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dc.contributor.authorStrauss, R.D.
dc.contributor.authorPotgieter, M.S.
dc.date.accessioned2016-02-15T07:21:04Z
dc.date.available2016-02-15T07:21:04Z
dc.date.issued2014
dc.identifier.citationStrauss, R.D. & Potgieter, M.S. 2014. Where does the heliospheric modulation of galactic cosmic rays start? Advances in space research, 53:1015-1023. [https://doi.org/10.1016/j.asr.2014.01.004]en_US
dc.identifier.issn0271-1177
dc.identifier.urihttp://hdl.handle.net/10394/16291
dc.identifier.urihttps://doi.org/10.1016/j.asr.2014.01.004
dc.description.abstractThe long outstanding question of where the heliospheric (solar) modulation of galactic cosmic rays actually begins, in terms of spatial position, as well as at what high kinetic energy, can now be answered. Both answers are possible by using the results of an advanced numerical model, together with appropriate observations. Voyager 1 has been exploring the outskirts of the heliosphere and is presently entering what can be called the very local interstellar medium. It has been generally expected, and accepted, that once the heliopause is crossed, the local interstellar spectrum (LIS) should be measured in situ by the Voyager spacecraft. However, we show that this may not be the case and that modulation effects on galactic cosmic rays can persist well beyond the heliopause. For example, proton observations at 100 MeV close to the heliopause can be lower by 25% to 40% than the LIS, depending on solar modulation conditions. It is also illustrated quantitatively that significant solar modulation diminishes above 50 GeV at Earth. It is found that cosmic ray observations above this energy contain less that 5% solar modulation effects and should therefore reflect the LIS for galactic cosmic rays. Input spectra, in other words the very LIS, for solar modulation models are now constrained by in situ observations and can therefore not any longer be treated arbitrarily. It is also possible for the first time to determine the lower limit of the very LIS from a few MeV/nuc to very high energies.en_US
dc.language.isoenen_US
dc.publisherElsevieren_US
dc.subjectCosmic raysen_US
dc.subjectsolar modulationen_US
dc.subjectheliopauseen_US
dc.subjectlocal interstellar spectraen_US
dc.subjectpositron excessen_US
dc.titleWhere does the heliospheric modulation of galactic cosmic rays start?en_US
dc.typeArticleen_US
dc.contributor.researchID13065440 - Strauss, Roelf Du Toit
dc.contributor.researchID10060014 - Potgieter, Marthinus Steenkamp


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