Abstract
This chapter presents a variety of more or less stand-alone topics that are closely linked to some specific aspects of cosmic ray physics. Some of the topics cannot be found easily in readily available cosmic ray literature because they may belong primarily to other disciplines of science. The chapter discusses cosmogenic nuclides in the atmosphere and in rocks. The bulk of the galactic cosmic radiation that is responsible for the production of cosmogenic nuclides, that is, the relatively intense but low energy component with energies <10 GeV/nucleon, is subject to solar modulation effects.
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