cosmic rays | has energy 2 GeV (average) | ![has source: Hopkins, J. 1976 Glossary of Astronomy and Astrophysics, University of Chicago Press, 2001-09-27 09:28:02.0 has source: Hopkins, J. 1976 Glossary of Astronomy and Astrophysics, University of Chicago Press, 2001-09-27 09:28:02.0](facet.gif) |
has composition 85% protons, 14% alpha-particles, 1% electrons, << 1% heavy nuclei | ![has source: Hopkins, J. 1976 Glossary of Astronomy and Astrophysics, University of Chicago Press, 2001-09-27 09:28:02.0 has source: Hopkins, J. 1976 Glossary of Astronomy and Astrophysics, University of Chicago Press, 2001-09-27 09:28:02.0](facet.gif) |
has synonym corpuscular radiation | ![2001-09-27 09:28:02.0 2001-09-27 09:28:02.0](facet.gif) |
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. | ![has source: Hopkins, J. 1976 Glossary of Astronomy and Astrophysics, University of Chicago Press, 2001-09-27 09:28:02.0 has source: Hopkins, J. 1976 Glossary of Astronomy and Astrophysics, University of Chicago Press, 2001-09-27 09:28:02.0](facet.gif) |
is a kind of radioactive particle | ![2001-09-27 09:28:02.0 2001-09-27 09:28:02.0](facet.gif) |
is a kind of charged particle | ![2001-09-27 09:28:02.0 2001-09-27 09:28:02.0](facet.gif) |
radioactive particle | has desintegration energy the total energy produced when the particle decays | ![2001-09-27 09:28:02.0 2001-09-27 09:28:02.0](facet.gif) |
has decay products the products produced immediately after decay | ![2001-09-27 09:28:02.0 2001-09-27 09:28:02.0](facet.gif) |
has lifetime The average time in which a particle decays | ![2001-09-27 09:28:02.0 2001-09-27 09:28:02.0](facet.gif) |
charged particle | is accelerated by electric or magnetic fields | ![2001-09-27 09:28:02.0 2001-09-27 09:28:02.0](facet.gif) |
has charge non-zero | ![2001-09-27 09:28:02.0 2001-09-27 09:28:02.0](facet.gif) |
particle | obeys uncertainty principle | ![2001-09-27 09:28:02.0 2001-09-27 09:28:02.0](facet.gif) |
has frequency inversely proportional to the wavelength | ![2001-09-27 09:28:02.0 2001-09-27 09:28:02.0](facet.gif) |
has wavelength inversely proportional to its momentum | ![2001-09-27 09:28:02.0 2001-09-27 09:28:02.0](facet.gif) |
has mass | ![2001-09-27 09:28:02.0 2001-09-27 09:28:02.0](facet.gif) |
physical object | has location or center of gravity | ![2001-09-27 09:27:27.0 2001-09-27 09:27:27.0](facet.gif) |
has angular momentum | ![2001-09-27 09:27:27.0 2001-09-27 09:27:27.0](facet.gif) |
has velocity | ![2001-09-27 09:27:27.0 2001-09-27 09:27:27.0](facet.gif) |
has momentum | ![2001-09-27 09:27:27.0 2001-09-27 09:27:27.0](facet.gif) |
has temperature | ![2001-09-27 09:27:27.0 2001-09-27 09:27:27.0](facet.gif) |
has volume | ![2001-09-27 09:27:27.0 2001-09-27 09:27:27.0](facet.gif) |
has extent | ![2001-09-27 09:27:27.0 2001-09-27 09:27:27.0](facet.gif) |
has material | ![2001-09-27 09:27:27.0 2001-09-27 09:27:27.0](facet.gif) |