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
Inelastic collisions between the galactic cosmic rays (GCRs) and the interstellar medium (ISM) are r...
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...
Precise measurements of predominantly secondary cosmic-ray Li, Be, and B together with current well-...
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 cosmic-ray isotopes of lithium, beryllium, and boron (LiBeB) are generally believed to originate...
The abundance of Li, Be, and B isotopes in galactic cosmic rays (GCR) between E=50-200 MeV/nucleon h...
The cosmic-ray isotopes of lithium, beryllium, and boron (LiBeB) are generally believed to originate...
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 bulk of galactic Li, Be, and B (LiBeB) abundances is believed to be created during energetic ine...
Inelastic collisions between the galactic cosmic rays (GCRs) and the interstellar medium (ISM) are r...
Inelastic collisions between the galactic cosmic rays (GCRs) and the interstellar medium (ISM) are r...
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...
Precise measurements of predominantly secondary cosmic-ray Li, Be, and B together with current well-...
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 cosmic-ray isotopes of lithium, beryllium, and boron (LiBeB) are generally believed to originate...
The abundance of Li, Be, and B isotopes in galactic cosmic rays (GCR) between E=50-200 MeV/nucleon h...
The cosmic-ray isotopes of lithium, beryllium, and boron (LiBeB) are generally believed to originate...
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 bulk of galactic Li, Be, and B (LiBeB) abundances is believed to be created during energetic ine...
Inelastic collisions between the galactic cosmic rays (GCRs) and the interstellar medium (ISM) are r...
Inelastic collisions between the galactic cosmic rays (GCRs) and the interstellar medium (ISM) are r...
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...