2.3.1 spase://CNES/Instrument/CDPP-AMDA/Voyager2/CRS CRS Cosmic Ray System 2009-05-20T21:10:14Z This investigation studied the origin and acceleration process, life history, and dynamic contribution of interstellar cosmic rays, the nucleosynthesis of elements in cosmic-ray sources, the behavior of cosmic rays in the interplanetary medium, and the trapped planetary energetic particle environment. The instrumentation included a High-Energy Telescope System (HETS) and a Low-Energy Telescope System (LETS). The HETS covered an energy range between 6 and 500 MeV/nucleon for nuclei ranging in atomic numbers from 1 through 30. In addition, electrons in the energy range between 3 and 100 MeV were measured by this telescope and an electron telescope. The LETS measured the energy and determined the identity of nuclei for energies between .15 and 30 MeV/nucleon and atomic numbers from 1 to 30. The instruments also measured the anisotropies of electrons and nuclei. In addition, electrons in the energy range between 3 and 100 MeV were measured by the electron telescope. spase://SMWG/Person/Edward.C.Stone.Jr PrincipalInvestigator NSSDC's Master Catalog http://nssdc.gsfc.nasa.gov/database/MasterCatalog?sc=1977-076A&ex=8 Information about the Cosmic Ray System (CRS) experiment on the Voyager 2 mission. EnergeticParticleInstrument Cosmic Ray System (CRS) on Voyager 2 spase://CNES/Observatory/CDPP-AMDA/Voyager2