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What is Cosmic Rays

Handbook of Research on Global Environmental Changes and Human Health
High energy particles, generally originating outside the Solar System. They are mainly 89% of protons (nuclei of hydrogen), they also include nuclei of helium (10%) and heavier nuclei (1%). When they arrive at Earth, they collide with the nuclei of atoms in the upper atmosphere, creating more particles.
Published in Chapter:
Space Weather and Link to Climate Change
Hamid Nebdi (Chouaïb Doukkali University, Morocco)
DOI: 10.4018/978-1-5225-7775-1.ch001
Abstract
Our nearest shining star, the Sun, source of radiations and energy, sometimes generates severe events and phenomena in space which can affect our technology and biosphere. On the other hand, space weather, as defined by National Aeronautics and Space Administration (NASA), is conditions on the Sun and in the solar wind, magnetosphere, ionosphere, and thermosphere that can influence the performance and reliability of space-borne and ground-based technological systems and can endanger human life or health. A brief description of the Sun-Earth connection is firstly presented. Secondly, a particular attention is given to highlight the Sun's variability and the link between the space weather and climate change by means of some recent studies.
Full Text Chapter Download: US $37.50 Add to Cart
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Advances in Electromagnetic Environmental Shielding for Aeronautics and Space Applications
Protons and high-energy atomic nuclei, originating from the sun and other distant galaxies, which move through space at almost the speed of light and produce showers of secondary particles (ionized particles (protons, electrons, muons, antiprotons, alpha particles, pions, positrons) and electromagnetic radiation or X-rays) that reach the surfaces.
Full Text Chapter Download: US $37.50 Add to Cart
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