Voyager observations in the distant heliosheath: An analogy with ISEE-3 observations in the deep geomagnetic tail

TL;DR

This paper draws an analogy between Voyager 1's observations in the distant heliosheath and ISEE-3's in the geomagnetic tail, suggesting similar magnetic and particle behaviors despite different environments.

Contribution

It proposes a novel analogy between heliosheath and geomagnetic tail regions, offering a new perspective on Voyager 1's observations and the structure of the heliopause.

Findings

Voyager 1's data resembles geomagnetic tail lobes observations.

Heliospheric field lines may be open to interstellar entry.

The heliopause might be beyond the 'heliocliff' region.

Abstract

We suggest an analogy between energetic particle and magnetic field observations made by the Voyager 1 spacecraft in the distant heliosheath at 122 AU in August 2012, and those made in the distant geomagnetic tail by the ISEE 3 spacecraft in 1982-1983, despite large differences in the time and distance scales. The analogy suggests that in August, 2012, Voyager 1 may not have moved from the anomalous cosmic ray (ACR)-dominated heliosheath into the interstellar medium but into a region equivalent to the "lobes" of the geomagnetic tail, composed of heliospheric field lines which have reconnected with the interstellar medium beyond the spacecraft and so are open to the entry of cosmic rays, while heliospheric particles (e.g., ACRs) are free to escape, and which maintain a ~Parker spiral configuration. The heliopause, analogous to the magnetopause forming the outer boundary of the lobes, may then lie beyond this so-called "heliocliff". Even if this analogy is incorrect, the remarkable similarities between the energetic particle and magnetic field observations in these very different regions are worth noting.