We discuss the influence of large scale cosmic magnetic fields on the propagation of hadronic cosmic rays above 10 19 eV based on large scale structure simulations. Our simulations suggest that rather substantial deflection up to several tens of degrees at 10 20 eV are possible for nucleon primaries
β¦ LIBER β¦
A method of measuring cosmic magnetic fields with ultra high energy cosmic ray data
β Scribed by Martin Erdmann; Peter Schiffer
- Publisher
- Elsevier Science
- Year
- 2010
- Tongue
- English
- Weight
- 716 KB
- Volume
- 33
- Category
- Article
- ISSN
- 0927-6505
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