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Date : 1989-05-05
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Cosmic ray Wikipedia ~ Cosmic rays are highenergy protons and atomic nuclei which move through space at nearly the speed of light They originate from the sun from outside of the solar system and from distant galaxies Upon impact with the Earths atmosphere cosmic rays can produce showers of secondary particles that sometimes reach the surface Data from the Fermi Space Telescope have been interpreted as evidence that a significant fraction of primary cosmic rays originate from the supernova explosions of stars
What Are Cosmic Rays Space ~ Cosmic rays are atom fragments that rain down on the Earth from outside of the solar system
Cosmic Rays Introduction NASA ~ Cosmic Rays Cosmic rays provide one of our few direct samples of matter from outside the solar system They are high energy particles that move through space at nearly the speed of light
NASAs Cosmicopia Cosmic Rays ~ Particles that bombard the Earth from anywhere beyond its atmosphere are known as cosmic rays Cosmic rays dont take pretty pictures but studying the quantity and type of these particles helps us to understand the acceleration processes involved and to measure the composition of the Sun as well as sources at the far distant reaches of the galaxy
Cosmic ray physics Britannica ~ Cosmic ray a highspeed particle—either an atomic nucleus or an electron—that travels through space Most of these particles come from sources within the Milky Way Galaxy and are known as galactic cosmic rays GCRs
Cosmic Rays Where Do They Come From ~ Cosmic rays are extremely highenergy charged particles usually protons that move at nearly the speed of light Some come from the Sun in the form of solar energetic particles while others are ejected from supernova explosions and other energetic events in interstellar and intergalactic space
What Are Cosmic Rays Telescope Array Project ~ Cosmic rays are energetic subatomic particles that arrive from outside the Earths atmosphere The lowest energy cosmic rays are produced by ordinary stars like the Sun
Cosmic rays particles from outer space CERN ~ The energies of the primary cosmic rays range from around 1 GeV – the energy of a relatively small particle accelerator – to as much as 10 8 TeV far higher than the beam energy of the Large Hadron rate at which these particles arrive at the top of the atmosphere falls off with increasing energy from about 10 000 per square metre per second at 1 GeV to less than one per
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