Observations of the Li, Be, and B isotopes and constraints on cosmic-ray propagation
- 1 January 2006
- journal article
- Published by Elsevier BV in Advances in Space Research
- Vol. 38 (7), 1558-1564
- https://doi.org/10.1016/j.asr.2006.09.008
Abstract
No abstract availableKeywords
This publication has 48 references indexed in Scilit:
- Theory of cosmic ray production in the supernova remnant RX J1713.7-3946Astronomy & Astrophysics, 2006
- A detailed spectral and morphological study of the gamma-ray supernova remnant RX J1713.7–3946 with HESSAstronomy & Astrophysics, 2006
- Detection of TeVγ-ray emission from the shell-type supernova remnant RX J0852.0-4622 with HESSAstronomy & Astrophysics, 2005
- Cosmic-ray Composition as Observed by UlyssesSpace Science Reviews, 2001
- On the low energy decrease in galactic cosmic ray secondary/primary ratiosAIP Conference Proceedings, 2000
- Galactic Cosmic-Ray Confinement Time: [ITAL]Ulysses[/ITAL] High Energy Telescope Measurements of the Secondary Radionuclide [TSUP]10[/TSUP]B[CLC]e[/CLC]The Astrophysical Journal, 1998
- The Elemental Composition of the Galactic Cosmic-Ray Source: ULYSSES High-Energy Telescope ResultsThe Astrophysical Journal, 1996
- A new measurement of the flux of the light cosmic-ray nuclei at high energiesThe Astrophysical Journal, 1994
- A measurement of cosmic-ray beryllium isotopes from 200 to 1500 MeV per nucleonThe Astrophysical Journal, 1978
- The mean mass of the abundant cosmic-ray nuclei from boron to silicon at 1.2 GeV per atomic mass unitThe Astrophysical Journal, 1978