Home > Publications database > Temporal Structures in Positron Spectra and Charge-Sign Effects in Galactic Cosmic Rays > print

001     1037645
005     20250203124501.0
024 7 _ |a 10.1103/PhysRevLett.131.151002
|2 doi
024 7 _ |a 0031-9007
|2 ISSN
024 7 _ |a 1092-0145
|2 ISSN
024 7 _ |a 1079-7114
|2 ISSN
024 7 _ |a 10.34734/FZJ-2025-00810
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024 7 _ |a 37897756
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024 7 _ |a WOS:001102896300001
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037 _ _ |a FZJ-2025-00810
082 _ _ |a 530
100 1 _ |a Aguilar, M.
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245 _ _ |a Temporal Structures in Positron Spectra and Charge-Sign Effects in Galactic Cosmic Rays
260 _ _ |a College Park, Md.
|c 2023
|b APS
336 7 _ |a article
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336 7 _ |a Output Types/Journal article
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336 7 _ |a Journal Article
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|m journal
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|s 1737443674_5305
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336 7 _ |a ARTICLE
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336 7 _ |a JOURNAL_ARTICLE
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336 7 _ |a Journal Article
|0 0
|2 EndNote
520 _ _ |a We present the precision measurements of 11 years of daily cosmic positron fluxes in the rigidity range from 1.00 to 41.9 GV based on 3.4 ×106 positrons collected with the Alpha Magnetic Spectrometer (AMS) aboard the International Space Station. The positron fluxes show distinctly different time variations from the electron fluxes at short and long timescales. A hysteresis between the electron fluxes and the positron fluxes is observed with a significance greater than 5⁢𝜎 at rigidities below 8.5 GV. On the contrary, the positron fluxes and the proton fluxes show similar time variation. Remarkably, we found that positron fluxes are modulated more than proton fluxes with a significance greater than 5⁢𝜎 for rigidities below 7 GV. These continuous daily positron fluxes, together with AMS daily electron, proton, and helium fluxes over an 11-year solar cycle, provide unique input to the understanding of both the charge-sign and mass dependencies of cosmic rays in the heliosphere.
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588 _ _ |a Dataset connected to CrossRef, Journals: juser.fz-juelich.de
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