Cosmic rays consist of elementary particles with enormous energy
which originate from outside our solar system and constantly hit
the Earth's atmosphere. Where do these cosmic rays originate? How
does nature accelerate the cosmic-ray particles to energies with
orders of magnitude beyond the limits of manmade particle
accelerators? What can we learn by measuring the interactions of
the cosmic rays with the atmosphere? Digital radio-antenna arrays
offer a promising, complementary measurement method for high-energy
cosmic rays. This thesis reports on substantial advances in the
development of the radio technique, which will be used to address
these questions in future experiments.
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