Propagation of ultra-high-energy cosmic ray nuclei in cosmic magnetic fields and implications for anisotropy measurements

Astroparticle Physics

Volumn 35, Issue 12, 2012, Pages 767-780

  Takami, Hajime ^a   Inoue, Susumu ^b   Yamamoto, Tokonatsu ^c  

^a MAX PLANCK INSTITUT FÜR PHYSIK   (Germany)

^b UNIVERSITY OF TOKYO   (Japan)

^c KONAN UNIVERSITY   (Japan)

Author keywords

Ultra high energy cosmic rays

Indexed keywords

ANGULAR SCALE; ANISOTROPY MEASUREMENTS; ARRIVAL DIRECTION; ASTROPHYSICAL SOURCES; CENTAURUS A; COSMIC MAGNETIC FIELDS; COSMIC-RAY NUCLEUS; CROSS CORRELATIONS; EXTRAGALACTIC MAGNETIC FIELDS; GALACTIC MAGNETIC FIELDS; HEAVY NUCLEUS; IRON NUCLEI; LARGE SCALE STRUCTURES; NUMBER DENSITY; PIERRE AUGER OBSERVATORY; POSITIONAL CORRELATION; SECONDARY PROTONS; SOURCE CORRELATION; SOURCE LOCATION; ULTRA HIGH-ENERGY COSMIC RAYS; ULTRA-HIGH ENERGIES;

ANISOTROPY; ASTROPHYSICS; COMPUTER SIMULATION; MAGNETIC FIELDS;

COSMIC RAYS;

EID: 84860855321     PISSN: 09276505     EISSN: None     Source Type: Journal    
DOI: 10.1016/j.astropartphys.2012.03.008     Document Type: Article

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