The flux of galactic cosmic rays (GCR) in the solar system appears to change with time. Based on the abundances in iron meteorites of cosmogenic nuclides of different half lives, Lavielle et al. (1999) found that the GCR flux increased in recent times (<100 Ma) by about 38% compared to average flux in the past 150 Ma to 700 Ma ago. A promising technique for calibrating the GCR flux during the past ~50 Ma, based on the 129I and 129Xe pair of nuclides, was discussed earlier (Marti 1986; Murty and Marti 1987). The 129I-129Xen chronometer provides a shielding-independent system as long as the exposure geometry remained fixed. It is especially suitable for large iron meteorites (Te-rich troilite) because of the effects by the GCR secondary neutr...
Cosmogenic radionuclides 10Be(t½ = 1.50 Ma), 26 Al(t½ = 705 ka), and 36Cl(t½ = 301 ka), measured by ...
The galactic cosmic ray (GCR) flux is modulated by solar activity: 11 and 22 year cycles are well es...
The depth profiles of cosmic ray tracks and radiisotopes such as 53Mn, 26Al, 60Co etc measured in so...
We report data on neutron capture products of the secondary cosmic ray component, the inferred proto...
We measured the He, Ne, and Ar isotopic concentrations and the 10Be, 26Al, 36Cl, and 41Ca concentrat...
The Ninth Symposium on Polar Science/Ordinary sessions: [OA] Antarctic meteorites / Hayabusa, Tue. 4...
Cosmic-ray-produced (cosmogenic) nuclides were studied in fragments of the Brenham pallasite, a larg...
The ⁵³Mn-⁵³Cr short-lived radionuclide decay system is a powerful tool to investigate the timescales...
Concentrations of stable and radioactive nuclides produced by cosmic ray particles in meteorites all...
The origin of ¹⁸ºW excesses in iron meteorites has been a recently debated topic. Here, a suite of I...
Different fluxes and spectra of galactic cosmic rays (GCR) and solar cosmic rays result in a wide va...
72nd Annual Meeting of the Meteoritical Society, held July 13-18, 2009 in Nancy, France
International audienceIt is admitted that 129I (T1/2 = 17 Ma) existed at the moment of the Earth's f...
The long accepted conclusion that the galactic cosmic ray flux has been "fairly" constant over the p...
The study of the isotopic abundances of the rare gases helium, neon and argon in iron meteorites has...
Cosmogenic radionuclides 10Be(t½ = 1.50 Ma), 26 Al(t½ = 705 ka), and 36Cl(t½ = 301 ka), measured by ...
The galactic cosmic ray (GCR) flux is modulated by solar activity: 11 and 22 year cycles are well es...
The depth profiles of cosmic ray tracks and radiisotopes such as 53Mn, 26Al, 60Co etc measured in so...
We report data on neutron capture products of the secondary cosmic ray component, the inferred proto...
We measured the He, Ne, and Ar isotopic concentrations and the 10Be, 26Al, 36Cl, and 41Ca concentrat...
The Ninth Symposium on Polar Science/Ordinary sessions: [OA] Antarctic meteorites / Hayabusa, Tue. 4...
Cosmic-ray-produced (cosmogenic) nuclides were studied in fragments of the Brenham pallasite, a larg...
The ⁵³Mn-⁵³Cr short-lived radionuclide decay system is a powerful tool to investigate the timescales...
Concentrations of stable and radioactive nuclides produced by cosmic ray particles in meteorites all...
The origin of ¹⁸ºW excesses in iron meteorites has been a recently debated topic. Here, a suite of I...
Different fluxes and spectra of galactic cosmic rays (GCR) and solar cosmic rays result in a wide va...
72nd Annual Meeting of the Meteoritical Society, held July 13-18, 2009 in Nancy, France
International audienceIt is admitted that 129I (T1/2 = 17 Ma) existed at the moment of the Earth's f...
The long accepted conclusion that the galactic cosmic ray flux has been "fairly" constant over the p...
The study of the isotopic abundances of the rare gases helium, neon and argon in iron meteorites has...
Cosmogenic radionuclides 10Be(t½ = 1.50 Ma), 26 Al(t½ = 705 ka), and 36Cl(t½ = 301 ka), measured by ...
The galactic cosmic ray (GCR) flux is modulated by solar activity: 11 and 22 year cycles are well es...
The depth profiles of cosmic ray tracks and radiisotopes such as 53Mn, 26Al, 60Co etc measured in so...