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Theory of Cosmic Ray Transport in the Heliosphere.

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Title: Theory of Cosmic Ray Transport in the Heliosphere.
Authors: Engelbrecht, N. Eugene1,2 (AUTHOR), Effenberger, F.3,4 (AUTHOR) fe@tp4.rub.de, Florinski, V.5 (AUTHOR), Potgieter, M. S.6 (AUTHOR), Ruffolo, D.7 (AUTHOR), Chhiber, R.8,9 (AUTHOR), Usmanov, A. V.8,9 (AUTHOR), Rankin, J. S.10 (AUTHOR), Els, P. L.1,2 (AUTHOR)
Source: Space Science Reviews. Jun2022, Vol. 218 Issue 4, p1-69. 69p.
Subjects: Galactic cosmic rays, Heliosphere, Magnetic fields, Cosmic rays
Abstract: Modelling the transport of cosmic rays (CRs) in the heliosphere represents a global challenge in the field of heliophysics, in that such a study, if it were to be performed from first principles, requires the careful modelling of both large scale heliospheric plasma quantities (such as the global structure of the heliosphere, or the heliospheric magnetic field) and small scale plasma quantities (such as various turbulence-related quantities). Here, recent advances in our understanding of the transport of galactic cosmic rays are reviewed, with an emphasis on new developments pertaining to their transport coefficients, with a special emphasis on novel theoretical and numerical simulation results, as well as the CR transport studies that employ them. Furthermore, brief reviews are given of recent progress in CR focused transport modelling, as well as the modelling of non-diffusive CR transport. [ABSTRACT FROM AUTHOR]
Copyright of Space Science Reviews is the property of Springer Nature and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract. (Copyright applies to all Abstracts.)
Database: Engineering Source
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  Data: Theory of Cosmic Ray Transport in the Heliosphere.
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  Data: <searchLink fieldCode="AR" term="%22Engelbrecht%2C+N%2E+Eugene%22">Engelbrecht, N. Eugene</searchLink><relatesTo>1,2</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Effenberger%2C+F%2E%22">Effenberger, F.</searchLink><relatesTo>3,4</relatesTo> (AUTHOR)<i> fe@tp4.rub.de</i><br /><searchLink fieldCode="AR" term="%22Florinski%2C+V%2E%22">Florinski, V.</searchLink><relatesTo>5</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Potgieter%2C+M%2E+S%2E%22">Potgieter, M. S.</searchLink><relatesTo>6</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Ruffolo%2C+D%2E%22">Ruffolo, D.</searchLink><relatesTo>7</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Chhiber%2C+R%2E%22">Chhiber, R.</searchLink><relatesTo>8,9</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Usmanov%2C+A%2E+V%2E%22">Usmanov, A. V.</searchLink><relatesTo>8,9</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Rankin%2C+J%2E+S%2E%22">Rankin, J. S.</searchLink><relatesTo>10</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Els%2C+P%2E+L%2E%22">Els, P. L.</searchLink><relatesTo>1,2</relatesTo> (AUTHOR)
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  Data: <searchLink fieldCode="JN" term="%22Space+Science+Reviews%22">Space Science Reviews</searchLink>. Jun2022, Vol. 218 Issue 4, p1-69. 69p.
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  Data: Modelling the transport of cosmic rays (CRs) in the heliosphere represents a global challenge in the field of heliophysics, in that such a study, if it were to be performed from first principles, requires the careful modelling of both large scale heliospheric plasma quantities (such as the global structure of the heliosphere, or the heliospheric magnetic field) and small scale plasma quantities (such as various turbulence-related quantities). Here, recent advances in our understanding of the transport of galactic cosmic rays are reviewed, with an emphasis on new developments pertaining to their transport coefficients, with a special emphasis on novel theoretical and numerical simulation results, as well as the CR transport studies that employ them. Furthermore, brief reviews are given of recent progress in CR focused transport modelling, as well as the modelling of non-diffusive CR transport. [ABSTRACT FROM AUTHOR]
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  Data: <i>Copyright of Space Science Reviews is the property of Springer Nature and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract.</i> (Copyright applies to all Abstracts.)
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      – SubjectFull: Heliosphere
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      – SubjectFull: Magnetic fields
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              Text: Jun2022
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