A precise measurement of the proton flux in primary cosmic rays with rigidity (momentum/charge) from 1 GV to 1.8 TV is presented based on 300 million events. Knowledge of the rigidity dependence of the proton flux is important in understanding the origin, acceleration, and propagation of cosmic rays. We present the detailed variation with rigidity of the flux spectral index for the first time. The spectral index progressively hardens at high rigidities
Knowledge of the precise rigidity dependence of the helium flux is important in understanding the or...
The precise measurements of the proton and helium flux in primary cosmic rays based on on data colle...
A precision measurement of the nitrogen flux with rigidity (momentum per unit charge) from 2.2 GV to...
A precise measurement of the proton flux in primary cosmic rays with rigidity (momentum/charge) from...
A precise measurement of the proton flux in primary cosmic rays with rigidity (momentum/charge) from...
Knowledge of the precise rigidity dependence of the helium flux is important in understanding the or...
The precise measurements of the proton and helium flux in primary cosmic rays based on on data colle...
A precision measurement of the nitrogen flux with rigidity (momentum per unit charge) from 2.2 GV to...
A precise measurement of the proton flux in primary cosmic rays with rigidity (momentum/charge) from...
A precise measurement of the proton flux in primary cosmic rays with rigidity (momentum/charge) from...
Knowledge of the precise rigidity dependence of the helium flux is important in understanding the or...
The precise measurements of the proton and helium flux in primary cosmic rays based on on data colle...
A precision measurement of the nitrogen flux with rigidity (momentum per unit charge) from 2.2 GV to...