'Cosmic ray muon data' presentation slideshows

Anisotropy of primary cosmic ray flux in Super-Kamiokande

Anisotropy of primary cosmic ray flux in Super-Kamiokande. Yuichi Oyama (KEK). Feb-26-2009. PNPI Winter school, Repino (Russia). New astronomy using underground cosmic-ray muons. G.Guillian et al., Physical Review D 75, 062003(2007). Y.Oyama, astro-ph/0605020.

313 views • 31 slides

Anisotropy of primary cosmic ray flux in Super-Kamiokande

Anisotropy of primary cosmic ray flux in Super-Kamiokande. Yuichi Oyama (KEK). for the Super-Kamiokande collaboration. Mar-6-2006 @ La Thuile 2006. New astronomy using underground cosmic-ray muons. (G.Guillian et al., submitted to PRD, astro-ph/0508468).

306 views • 30 slides

SVD software meeting summary Jan. 14 th , 2004

SVD software meeting summary Jan. 14 th , 2004. Data quality (Ishino) Alignment and IP resolution (Kibayashi) Gsim-svd status (T.Hara) Trak status (Karim) via e-mail Tag Vertex (T.Higuchi) Trigger simulator (K.Hara) MC generation (Shibata). Data quality (Ishino). Run 48. Run 90.

155 views • 6 slides

First MT Prototype Station

116 views • 1 slides