Publication Date:
2019-06-28
Description:
The energy spectra of high energy gamma-rays and hadrons were obtained by the emulsion chamber with 40 c.u. thickness at Mt. Fuji (3750 m). These results are compared with the Monte Carlo calculation based on the same model which is used in a family analysis. Our data are compatible with the model of heavy-enriched primary and scaling in the fragmentation region.
Keywords:
SPACE RADIATION
Type:
HE-3.1-3
,
19th Intern. Cosmic Ray Conf - Vol. 6; p 208-211; NASA-CP-2376-VOL-6
Format:
application/pdf