Relay-Version: version B 2.10 5/3/83; site utzoo.UUCP Posting-Version: version B 2.10.1 6/24/83; site utastro.UUCP Path: utzoo!watmath!clyde!burl!we13!ihnp4!harpo!seismo!ut-sally!utastro!ethan From: ethan@utastro.UUCP (Ethan Vishniac) Newsgroups: net.physics Subject: northern lights (Aurora Borealis) Message-ID: <200@utastro.UUCP> Date: Fri, 27-Apr-84 17:45:47 EDT Article-I.D.: utastro.200 Posted: Fri Apr 27 17:45:47 1984 Date-Received: Sun, 29-Apr-84 07:55:50 EDT Organization: UTexas Astronomy Dept., Austin, Texas Lines: 18 Fred (and any other interested people): A solar flare is an eruption in the upper layers of the sun's atmosphere. It involves a complicated, and not well understood, interaction between the charged particles ( mostly protons and electrons, although some heavier ions are present) and the sun's magnetic field. The end result is that large numbers of the charged particles are ejected from the sun at very large speeds. When they reach the Earth they can get trapped in our magnetic field. The interaction between these particles and our magnetic field produces radiation (i.e. photons) which we call the northern lights. N.B. photons are massless, uncharged particles which are the quanta of free electromagnetic radiation (light). "Give a roar for Nora Ethan Vishniac standing in the night {ut-sally,kpno,ut-ngp}utastro!ethan Who saw the great Aurora Astronomy Department Borealis burning bright" University of Texas -Pogo Austin, Texas 78712