H.-J. Lange

TL;DR: In this paper, a consistent database covering presently ca 550 nuclear reactions and containing nearly 15,000 individual cross sections of which about 10000 are reported here for the first time, providing a basis for model calculations of the production of cosmogenic nuclides in extraterrestrial matter by solar and galactic cosmic ray protons.

TL;DR: In this paper, the authors measured the depth and size dependence of cosmogenic nuclides in ordinary chondrites for preatmospheric radii between 8.5 cm and about 100 cm, and the observed depth profiles and the dependence of the center production rates on meteoroid size were well reproduced by model calculations based on Monte Carlo calculations of the intra and internuclear cascade of galactic protons in meteoritic matter and on experimental and theoretical excitation functions of the underlying nuclear reactions.

TL;DR: In this paper, a systematic investigation of proton-induced reactions for p energies between 800 and 2600 MeV, the target elements O, Mg, Al, Si, Ca, Ti, V, Mn, Fe, Co, Ni, Cu, Zr, Rh, Nb, Ba and Au were irradiated with 800 MeV protons at LAMPF/Los Alamos National Laboratory, and with 1200, 1600 and 2600 MEV at Laboratoire National Saturne/Saclay.

TL;DR: In a series of irradiation experiments at the cyclotron of the Svedberg Laboratory/University of Uppsala sixteen different target elements were investigated for proton energies up to 100 MeV in order to determine such thin-target excitation functions as mentioned in this paper.