Oscillations in the open solar magnetic flux with a period of 1.68 years: imprint on galactic cosmic rays and implications for heliospheric shielding

An understanding of how the heliosphere modulates galactic cosmic ray (GCR) fluxes and spectra is important, not only for studies of their origin, acceleration and propagation in our galaxy, but also for predicting their effects (on technology and on the Earth's environment and organisms) and f...

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Main Authors: A. Rouillard, M. Lockwood
Format: Article
Language:English
Published: Copernicus Publications 2004-12-01
Series:Annales Geophysicae
Online Access:https://www.ann-geophys.net/22/4381/2004/angeo-22-4381-2004.pdf
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author A. Rouillard
M. Lockwood
M. Lockwood
author_facet A. Rouillard
M. Lockwood
M. Lockwood
author_sort A. Rouillard
collection DOAJ
description An understanding of how the heliosphere modulates galactic cosmic ray (GCR) fluxes and spectra is important, not only for studies of their origin, acceleration and propagation in our galaxy, but also for predicting their effects (on technology and on the Earth's environment and organisms) and for interpreting abundances of cosmogenic isotopes in meteorites and terrestrial reservoirs. In contrast to the early interplanetary measurements, there is growing evidence for a dominant role in GCR shielding of the total open magnetic flux, which emerges from the solar atmosphere and enters the heliosphere. In this paper, we relate a strong 1.68-year oscillation in GCR fluxes to a corresponding oscillation in the open solar magnetic flux and infer cosmic-ray propagation paths confirming the predictions of theories in which drift is important in modulating the cosmic ray flux.<br><br> <b>Key words.</b> Interplanetary physics (Cosmic rays, Interplanetary magnetic fields)
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spelling doaj.art-0d9cb480410c49139d2ba37509e580542022-12-21T17:32:49ZengCopernicus PublicationsAnnales Geophysicae0992-76891432-05762004-12-01224381439510.5194/angeo-22-4381-2004Oscillations in the open solar magnetic flux with a period of 1.68 years: imprint on galactic cosmic rays and implications for heliospheric shieldingA. Rouillard0M. Lockwood1M. Lockwood2Department of Physics and Astronomy, University of Southampton, Southampton, SO17 1BJ, UKRutherford Appleton Laboratory, Chilton, OX11 0QX, UKDepartment of Physics and Astronomy, University of Southampton, Southampton, SO17 1BJ, UKAn understanding of how the heliosphere modulates galactic cosmic ray (GCR) fluxes and spectra is important, not only for studies of their origin, acceleration and propagation in our galaxy, but also for predicting their effects (on technology and on the Earth's environment and organisms) and for interpreting abundances of cosmogenic isotopes in meteorites and terrestrial reservoirs. In contrast to the early interplanetary measurements, there is growing evidence for a dominant role in GCR shielding of the total open magnetic flux, which emerges from the solar atmosphere and enters the heliosphere. In this paper, we relate a strong 1.68-year oscillation in GCR fluxes to a corresponding oscillation in the open solar magnetic flux and infer cosmic-ray propagation paths confirming the predictions of theories in which drift is important in modulating the cosmic ray flux.<br><br> <b>Key words.</b> Interplanetary physics (Cosmic rays, Interplanetary magnetic fields)https://www.ann-geophys.net/22/4381/2004/angeo-22-4381-2004.pdf
spellingShingle A. Rouillard
M. Lockwood
M. Lockwood
Oscillations in the open solar magnetic flux with a period of 1.68 years: imprint on galactic cosmic rays and implications for heliospheric shielding
Annales Geophysicae
title Oscillations in the open solar magnetic flux with a period of 1.68 years: imprint on galactic cosmic rays and implications for heliospheric shielding
title_full Oscillations in the open solar magnetic flux with a period of 1.68 years: imprint on galactic cosmic rays and implications for heliospheric shielding
title_fullStr Oscillations in the open solar magnetic flux with a period of 1.68 years: imprint on galactic cosmic rays and implications for heliospheric shielding
title_full_unstemmed Oscillations in the open solar magnetic flux with a period of 1.68 years: imprint on galactic cosmic rays and implications for heliospheric shielding
title_short Oscillations in the open solar magnetic flux with a period of 1.68 years: imprint on galactic cosmic rays and implications for heliospheric shielding
title_sort oscillations in the open solar magnetic flux with a period of 1 68 years imprint on galactic cosmic rays and implications for heliospheric shielding
url https://www.ann-geophys.net/22/4381/2004/angeo-22-4381-2004.pdf
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