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      Interstellar Now! Missions to Explore Nearby Interstellar Objects

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          The Solar Wind as a Turbulence Laboratory

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            Voyager 1 Observes Low-Energy Galactic Cosmic Rays in a Region Depleted of Heliospheric Ions

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              In situ observations of interstellar plasma with Voyager 1.

              Launched over 35 years ago, Voyagers 1 and 2 are on an epic journey outward from the Sun to reach the boundary between the solar plasma and the much cooler interstellar medium. The boundary, called the heliopause, is expected to be marked by a large increase in plasma density, from about 0.002 per cubic centimeter (cm(-3)) in the outer heliosphere, to about 0.1 cm(-3) in the interstellar medium. On 9 April 2013, the Voyager 1 plasma wave instrument began detecting locally generated electron plasma oscillations at a frequency of about 2.6 kilohertz. This oscillation frequency corresponds to an electron density of about 0.08 cm(-3), very close to the value expected in the interstellar medium. These and other observations provide strong evidence that Voyager 1 has crossed the heliopause into the nearby interstellar plasma.
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                Author and article information

                Journal
                Advances in Space Research
                Advances in Space Research
                Elsevier BV
                02731177
                July 2021
                July 2021
                Article
                10.1016/j.asr.2021.06.052
                562af5b3-396c-40b4-88f6-c6d3ccfb52be
                © 2021

                https://www.elsevier.com/tdm/userlicense/1.0/

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