Cosmic-ray spectrum and composition; direct observation

[1]  M. Simon,et al.  Propagation of Galactic Cosmic Rays under Diffusive Reacceleration , 1995 .

[2]  T. G. Guzik,et al.  The cosmic-ray He-3/He-4 ratio from 100 to 1600 MeV/amu , 1993 .

[3]  T. Gaisser,et al.  Cosmic-ray secondary antiprotons - A closer look , 1992 .

[4]  R. Silberberg,et al.  Spallation processes and nuclear interaction products of cosmic rays. , 1990, Physics reports.

[5]  Webber,et al.  Individual isotopic fragmentation cross sections of relativistic nuclei in hydrogen, helium, and carbon targets. , 1990, Physical review. C, Nuclear physics.

[6]  W. Webber,et al.  A new calculation of the cosmic-ray antiproton spectrum in the Galaxy and heliospheric modulation effects on this spectrum using a drift plus wavy current sheet model , 1989 .

[7]  Li,et al.  Hadronic interactions and primary-cosmic-ray composition at energies around 10(15)-10(16) eV derived from the analysis of high-energy gamma families. , 1988, Physical review. D, Particles and fields.

[8]  W. Binns.  Ultra heavy nuclei in the cosmic radiation , 1988 .

[9]  R. Golden,et al.  A reexamination of the cosmic-ray helium spectrum and the He-3/He-4 ratio at high energies , 1987 .

[10]  Y. Mizumoto,et al.  Energy spectrum of primary cosmic rays between 10$^{14.5}$ and 10$^{18}$ eV , 1984 .

[11]  R. Protheroe.  On the nature of the cosmic ray positron spectrum , 1981 .

[12]  C. Pennypacker,et al.  A Measurement of the Cosmic-Ray Antiproton Flux and a Search for Antihelium , 1981 .

[13]  R. R. Daniel,et al.  Evidence for the existence of cosmic-ray antiprotons , 1979 .

[14]  Peter Meyer,et al.  Charge Composition and Energy Spectra of Cosmic Ray Nuclei , 1974 .

[15]  B. Peters.  Origin of cosmic radiation , 1959 .