise

    Cosmic noise, also known as galactic radio noise, is radio-frequency electromagnetic radiation from sources outside of the Earth's atmosphere. Its characteristics are comparable to those of thermal noise .

  7. Saturn Electrostatic Discharges - Wikipedia

    en.wikipedia.org/wiki/Saturn_Electrostatic...

    Saturn Electrostatic Discharges (also referred to as SEDs) are atmospheric lightning events in convective weather storms on Saturn that produce high frequency (HF) radio emissions (1–40 MHz). Terrestrial lighting events on Earth , in comparison, occur in the very low frequency (VLF) radio band, between 3 Hz and 30 kHz.

  8. Have Quick - Wikipedia

    en.wikipedia.org/wiki/HAVE_QUICK

    Have Quick (also HAVEQUICK, short HQ) is an ECM-resistant frequency-hopping system used to protect military aeronautical mobile (OR) radio traffic. Since the end of World War II , U.S. and Allied military aircraft have used AM radios in the NATO harmonised 225–400 MHz UHF band (part of NATO B band [ 1 ] ) for short range air-to-air and ground ...

  9. J1407b - Wikipedia

    en.wikipedia.org/wiki/J1407b

    J1407b's disk has a 4-million km (2.5-million mi)-wide gap between radii 0.396 to 0.421 AU (59.2 to 63.0 million km; 36.8 to 39.1 million mi), which is believed to have been created by a nearly-Earth-sized (<0.8 M 🜨) exomoon orbiting within that gap and clearing out material, in a similar fashion to the shepherd moons of Saturn's rings.