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Cosmic rays beyond the boundary of the heliosphere

Florinski, V. and Stone, E. C. and Cummings, A. C. and le Roux, J. A. (2015) Cosmic rays beyond the boundary of the heliosphere. In: The 34th International Cosmic Ray Conference. Proceedings of Science. No.236. SISSA , Trieste, Italy, Art. No. 214. https://resolver.caltech.edu/CaltechAUTHORS:20180824-100033018

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Abstract

In August of 2012 the Voyager 1 space probe has left the solar-wind bubble of ionized gas we call the heliosphere and entered the denser and colder environment of the interstellar cloud surrounding the solar system. Energetic charged particles underwent dramatic changes past the heliopause: the heliospheric ions disappeared completely, while the galactic cosmic rays were for the first time measured in their unmodulated state. The interstellar medium turned out to be almost entirely devoid of turbulent magnetic fluctuations, therefore the transport of cosmic rays is governed by a large-scale geometry of the magnetic field. We discuss observations of heliospheric ions, including anomalous cosmic rays, near the heliopause transition, and propose interpretations of the measured intensities and pitch-angle distributions based on gradient drift in a weakly nonuniform magnetic field. The heliopause transition appears to be permeated by magnetic flux tubes connected to the interstellar space and facilitating particle escape. These flux tubes may be a product of interchange instability driven by a plasma pressure gradient across the heliopause. The curvature of magnetic field lines and the anti-sunward gradient in plasma kinetic pressure provide conditions favorable for an interchange. The two flux tube crossings by the spacecraft allowed an indirect measurement of the plasma radial velocity near the heliopause.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
https://doi.org/10.22323/1.236.0214DOIBook Section
ORCID:
AuthorORCID
Florinski, V.0000-0001-5485-2872
Stone, E. C.0000-0002-2010-5462
Cummings, A. C.0000-0002-3840-7696
Additional Information:Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-ShareAlike. This work was supported, in part, by NASA grant NNX12AH44G and by NSF grant AGS-0955700.
Funders:
Funding AgencyGrant Number
NASANNX12AH44G
NSFAGS-0955700
Series Name:Proceedings of Science
Issue or Number:236
Record Number:CaltechAUTHORS:20180824-100033018
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20180824-100033018
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:89133
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:27 Aug 2018 18:12
Last Modified:03 Oct 2019 20:13

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