Precision Measurement of the monthly cosmic Ray fluxes e−, e+, p, He) with the Alpha Magnetic Spectrometer on the ISS

The precision measurements of the monthly cosmic ray fluxes with Alpha Magnetic Spectrometer on the International Space Station are presented. Individual electron, positron, proton and helium spectra have been measured for each Bartel’s rotation period (27 days) in the time range from May 2011 to Ma...

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Main Author: Graziani Maura
Format: Article
Language:English
Published: EDP Sciences 2019-01-01
Series:EPJ Web of Conferences
Online Access:https://www.epj-conferences.org/articles/epjconf/pdf/2019/14/epjconf_ricap2019_01052.pdf
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spelling doaj-355750ad94c7451db828eb82573132a02021-08-02T06:20:53ZengEDP SciencesEPJ Web of Conferences2100-014X2019-01-012090105210.1051/epjconf/201920901052epjconf_ricap2019_01052Precision Measurement of the monthly cosmic Ray fluxes e−, e+, p, He) with the Alpha Magnetic Spectrometer on the ISSGraziani MauraThe precision measurements of the monthly cosmic ray fluxes with Alpha Magnetic Spectrometer on the International Space Station are presented. Individual electron, positron, proton and helium spectra have been measured for each Bartel’s rotation period (27 days) in the time range from May 2011 to May 2017. This period covers the ascending phase of solar cycle #24 together with the reversal of the Sun’s magnetic field polarity through the minimum. The fluxes reveal a characteristic time dependence below 20 GeV. The data show a strong charge-sign dependent effects corresponding to the the polarity reversal of the solar magnetic field.https://www.epj-conferences.org/articles/epjconf/pdf/2019/14/epjconf_ricap2019_01052.pdf
collection DOAJ
language English
format Article
sources DOAJ
author Graziani Maura
spellingShingle Graziani Maura
Precision Measurement of the monthly cosmic Ray fluxes e−, e+, p, He) with the Alpha Magnetic Spectrometer on the ISS
EPJ Web of Conferences
author_facet Graziani Maura
author_sort Graziani Maura
title Precision Measurement of the monthly cosmic Ray fluxes e−, e+, p, He) with the Alpha Magnetic Spectrometer on the ISS
title_short Precision Measurement of the monthly cosmic Ray fluxes e−, e+, p, He) with the Alpha Magnetic Spectrometer on the ISS
title_full Precision Measurement of the monthly cosmic Ray fluxes e−, e+, p, He) with the Alpha Magnetic Spectrometer on the ISS
title_fullStr Precision Measurement of the monthly cosmic Ray fluxes e−, e+, p, He) with the Alpha Magnetic Spectrometer on the ISS
title_full_unstemmed Precision Measurement of the monthly cosmic Ray fluxes e−, e+, p, He) with the Alpha Magnetic Spectrometer on the ISS
title_sort precision measurement of the monthly cosmic ray fluxes e−, e+, p, he) with the alpha magnetic spectrometer on the iss
publisher EDP Sciences
series EPJ Web of Conferences
issn 2100-014X
publishDate 2019-01-01
description The precision measurements of the monthly cosmic ray fluxes with Alpha Magnetic Spectrometer on the International Space Station are presented. Individual electron, positron, proton and helium spectra have been measured for each Bartel’s rotation period (27 days) in the time range from May 2011 to May 2017. This period covers the ascending phase of solar cycle #24 together with the reversal of the Sun’s magnetic field polarity through the minimum. The fluxes reveal a characteristic time dependence below 20 GeV. The data show a strong charge-sign dependent effects corresponding to the the polarity reversal of the solar magnetic field.
url https://www.epj-conferences.org/articles/epjconf/pdf/2019/14/epjconf_ricap2019_01052.pdf
work_keys_str_mv AT grazianimaura precisionmeasurementofthemonthlycosmicrayfluxeseephewiththealphamagneticspectrometerontheiss
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