Abstract:Neue Messungen der Plasmaeigenschaften in der Umgebung von Voyager 1 belegen, dass die Raumsonde die Heliosphäre verlassen und den interstellaren Raum erreicht hat. Insbesondere Messungen der Ionendichten, Elektronenplasma‐Schwingungen und Magnetfelder entsprechen den Vorhersagen für den Übergang in das interstellare Medium.
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