Other
Scientific paper
Aug 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....5..382r&link_type=abstract
In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 5 p 382-385 (SEE N85-34991 23-93)
Other
Cosmology, Energetic Particles, Galactic Radiation, Nuclides, Particle Flux Density, Primary Cosmic Rays, Heliosphere, Interplanetary Space, Radiant Flux Density, Solar Activity Effects, Solar Cosmic Rays, Solar Protons
Scientific paper
The production rates of cosmogenic nuclides were calculated for the primary protons in the galactic and solar cosmic rays. At 1 AU, the long-term average fluxes of solar protons usually produce many more atoms of cosmogenic nuclide than the primary protons in the galactic cosmic rays (GCR). Because the particle fluxes inside meteorites and other large objects in space include many secondary neutrons, the production rates and ratios inside large objects are often very different from those by just the primary GCR protons. It is possible to determine if a small object, was small in space or broken from a meteorite. Because heliospherical modulation and other interactions change the GCR particle spectrum, the production of cosmogenic nuclides by the GCR particles outside the heliosphere will be different from that by modulated GCR primaries.
No associations
LandOfFree
Cosmogenic-nuclide production by primary cosmic-ray protons does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Cosmogenic-nuclide production by primary cosmic-ray protons, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Cosmogenic-nuclide production by primary cosmic-ray protons will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-757087