Relay-Version: version B 2.10 5/3/83; site utzoo.UUCP Posting-Version: version B 2.10.2 9/18/84; site petrus.UUCP Path: utzoo!watmath!clyde!burl!ulysses!gamma!epsilon!zeta!sabre!bellcore!petrus!mwg From: mwg@petrus.UUCP Newsgroups: net.physics Subject: Re: Cosmic Rays vs Gamma Rays Message-ID: <376@petrus.UUCP> Date: Tue, 18-Jun-85 11:26:18 EDT Article-I.D.: petrus.376 Posted: Tue Jun 18 11:26:18 1985 Date-Received: Wed, 19-Jun-85 04:27:05 EDT References: <277@sri-arpa.ARPA> Organization: Bell Communications Research, Inc Lines: 32 ++ I've been reading a great book, written in 1958, which, among other things shows that the common modern usage of the term "cosmic ray" has been around for a little while: ...the physicists make use of the so-called cosmic radiation. The electromagnetic fields on the surface of stars extending over huge spaces are under certain circumstances able to accelerate charged atomic particles, electrons and nuclei. The nuclei, owing to their greater inertia, seem to have a better chance of remaining in the accelerating field for a long distance, and finally when they leave the surface of the star into empty space they have already traveled through potentials of several thousand million volts. There may be a further acceleration in the magnetic fields between the stars; in any case the nuclei seem to be kept within the space of the galaxy for a long time by varying magnetic fields, and finally they fill this space with what one calls cosmic radiation. This radiation reaches the earth from the outside and consists of nuclei of practically all kinds, hydrogen and helium and many heavier elements, HAVING ENERGIES FROM ROUGHLY A HUNDRED OR A THOUSAND MILLION ELECTRON VOLTS TO, AGAIN IN RARE CASES, A MILLION TIMES THIS AMOUNT. When the particles of this cosmic radiation penetrate into the atmosphere of the earth they hit the nitrogen atoms or oxygen atoms of the atmosphere or may hit any experimental equipment exposed to the radiation. - Werner Heisenberg Physics and Philosophy pp 158-159 (Just a short historical vignette) -Mark