The effects of variable terrestrial environments of the Sun during its galactic orbit are discussed. Emphasis is put on the energetic particle populations, like pick-up ions, anomalous and galactic cosmic rays. After putting the analysis briefly into the context of the ongoing debate regarding a cosmic ray-terrestrial climate link, we study the structure of the heliosphere in various interstellar environments, particularly in dense clouds of atomic hydrogen. We continue with a computation of the energy spectra of both anomalous and galactic cosmic rays for galactic regions located in clouds and/or in galactic spiral arms. In the light of these results we discuss the consequences for the terrestrial and planetary environments, as well as for small solar system bodies. © 2006 Springer. All Rights Reserved.
CITATION STYLE
Fahr, H. J., Fichtner, H., Scherer, K., & Stawicki, O. (2006). Variable terrestrial particle environments during the galactic orbit of the sun. In Solar Journey: The Significance of Our Galactic Environment for the Heliosphere and Earth (pp. 259–279). Springer Netherlands. https://doi.org/10.1007/1-4020-4557-3_9
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