The direct observation of cosmic ray composition in JACEENo significant changes in spectral index for protons up to 500 TeV and higher intensity for helium above 2 TeV were observed. For heavier elements, a general tendency of intensity enhancement of medium heavies in the relative abundance above about 10 TeV/amu was observed.
Document ID
19900044807
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Burnett, T. H. (Washington, University Seattle, United States)
Dake, S. (Kobe University Japan)
Derrickson, J. H. (Washington Univ. Seattle, WA, United States)
Fountain, W. F. (NASA Marshall Space Flight Center Huntsville, AL, United States)
Fuki, M. (Matsusho Gakuen Junior College Matsumoto, Japan)