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Production mechanisms of cosmogenic nuclides in terrestrial rocks

THE FUNDAMENTALS OF SURFACE EXPOSURE DATING Production mechanisms of cosmogenic nuclides in terrestrial rocks [Pg.732]

Spallation. The cosmic ray energy spectrum below - 12 km altitude in the atmosphere is invariant despite the roughly exponential decrease of its flux (Lai and [Pg.732]

Target element Spallation Thermal neutron capture Negative muon capture [Pg.733]

2000) data for the noble gas isotopes are not eurrently available, but would look at least qualitatively similar. Depth is given in meters of water equivalent, where 1 m.w.e. eorresponds to a shielding depth of 100 gfcnP. [Used by permission of the editor of Nuel. Instr. and Meth. in Phys. Res. B, from Heisinger and Nolle (2000), Fig. l,p. 791.] [Pg.735]

No and N are the numbers of particles at the top of the atmosphere and at the location of the observer, respectively, d is the atmospheric depth (expressed in units of g/cm ), and A is the attenuation length or mean free path (in the same units). A is not a constant but changes with latitude, due to the modification of the cosmic ray energy spectrum depending on the cutoff rigidity, and is also slightly variable with altitude (e.g., Lai 1991). [Pg.736]


See other pages where Production mechanisms of cosmogenic nuclides in terrestrial rocks is mentioned: [Pg.749]    [Pg.756]   


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Cosmogenic

Cosmogenic nuclides

Nuclide

Nuclide production

Nuclides

Of nuclides

Product mechanical

Production/productivity terrestrial

Rock mechanics

Terrestrial

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