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Antiprotons at Solar Maximum

New measurements with good statistics will make it possible to observe the time variation of cosmic antiprotons at 1 AU through the approaching peak of solar activity. We report a new computation of the interstellar antiproton spectrum expected from collisions between cosmic protons and the interste...

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Detalles Bibliográficos
Autores principales: Bieber, John W., Burger, R.A., Engel, Ralph, Gaisser, Thomas K., Roesler, Stefan, Stanev, Todor
Lenguaje:eng
Publicado: 1999
Materias:
Acceso en línea:https://dx.doi.org/10.1103/PhysRevLett.83.674
http://cds.cern.ch/record/381287