Cosmic Ray
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General Overview :: Cosmic Ray
Cosmic rays are energetic particles originating from Outer space that impinge on Earth's atmosphere. Almost 90 of all the incoming Cosmic ray particles are simple protons, with nearly 10 being Helium nuclei , and slightly under 1 are heavier elements, electrons , or GAMMA ray photons. The term ray is a misnomer, as cosmic particles arrive individually, not in the form of a ray or beam of particles. However, when they were first discovered, cosmic rays were thought to be rays. When their particle nature needs to be emphasized, "cosmic ray particle" is written. The variety of particle energies reflects the wide variety of sources. The origins of these particles range from energetic processes on the Sun all the way to as yet unknown events in the farthest reaches of the visible Universe. Cosmic rays can have energies of over 1020 ;eV, far higher than the 1012 to 1013 ;eV that man-made particle accelerators can produce. There has been interest in investigating cosmic rays of even greater energies. Cosmic rays may broadly be divided into two categories, primary and secondary. The cosmic rays that arise in extrasolar astrophysical sources are primary cosmic rays; these primary cosmic rays can interact with interstellar matter to create secondary cosmic rays. The Sun also emits low Energy cosmic rays associated with Solar flares. The exact composition of primary cosmic rays, outside the Earth's atmosphere, is dependent on which part of the Energy Spectrum is observed. However, in general, almost 90 of all the incoming cosmic rays are protons, about 9 are helium nuclei and nearly 1 are electrons. The ratio of hydrogen to helium nuclei is about the same as the primordial Elemental abundance ratio of these elements in the universe.
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