High energy cosmic ray physics with the MACRO experiment at gran sasso
- Ambrosio M
- Antolini R
- Auriemma G
- Baker R
- Baldini A
- Barbarino GC
- Barish BC
- Battistoni G
- Bellotti R
- Bemporad C
- Bernardini P
- Bilokon H
- Bisi V
- Bloise C
- Bosio T
- Bower C
- Bussino S
- Cafagna F
- Calicchio M
- Campana D
- Carboni M
- Castellano M
- Cecchini S
- Cei F
- Chiarella V
- Corona A
- Coutu S
- DeCataldo G
- Dekhissi H
- DeMarzo C
- DeMitri I
- DeVincenzi M
- DiCredico A
- Erriquez O
- Fantini R
- Favuzzi C
- Forti C
- Fusco P
- Giacomelli G
- Giannini G
- Giglietto N
- Goretti M
- Grassi M
- Heinz R
- Hong JT
- Iarocci E
- Katsavounidis E
- Kearns E
- Kyriazopoulou S
- Lamanna E
- Lane C
- Levin DS
- Lipari P
- Longley NP
- Longo MJ
- Mancarella G
- Mandrioli G
- MargiottaNeri A
- Marini A
- Martello D
- MarzariChiesa A
- Mazziotta MN
- Michael DG
- Mikheyev S
- MIller L
- Monacelli P
- Montaruli T
- Monteno M
- Mufson S
- Musser J
- Nicolo D
- Nolty R
- Okada C
- Orth C
- Osteria G
- Palamara O
- Parlati S
- Patera V
- Patrizii L
- Pazzi R
- Peck CW
- Petrera S
- Pistilli P
- Popa V
- Raino A
- Reynoldson J
- Ronga F
- Rubizzo U
- Sanzgiri A
- Sartogo F
- Satriano C
- Satta L
- Scapparone E
- Scholberg K
- Sciubba A
- SerraLugaresi P
- Severi M
- Sitta M
- Spinelli P
- Spinetti M
- Spurio M
- Steinberg R
- Stone JL
- Sulak LR
- Surdo A
- Tarle G
- Togo V
- Valente V
- Walter CW
- Webb R
DOIAbstract
The multimuon data collected by the MACRO detector at Gran Sasso have been analyzed using a new method. The resulting all-particle spectrum is consistent with EAS measurements but higher and flatter than the one obtained from direct experiments
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