Precise measurements of predominantly secondary cosmic-ray Li, Be, and B together with current well-measured production cross-sections for these isotopes help to improve our understanding of galactic cosmic ray propagation models. The Cosmic Ray Isotope Spectrometer (CRIS) on ACE has been measuring isotopic composition of cosmic rays since 1997 with high statistical precision. We present the isotopic abundances from CRIS and discuss these observations in the context of cosmic-ray transport models and previous cosmic-ray measurements
The isotopes of lithium, beryllium, and boron (LiBeB) are known in nature to be produced primarily b...
The isotopes of lithium, beryllium, and boron (LiBeB) are known in nature to be produced primarily b...
The elemental abundances of galactic cosmic rays (GCR) observed near Earth provide information about...
Precise measurements of predominantly secondary cosmic-ray Li, Be, and B together with current well-...
The cosmic-ray isotopes of lithium, beryllium, and boron (LiBeB) are generally believed to originate...
The cosmic-ray isotopes of lithium, beryllium, and boron (LiBeB) are generally believed to originate...
Radioactive cosmic ray nuclei produced by nuclear interactions during cosmic ray propagation through...
Radioactive cosmic ray nuclei produced by nuclear interactions during cosmic ray propagation through...
The abundance of Li, Be, and B isotopes in galactic cosmic rays (GCRs) between E = 50 and 200 MeV/nu...
The abundance of Li, Be, and B isotopes in galactic cosmic rays (GCRs) between E = 50 and 200 MeV/nu...
The abundance of Li, Be, and B isotopes in galactic cosmic rays (GCRs) between E = 50 and 200 MeV/nu...
The elemental abundances of galactic cosmic rays (GCR) observed near Earth provide information about...
The abundance of Li, Be, and B isotopes in galactic cosmic rays (GCR) between E=50-200 MeV/nucleon h...
The elemental abundances of galactic cosmic rays (GCR) observed near Earth provide information about...
The isotopes of lithium, beryllium, and boron (LiBeB) are known in nature to be produced primarily b...
The isotopes of lithium, beryllium, and boron (LiBeB) are known in nature to be produced primarily b...
The isotopes of lithium, beryllium, and boron (LiBeB) are known in nature to be produced primarily b...
The elemental abundances of galactic cosmic rays (GCR) observed near Earth provide information about...
Precise measurements of predominantly secondary cosmic-ray Li, Be, and B together with current well-...
The cosmic-ray isotopes of lithium, beryllium, and boron (LiBeB) are generally believed to originate...
The cosmic-ray isotopes of lithium, beryllium, and boron (LiBeB) are generally believed to originate...
Radioactive cosmic ray nuclei produced by nuclear interactions during cosmic ray propagation through...
Radioactive cosmic ray nuclei produced by nuclear interactions during cosmic ray propagation through...
The abundance of Li, Be, and B isotopes in galactic cosmic rays (GCRs) between E = 50 and 200 MeV/nu...
The abundance of Li, Be, and B isotopes in galactic cosmic rays (GCRs) between E = 50 and 200 MeV/nu...
The abundance of Li, Be, and B isotopes in galactic cosmic rays (GCRs) between E = 50 and 200 MeV/nu...
The elemental abundances of galactic cosmic rays (GCR) observed near Earth provide information about...
The abundance of Li, Be, and B isotopes in galactic cosmic rays (GCR) between E=50-200 MeV/nucleon h...
The elemental abundances of galactic cosmic rays (GCR) observed near Earth provide information about...
The isotopes of lithium, beryllium, and boron (LiBeB) are known in nature to be produced primarily b...
The isotopes of lithium, beryllium, and boron (LiBeB) are known in nature to be produced primarily b...
The isotopes of lithium, beryllium, and boron (LiBeB) are known in nature to be produced primarily b...
The elemental abundances of galactic cosmic rays (GCR) observed near Earth provide information about...