Solar modulation of cosmic electrons - Evidence for dynamic regulation

Tuska, E.; Evenson, P. A.; Meyer, P.

doi:10.1086/186043

Cited by 19 publications

(6 citation statements)

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“…cycles [64,65]. Charge-sign-dependent solar modulation has also been clearly seen in the antiproton-to-proton flux ratio measured before and after the most recent (2000) reversal of the solar magnetic field by a series of flights of the BESS balloon-borne experiment [32].…”

Section: Theoretical Interpretationsmentioning

confidence: 99%

PAMELA and indirect dark matter searches

et al. 2009

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Abstract. We present a review of the experimental results obtained by PAMELA in measuring the ( p,p) and e ± abundance in cosmic rays. In this context, we discuss the interpretation of the observed anomalous positron excess in terms of the annihilation of dark matter particles as well as in terms of standard astrophysical sources. Moreover we show the constraints on dark matter models fromp data.

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Section: Theoretical Interpretationsmentioning

confidence: 99%

PAMELA and indirect dark matter searches

et al. 2009

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“…The study of solar modulation is very complex, and ideally involves long-term (extending over much of the solar cycle) measurements of all charged components of the cosmic radiation. It is probable that the modulation effect depends on the particle charge-sign and solar magnetic field polarity (Potgieter and Burger 1990, Tuska et al 1991). Although the Sun has a complex magnetic field, the dipole term nearly always dominates in determining the magnetic field of the solar wind.…”

Section: Solar Modulationmentioning

confidence: 99%

Precise measurements of the cosmic ray antiproton spectrum with BESS including the effects of solar modulation

Mitchell

Abe

Anraku

et al. 2005

Advances in Space Research

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“…The study of solar modulation is very complex, and ideally involves long-term (extending over much of the solar cycle) measurements of all charged components of the cosmic radiation. It is probable that the modulation effect depends on the particle chargesign and solar magnetic field polarity [49,50]. Although the Sun has a complex magnetic field, the dipole term nearly always dominates in determining the magnetic field of the solar wind.…”

Section: Solar Modulationmentioning

confidence: 99%