Abstract
A large part of this workshop has dealt with galactic and anomalous cosmic rays in the quiet heliosphere, which we have seen is dominated by quasi-steady, co-rotating structures, called co-rotating interaction regions (CIRs). There is a significant degree of consensus regarding the basic processes affecting cosmic rays during this time, and comparison with observations suggests that the theoretical models may be capturing much of the essential physics.
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© 1998 Springer Science+Business Media Dordrecht
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Jokipii, J.R., Wibberenz, G. (1998). Epilogue: Cosmic Rays in the Active Heliosphere. In: Fisk, L.A., Jokipii, J.R., Simnett, G.M., von Steiger, R., Wenzel, KP. (eds) Cosmic Rays in the Heliosphere. Space Sciences Series of ISSI, vol 3. Springer, Dordrecht. https://doi.org/10.1007/978-94-017-1189-0_21
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DOI: https://doi.org/10.1007/978-94-017-1189-0_21
Publisher Name: Springer, Dordrecht
Print ISBN: 978-90-481-5032-8
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