Studies of the fragmentation of various nuclei in CH2 and C targets were continued with the objective of obtaining cross sections in hydrogen for use in the cosmic ray propagation problem. New measurements include Fe-56. Measurements were made at 6 energies between 300 and 1700 MeV/nuc. C-12 measurements were made at six energies. Si-28 measurements were made at three energies and measurements were made at two energies. New data on C.-12 Si-28 and AR-44 nuclei are given. The data are compare it with the earlier semi-empirical predictions
Over the past few years, the HEAO-3 measurements of the abundances of ultra-heavy cosmic ray nuclei ...
Any study of the origin of the UH nuclei in the cosmic rays requires that their observed abundances ...
Models of cosmic-ray propagation in the Galaxy rely heavily on knowledge of the nuclear fragmentatio...
Measurements are reported of the yields of individual isotopes of Cr to Co(Z = 24 to 27) resulting f...
We compare experimentally measured yields of isotopes of elements from _(12)Mg to _(19)K resulting ...
We have measured the total charge changing cross sections as a function of energy for projectile _(3...
We have measured the total charge changing cross sections as a function of energy for projectile _(3...
The fragmentation of {sup 28}Si in targets of C, CH{sub 2}, Cu and Pb has been investigated at the L...
Radiation effects caused by single cosmic ray particles have been studied for many years in radiobio...
The fragmentation of a 225 MeV/n O-16 beam was investigated at the Bevalac. Preliminary cross sectio...
The objective of this project was to increase the fundamental knowledge about radiation effects of c...
Inclusive cross sections for high energy interactions at 0.9, 2.3, 3.6, and 13.5 GeV/nucleon of O-16...
We have measured the charge-changing cross sections of 10.6 GeV/nucleon ^(197)Au nuclei interacting ...
We have measured the charge-changing cross sections of 10.6 GeV/nucleon ^(197)Au nuclei interacting ...
In planning for long-duration spaceflight, it will beimportant to accurately model the exposure of a...
Over the past few years, the HEAO-3 measurements of the abundances of ultra-heavy cosmic ray nuclei ...
Any study of the origin of the UH nuclei in the cosmic rays requires that their observed abundances ...
Models of cosmic-ray propagation in the Galaxy rely heavily on knowledge of the nuclear fragmentatio...
Measurements are reported of the yields of individual isotopes of Cr to Co(Z = 24 to 27) resulting f...
We compare experimentally measured yields of isotopes of elements from _(12)Mg to _(19)K resulting ...
We have measured the total charge changing cross sections as a function of energy for projectile _(3...
We have measured the total charge changing cross sections as a function of energy for projectile _(3...
The fragmentation of {sup 28}Si in targets of C, CH{sub 2}, Cu and Pb has been investigated at the L...
Radiation effects caused by single cosmic ray particles have been studied for many years in radiobio...
The fragmentation of a 225 MeV/n O-16 beam was investigated at the Bevalac. Preliminary cross sectio...
The objective of this project was to increase the fundamental knowledge about radiation effects of c...
Inclusive cross sections for high energy interactions at 0.9, 2.3, 3.6, and 13.5 GeV/nucleon of O-16...
We have measured the charge-changing cross sections of 10.6 GeV/nucleon ^(197)Au nuclei interacting ...
We have measured the charge-changing cross sections of 10.6 GeV/nucleon ^(197)Au nuclei interacting ...
In planning for long-duration spaceflight, it will beimportant to accurately model the exposure of a...
Over the past few years, the HEAO-3 measurements of the abundances of ultra-heavy cosmic ray nuclei ...
Any study of the origin of the UH nuclei in the cosmic rays requires that their observed abundances ...
Models of cosmic-ray propagation in the Galaxy rely heavily on knowledge of the nuclear fragmentatio...