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The Implication of the Helium-to-proton Flux Ratio in Galactic Cosmic Rays
The measurement of daily proton and helium fluxes by AMS-02 shows that the helium-to-proton flux ratio (He/H) is negatively correlated with the solar activity at rigidity 1.7–7 GV. What is the behavior of He/H at rigidity lower than 1.7 GV? How can this phenomenon be described quantitatively and lin...
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Published in: | The Astrophysical journal 2023-12, Vol.959 (2), p.139 |
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Main Authors: | , |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites |
Online Access: | Get full text |
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Summary: | The measurement of daily proton and helium fluxes by AMS-02 shows that the helium-to-proton flux ratio (He/H) is negatively correlated with the solar activity at rigidity 1.7–7 GV. What is the behavior of He/H at rigidity lower than 1.7 GV? How can this phenomenon be described quantitatively and linked to the underlying mechanisms? In this work, based on a theoretical derivation, we find that the slope (
S
) of
ln
(
He
/
H
)
versus ln(H) is a good indicator of the variation of He/H.
S
> 0 means the variation of He/H is anticorrelated with the solar activity, and vice versa. Furthermore, the value of
S
is quantitatively related to the difference in protons and helium nuclei in the local interstellar spectrum (LIS) and in solar modulation. A 3D time-dependent numerical model is used to reproduce the observed proton and helium data. The results of the simulation show that, with increasing rigidity, the parameter
S
increases from negative values to positive values at around 1 GV, reaches a maximum value at around 2 GV, and then decreases until it approaches 0. Interestingly,
S
is equal to 0 at around 1 GV. This means that He/H at this rigidity is almost unchanged with the variation in solar activity. Finally, the expression for
S
is validated by changing the LIS used in the numerical procedure. This shows that the overall profile of
S
as a function of rigidity is mainly determined by the mass-to-charge ratio, and the specific value of
S
is strongly affected by the difference in the LIS between protons and helium nuclei. |
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ISSN: | 0004-637X 1538-4357 |
DOI: | 10.3847/1538-4357/ad0b09 |