cascade shower

From Glossary of Meteorology
Revision as of 08:55, 26 March 2024 by WikiTeq (talk | contribs) (Rewrite with Template:Term and clean up)
(diff) ← Older revision | Latest revision (diff) | Newer revision → (diff)

(Also air shower, cascade, extensive air shower, shower.) Multiple generations of secondary cosmic rays produced when primary cosmic rays interact with atoms in the upper atmosphere, yielding subatomic particles and gamma rays. The secondary cosmic rays in turn produce even more down through the atmosphere.
Billions of these particles travel downward at nearly the speed of light and at ground level may extend over several square kilometers (in which instance the shower may be termed an extensive air shower). The maximum flux of cosmic rays, both primary and secondary, is at an altitude of 20 km, and below this the absorption by the atmosphere reduces the flux, though the rays are still readily detectable at sea level. Intensity of cosmic ray showers has also been observed to vary with latitude, being more intense at the poles.
Friedlander, M. W. 1989. Cosmic Rays. pp. 13, 79.

Copyright 2024 American Meteorological Society (AMS). For permission to reuse any portion of this work, please contact permissions@ametsoc.org. Any use of material in this work that is determined to be “fair use” under Section 107 of the U.S. Copyright Act (17 U.S. Code § 107) or that satisfies the conditions specified in Section 108 of the U.S.Copyright Act (17 USC § 108) does not require AMS’s permission. Republication, systematic reproduction, posting in electronic form, such as on a website or in a searchable database, or other uses of this material, except as exempted by the above statement, require written permission or a license from AMS. Additional details are provided in the AMS Copyright Policy statement.