“…All-particle energy spectrum of cosmic rays, the flux is multiplied by E 3 . Results from direct measurements by Grigorov et al (Grigorov et al, 1999), JACEE (Asakimori et al, 1995), RUNJOB (Derbina et al, 2005), and SOKOL (Ivanenko et al, 1993) as well as from the air shower experiments AGASA (Takeda et al, 2003), Akeno 1 km 2 (Nagano et al, 1984a), and 20 km 2 (Nagano et al, 1984b), AUGER (Sommers et al, 2005), BASJE-MAS (Ogio et al, 2004), BLANCA (Fowler et al, 2001), CASA-MIA (Glasmacher et al, 1999b), DICE (Swordy and Kieda, 2000), EAS-TOP (Aglietta et al, 1999), Fly's Eye (Corbato et al, 1994), GRAPES-3 interpreted with two hadronic interaction models (Hayashi et al, 2005), Haverah Park (Lawrence et al, 1991) and (Ave et al, 2003), HEGRA (Arqueros et al, 2000), HiRes-MIA (Abu-Zayyad et al, 2001a), HiRes-I (Abbasi et al, 2004), HiRes-II (Abbasi et al, 2005), KASCADE electrons and muons interpreted with two hadronic interaction models , hadrons , and a neural network analysis combining different shower components (Antoni et al, 2002), KASCADE-Grande (preliminary) (Haungs et al, 2006b), MSU (Fomin et al, 1991), Mt. Norikura (Ito et al, 1997), SUGAR (Anchordoqui and Goldberg, 2004), Tibet ASγ (Amenomori et al, 2000a) and ASγ-III (Amenomori et al, 2003), Tunka-25 (Chernov et al, 2006), and Yakutsk (Glushkov et al, 2003).…”