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Paper 1 to 4 of 4 |
1)
Method for calculating arrival distribution of ultra-high-energy
cosmic rays with modifications by the galactic magnetic field.
H. Yoshiguchi,
S. Nagataki,
K. Sato
(Tokyo U. & Kyoto U., FIHS & Tokyo U., RESCEU)
. 2004. 6pp.
Prepared for CRIS 2004: 5th Cosmic Ray International Seminar: GZK and
Surroundings, Catania, Italy, 31 May - 4 Jun 2004.
Published in Nucl.Phys.Proc.Suppl.136:250-255,2004. Also in
*Catania 2004, GZK and surroundings* 250-255
2)
Numerical study on the propagation of ultra-high-energy cosmic rays in
the galactic magnetic field.
H. Yoshiguchi,
S. Nagataki,
K. Sato
(Tokyo U. & Tokyo U., RESCEU)
. 2004. 8pp.
Published in Astrophys.J.607:840-847,2004.
3)
Small scale clustering in isotropic arrival distribution of ultra-high
energy cosmic rays.
H. Yoshiguchi,
S. Nagataki,
S. Tsubaki,
K. Sato
(Tokyo U. of Sci. & Tokyo U.)
. Jul 2003. 4pp.
Prepared for 28th International Cosmic Ray Conferences (ICRC 2003),
Tsukuba, Japan, 31 Jul - 7 Aug 2003.
Published in *Tsukuba 2003,
Cosmic ray* 659-662
4)
Propagation of ultra-high energy cosmic rays from sources in the
super-galactic plane.
H. Yoshiguchi
(Tokyo U.)
. Nov 2001.
Prepared for 5th RESCEU International Symposium on New Trends in
Theoretical and Observations Cosmology, Tokyo, Japan, 13-16 Nov 2001.
Published in
*Tokyo 2001, New trends in theoretical and observational cosmology* 385-386
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