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Evidence for changing of cosmic ray composition between 10(17) and 10(18) eV from multicomponent measurements

Abu-Zayyad T; Belov K; Bird DJ; Boyer J; Cao Z; Catanese M; Chen GF; Clay RW; Covault CE; Cronin JW; Dai HY; Dawson BR; Elbert JW; Fick BE; Fortson LF; Fowler JW; Gibbs KG; Glasmacher MA; Green KD; Ho Y; Huang A; Jui CC; Kidd MJ; Kieda DB; Knapp BC; Ko S.

Phys Rev Lett ; 84(19): 4276-9, 2000 May 08.

Artículo en Inglés | MEDLINE | ID: mdl-10990665

RESUMEN

The average mass composition of cosmic rays with primary energies between 10(17) and 10(18) eV has been studied using a hybrid detector consisting of the High Resolution Fly's Eye (HiRes) prototype and the MIA muon array. Measurements have been made of the change in the depth of shower maximum and the muon density as a function of energy. The results show that the composition is changing from a heavy to lighter mix as the energy increases.

Evidence for correlated changes in the spectrum and composition of cosmic rays at extremely high energies.

Bird DJ; Corbató SC; Dai HY; Dawson BR; Elbert JW; Gaisser TK; Green KD; Huang MA; Kieda DB; Ko S; Larsen CG; Loh EC; Luo M; Salamon MH; Smith D; Sokolsky P; Sommers P; Stanev T; Tang JK; Thomas SB; Tilav S.

Phys Rev Lett ; 71(21): 3401-3404, 1993 Nov 22.

Artículo en Inglés | MEDLINE | ID: mdl-10054968

Cosmic-ray composition around 10(1)8 eV.

Gaisser TK; Stanev T; Tilav S; Corbato SC; Dai HY; Dawson BR; Elbert JW; Emerson B; Kieda DB; Luo M; Ko S; Larsen C; Loh EC; Salamon MH; Smith JD; Sokolsky P; Sommers P; Tang J; Thomas SB; Bird DJ.

Phys Rev D Part Fields ; 47(5): 1919-1932, 1993 Mar 01.

Artículo en Inglés | MEDLINE | ID: mdl-10015774

RESUMEN

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