Astronomy and Astrophysics – Astronomy
Scientific paper
Oct 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ncimc..10..505v&link_type=abstract
Nuovo Cimento C, Serie 1 (ISSN 0390-5551), vol. 10 C, Sept.-Oct. 1987, p. 505-515.
Astronomy and Astrophysics
Astronomy
1
Cosmology, Galactic Cosmic Rays, Nuclear Fusion, Solar System, Astronomical Models, Astronomical Spectroscopy, Beryllium, Meteoritic Composition, Oscillations, Temporal Distribution
Scientific paper
A variable-rate cosmogenic production model is proposed which takes account of the changes in Galactic cosmic-ray irradiation conditions arising from the vertical oscillation of the solar system about the Galactic plane. The model incorporates and substantiates several ideas and suggestions previously put forward in the literature. The time distribution of the Be-10 concentration predicted by the model appears to be consistent with the data of the deep-sea sediment core RC 12-65. A comparison of the present model with the conventional constant-production-rate model is carried out, especially with reference to time-integrated concentrations in meteorites.
Marzari Francesco
Sartori S. M.
Stievano B. M.
Tuniz C..
Vanzani V.
No associations
LandOfFree
Modulation of the cosmogenic nuclide production expected from the galactovertical motion of the solar system 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 Modulation of the cosmogenic nuclide production expected from the galactovertical motion of the solar system, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Modulation of the cosmogenic nuclide production expected from the galactovertical motion of the solar system will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1776404