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- W2083172871 abstract "We present a possible explanation for the transient increase in the galactic cosmic ray flux observed by Voyager 1 (V1) beyond the heliopause, in 2013 March. We suggest that this disturbance may be caused by a propagating disturbance in the interstellar magnetic field, of heliospheric origin. A model in which a magnetic disturbance, propagating outward from the heliosphere into the very-local interstellar plasma, affects the galactic cosmic rays is presented. We also discuss the possibility that this event is related to the plasma-wave event observed some 25 days later by the PWS experiment on V1." @default.
- W2083172871 created "2016-06-24" @default.
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- W2083172871 date "2014-09-24" @default.
- W2083172871 modified "2023-09-25" @default.
- W2083172871 title "INTERPRETATION OF THE DISTURBANCE IN GALACTIC COSMIC RAYS OBSERVED ON <i>VOYAGER 1</i> BEYOND THE HELIOPAUSE" @default.
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- W2083172871 doi "https://doi.org/10.1088/2041-8205/794/1/l4" @default.
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