Atmospheric Noise
Get Atmospheric Noise essential facts below. View Videos or join the Atmospheric Noise discussion. Add Atmospheric Noise to your topic list for future reference or share this resource on social media.
Atmospheric Noise
CCIR 322 atmospheric noise relationship. The standard has tables and maps that determine the noise figure at 1 MHz according to the season and the time of day. This graph converts that noise figure to other frequencies. Notice that the plotted lines are spaced in 10 dB increments at 1 MHz.

Atmospheric noise is radio noise caused by natural atmospheric processes, primarily lightning discharges in thunderstorms. On a worldwide scale, there are about 40 lightning flashes per second – ?3.5 million lightning discharges per day.[1]


Replica of Jansky's radio telescope, now at the National Radio Astronomy Observatory. 38°25?54?N 79°48?59?W / 38.431659°N 79.816253°W / 38.431659; -79.816253

In 1925, AT&T Bell Laboratories started investigating the sources of noise in its transatlantic radio telephone service.[2]

Karl Jansky, a 22-year-old researcher, undertook the task. By 1930, a radio antenna for a wavelength of 14.6 meters was constructed in Holmdel, NJ, to measure the noise in all directions. Jansky recognized three sources of radio noise.[3] The first (and strongest) source was local thunderstorms. The second source was weaker noise from more distant thunderstorms. The third source was a still weaker hiss that turned out to be galactic noise from the center of the Milky Way. Jansky's research made him the father of radio astronomy.[4]

In early 1950s, a mathematical model of the impact of lightning and thunderstorms on broadcasting was published by S. V. C. Aiya [5]


Atmospheric noise is radio noise caused by natural atmospheric processes, primarily lightning discharges in thunderstorms. It is mainly caused by cloud-to-ground flashes as the current is much stronger than that of cloud-to-cloud flashes.[] On a worldwide scale, 3.5 million lightning flashes occur daily. This are about 40 lightning flashes per second.[1]

The sum of all these lightning flashes results in atmospheric noise. It can be observed,[6] with a radio receiver, in the form of a combination of white noise (coming from distant thunderstorms) and impulse noise (coming from a near thunderstorm). The power-sum varies with seasons and nearness of thunderstorm centers.

Although lightning has a broad-spectrum emission, its noise power increases with decreasing frequency. Therefore, at very low frequency and low frequency, atmospheric noise often dominates, while at high frequency, man-made noise dominates in urban areas.


From 1960s to 1980s, a worldwide effort was made to measure the atmospheric noise and variations. Results have been documented in CCIR Report 322.[7][8] CCIR 322 provided seasonal world maps showing the expected values of the atmospheric noise figure Fa at 1 MHz during four hour blocks of the day. Another set of charts relates the Fa at 1 MHz to other frequencies. CCIR Report 322 has been superseded by ITU P.372[9] publication.

Random number generation

Atmospheric noise and variation is also used to generate high quality random numbers.[10] Random numbers have interesting applications in the security domain.[11]

See also


  1. ^ a b "Annual Lightning Flash Rate Map". Science On a Sphere. NOAA. Archived from the original on 24 March 2014. Retrieved 2014.
  2. ^ Singh 2005, pp. 402-408
  3. ^ Singh 2005, pp. 404-405
  4. ^ Singh 2005, p. 406
  5. ^ V, S. (December 1956). "Noise Radiation from Tropical Thunderstorms in the Standard Broadcast Band". Nature. pp. 1249-1249. doi:10.1038/1781249a0. Retrieved 2021.
  6. ^ Sample of atmospheric noise "Archived copy". Archived from the original on 2005-12-18. Retrieved .CS1 maint: archived copy as title (link)
  7. ^ International Radio Consultative Committee (1968), Characteristics and Applications of Atmospheric Radio Noise Data, Geneva: International Telecommunications Union, CCIR Report 322-3; first CCIR Report 322 was 1963; revised; second is ISBN 92-61-01741-X.
  8. ^ Lawrence, D. C. (June 1995), CCIR Report 322 Noise Variation Parameters, San Diego, CA: Naval Command, Control and Ocean Surveillance Center, RDT&E Division, NRaD Technical Document 2813, archived from the original on 2009-11-13; also DTIC Archived 2015-09-25 at the Wayback Machine
  9. ^ ITU, Recommendation P.372: Radio Noise
  10. ^ Haahr, Mads, Introduction to Randomness and Random Numbers,, retrieved 2011, self-published.
  11. ^


  This article uses material from the Wikipedia page available here. It is released under the Creative Commons Attribution-Share-Alike License 3.0.



Music Scenes