Relay-Version: version B 2.10 5/3/83; site utzoo.UUCP Path: utzoo!watmath!clyde!bonnie!akgua!whuxlm!whuxl!houxm!mtuxo!mtunh!mtung!mtunf!ariel!vax135!cornell!uw-beaver!tektronix!zehntel!hplabs!sri-unix!crummer@AEROSPACE.ARPA From: crummer@AEROSPACE.ARPA Newsgroups: net.physics Subject: Cosmic Rays and Background Radiation Message-ID: <281@sri-arpa.ARPA> Date: Mon, 17-Jun-85 20:49:58 EDT Article-I.D.: sri-arpa.281 Posted: Mon Jun 17 20:49:58 1985 Date-Received: Sun, 23-Jun-85 03:18:16 EDT Lines: 14 From: Charlie Crummer The 3 degree Kelvin background is universe-wide. Cosmic rays are charged particles or ions that get accelerated by some mysterious means or other (Maybe Uri Geller or something.). They have a spectrum of energies, of course, but some of them have truly large energies (like 10^20 Gev). Where a typical high energy event generated by an accelerator will have maybe 15 prongs, a typical cosmic ray may have over 100 daughter particles. --Charlie P.S. Cosmic rays are NOT the background radiation. --C