u‰‰ŽาFŽฤ“c@“O ŽiยŽRŠw‰@‘ๅŠw—HŠw•”j “๚ŽžF‚P‚OŒŽ@‚P‚T“๚i‹เj@Œ฿Œใ‚SŽž‚R‚O•ช‚ฉ‚็ ๊ŠF ยŽRŠw‰@‘ๅŠw@—HŠw•”i‘Š–อŒดƒLƒƒƒ“ƒpƒXj‚k“‚UŠK@‚k‚U‚O‚RŽบ ‘่–ฺF uCosmic-rays as Particle Physics and Astrophysicsv —vŽ|F It has been about a century since V. Hess discovered the cosmic-ray (CR) in 1912. First I overview the history of CRs from the view point of particle physics, focusing upon the Brazil-Japan (B-J) Emulsion Chamber Collaboration in connection with the accelerator physics. The B-J collaboration started from a letter of Prof. Yukawa to Prof. Lattes in 1959, proposing a joint experiment of CRs at Mt. Chacaltaya, who, needless to say, predicted a new particle, gmesonh, in 1935, and discovered it in 1947 respectively. In my talk, I survey the contributions of the B-J emulsion chamber experiments to the particle physics, what are successful and/or unsuccessful, while of rather my personal summary with a biased view. Second I present the CR physics from the view point of astrophysics, focusing my interest on the CR acceleration and the propagation in the Galaxy, in connection with several anomalies recently observed in CRs such as the excess of electron-positron. After viewing briefly the energy budget of CRs in the Galaxy, I present the development of the CR acceleration and the propagation, based on RUNJOB data (RUssia-Nippon JOint Balloon program) together with those obtained most recently by satellite (FERMI) as well as balloons (ATIC, CREAM, TRACER), and finally summarize what are open questions in CR physics reserved for future studies in both theory and experiment. ---------------------------------