| cosmic rays | has energy 2 GeV (average) |  |
| has composition 85% protons, 14% alpha-particles, 1% electrons, << 1% heavy nuclei |  |
| has synonym corpuscular radiation |  |
| has definition High-energy charged particles which stream at relativistic velocities down to Earth from space. The Sun ejects low-energy (107 - 1010 eV) cosmic rays during solar flares (those of lower energy than this are unobservable from Earth because of solar system magnetic fields). Those of intermediate energy (1010 - 1016 eV) have an isotropic distribution, and are apparently produced in the Galaxy. Possible sources of acceleration are shock waves accompanying supernovae (although cosmic rays have a higher hydrogen content than would be expected from a star that has processed material to iron), and the rotating magnetic fields of pulsars. The light elements Li, Be, and B have a higher abundance ratio in cosmic rays than in the solar system. |  |
| is a kind of radioactive particle |  |
| is a kind of charged particle |  |
| radioactive particle | has desintegration energy the total energy produced when the particle decays |  |
| has decay products the products produced immediately after decay |  |
| has lifetime The average time in which a particle decays |  |
| charged particle | is accelerated by electric or magnetic fields |  |
| has charge non-zero |  |
| particle | obeys uncertainty principle |  |
| has frequency inversely proportional to the wavelength |  |
| has wavelength inversely proportional to its momentum |  |
| has mass |  |
| physical object | has location or center of gravity |  |
| has angular momentum |  |
| has velocity |  |
| has momentum |  |
| has temperature |  |
| has volume |  |
| has extent |  |
| has material |  |