Download e-book for iPad: A thin cosmic rain : particles from outer space by Michael W. Friedlander

By Michael W. Friedlander

ISBN-10: 0674002881

ISBN-13: 9780674002883

Enigmatic for a few years, cosmic rays at the moment are recognized to be now not rays in any respect, yet debris, the nuclei of atoms, dropping rain regularly on this planet, the place they are often detected through the surroundings and occasionally even hundreds of thousands of toes underground. This booklet tells the long-running detective tale in the back of the invention and learn of cosmic rays, a narrative that stretches from the early days of subatomic particle physics within the Nineties to the frontiers of high-energy astrophysics today.

Writing for the beginner scientist and the informed normal reader, Michael Friedlander, a cosmic ray researcher, relates the background of cosmic ray technology from its unintentional discovery to its current prestige. He explains how cosmic rays are pointed out and the way their energies are measured, then surveys present wisdom and theories of skinny cosmic rain. the main thorough, up to date, and readable account of those interesting phenomena, his e-book makes us social gathering to the quest into the character, habit, and origins of cosmic rays—and into the assets in their huge, immense power, occasionally 1000s of hundreds of thousands instances more than the strength possible within the strongest earthbound particle accelerators. As this seek led unexpectedly to the invention of recent debris corresponding to the muon, pion, kaon, and hyperon, and because it unearths scenes of amazing violence within the cosmos and gives clues approximately black holes, supernovas, neutron stars, quasars, and neutrinos, we see in actual fact why cosmic rays stay important to an astonishingly assorted variety of analysis reports on scales infinitesimally small and large.

Attractively illustrated, engagingly written, this can be a interesting inside of examine a technology on the heart of our figuring out of our universe.

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Photograph courtesy of Washington University Archives, St. ) —43— t h e e a rt h ’ s m a g n e t i c i n f l u e n c e the polar regions there would be no restriction on the energies of the detectable primary particles. Overall, the number of particles detected should increase steadily as one moves away from the magnetic equator. The observations of Clay and Compton were thus nicely explained. The latitude effect showed clearly that primary CR particles had to be electrically charged, but that both positive and negative charges would show the same effect.

1. Some computed cosmic ray orbits, showing the effect of the Earth’s magnetic field on incoming charged particles. The complexity of each orbit depends sensitively on the particle’s charge, momentum, and direction of travel. Some particles may spiral around the Earth many times before descending to a low altitude. ) —40— t h e e a rt h ’ s m a g n e t i c i n f l u e n c e tion can keep the computing time (and cost) to a minimum while protecting against errors that could accumulate when a final result is based on millions of successive calculations.

A similar magnetic effect is employed in experiments designed for hydrogen fusion (thermonuclear) reactions: a carefully shaped magnetic “bottle” confines a hot ionized gas (a plasma) so it cannot touch (and vaporize) the walls of its containing vessel. Particles trapped in the Earth’s radiation belts can continue to bounce between hemispheres until some new influence intrudes. 1 Particle speeds expressed as fractions of the speed of light. 88 —51— t h e e a rt h ’ s m a g n e t i c i n f l u e n c e field is not perfectly regular, the drift motion is actually very complex, and some particles can transfer to different field lines that will guide them down into denser regions of the atmosphere, where they will be lost through collisions.

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A thin cosmic rain : particles from outer space by Michael W. Friedlander

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