A systematic comparison of two different models of cosmogenic nuclide production in meteorites

Details A systematic comparison of two different models of cosmogenic nuclide production in meteorites A systematic comparison of two different models of cosmogenic nuclide production in meteorites

Feb 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ncimc..13..139p&link_type=abstract

Nuovo Cimento C, Serie 1 (ISSN 0390-5551), vol. 13 C, Jan.-Feb. 1990, p. 139-145.

Astronomy and Astrophysics

Astronomy

Abundance, Cosmochemistry, Cosmology, Meteoritic Composition, Astronomical Models, Galactic Cosmic Rays, Mass Spectroscopy, Meteorites, Radioactive Age Determination

Scientific paper

A systematic comparison of a variable cosmogenic-production rate model (proposed in a previous paper) with the conventional constant-production rate model is carried out. Attention is focused on the time-integrated concentrations in meteorites. A graphical method for the estimate of the exposure and terrestrial ages is applied with reference to the ten pairs of the five long-lived cosmogenic nuclides Cl-36, Al-26, Be-10, Mn-53, and I-129 of interest in the accelerator mass spectrometry.

Affiliated with

Also associated with

No associations

Rating

A systematic comparison of two different models of cosmogenic nuclide production in meteorites 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 A systematic comparison of two different models of cosmogenic nuclide production in meteorites, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A systematic comparison of two different models of cosmogenic nuclide production in meteorites will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1843102