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The dynamic heliosphere, solar activity, and cosmic rays

dc.contributor.authorPotgieter, Marius S.en_US
dc.contributor.researchID10060014 - Potgieter, Marthinus Steenkamp
dc.date.accessioned2012-02-29T09:51:58Z
dc.date.available2012-02-29T09:51:58Z
dc.date.issued2010en_US
dc.description.abstractThis brief review addresses the relation between solar activity, cosmic ray variations and the dynamics of the heliosphere. The global features of the heliosphere influence what happens inside its boundaries on a variety of time-scales. Galactic and anomalous cosmic rays are the messengers that convey vital information on global heliospheric changes in the manner that they respond to these changes. By observing cosmic rays over a large range of energies at Earth, and with various space detectors, a better understanding is gained about space weather and climate. The causes of the cosmic ray variability are reviewed, with emphasis on the 11-year and 22-year cycles, step modulation, charge-sign dependent modulation and particle drifts. Advances in this field are selectively discussed in the context of what still are some of the important uncertainties and outstanding issues
dc.identifier.citationPotgieter, M.S. 2010. The dynamic heliosphere, solar activity, and cosmic rays. Advances in space research, 46(4):402-412. [https://doi.org/10.1016/j.asr.2009.09.016]en_US
dc.identifier.issn0273-1177en_US
dc.identifier.urihttp://hdl.handle.net/10394/6130
dc.identifier.urihttps://doi.org/10.1016/j.asr.2009.09.016
dc.publisherElsevieren_US
dc.subjectHeliosphere
dc.subjectCosmic rays
dc.subjectSolar activity
dc.subjectLong-term modulation
dc.subjectSpace climate
dc.titleThe dynamic heliosphere, solar activity, and cosmic raysen_US

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