UHECRS, very high energy protons and charged nuclei, occasionally arrive on Earth, where they are
detected by cosmic ray detectors such as the Pierre Auger Observatory in Argentina.
Not exact matches
The renowned British physicist Paul Dirac first posited the existence of antimatter in 1928, and four years later researchers at Caltech
detected the first documented antiparticles — positrons produced
by the impact of
cosmic rays on the atmosphere.
Over time, it should
detect tens or hundreds of
cosmic rays from individual AGNs and their range of energies should clarify exactly how they were accelerated — a process thought to be controlled
by magnetic fields around the colossal black holes.
It does so
by detecting the gamma
rays those elements emit when they are bombarded
by high - energy charged particles from space called
cosmic rays.
By detecting the faint fluorescence and the particles that reach the ground, Auger should be able to pin down the energy and direction of the original
cosmic ray.
The EUSO telescope, which will be used to find debris, was originally planned to
detect ultraviolet light emitted from air showers produced
by ultra-high energy
cosmic rays entering the atmosphere at night.
The high - energy
cosmic neutrinos
detected by IceCube are believed to originate from
cosmic -
ray interactions with matter (proton - proton interactions); from
cosmic -
ray interactions with radiation (proton - photon interactions); or from the decay or destruction of heavy, invisible «dark matter.»
The idea is to
detect neutrinos produced
by interactions between
cosmic rays and Earth's atmosphere.
It covers an area of 3000 square kilometers with approximately 1600 surface detector stations which
detect cosmic ray shower particles directly, as well as four fluorescence detectors which overlook the atmosphere above the surface array and
detect fluorescence light emitted
by shower particles.
The Pierre Auger Observatory has
detected more muons from
cosmic -
ray showers than predicted
by the most up - to - date particle - physics models.
Such a telescope would use large arrays of ground - based telescopes to
detect blue flashes of Cerenkov radiation, which are caused
by very high energy gamma -
ray photons from
cosmic sources smashing into the atmosphere.
The array is slated to be so much larger than Auger South because the highest energy
cosmic rays are only
detected by Auger South twice a month.
During periods of heightened solar activity, fewer galactic
cosmic rays (GCRs) are
detected by earthbound neutron monitors.