Relative Composition and Energy Spectra of Light Nuclei in Cosmic Rays: Results from AMS-01
Measurement of the chemical and isotopic composition of cosmic rays is essential for the precise understanding of their propagation in the galaxy. While the model parameters are mainly determined using the B/C ratio, the study of extended sets of ratios can provide stronger constraints on the propag...
Main Authors: | , , , , , , , , , , , , , , , , , , , , , , |
---|---|
Other Authors: | |
Format: | Article |
Language: | en_US |
Published: |
IOP Publishing
2013
|
Online Access: | http://hdl.handle.net/1721.1/76316 https://orcid.org/0000-0002-4436-6077 https://orcid.org/0000-0001-7831-7460 https://orcid.org/0000-0002-0450-7007 https://orcid.org/0000-0002-5006-6847 https://orcid.org/0000-0003-3513-8408 https://orcid.org/0000-0002-8667-5660 https://orcid.org/0000-0002-0236-7274 https://orcid.org/0000-0002-7172-9021 |
Internet
http://hdl.handle.net/1721.1/76316https://orcid.org/0000-0002-4436-6077
https://orcid.org/0000-0001-7831-7460
https://orcid.org/0000-0002-0450-7007
https://orcid.org/0000-0002-5006-6847
https://orcid.org/0000-0003-3513-8408
https://orcid.org/0000-0002-8667-5660
https://orcid.org/0000-0002-0236-7274
https://orcid.org/0000-0002-7172-9021