Science Nuggets

New Take on A Magnetic Mystery

Heliosphere and LISM Interactions

(Turner et al., Astrophys. J., [2024]; DOI:10.3847/1538-4357/ad05d3)

Voyager 1 and 2 both crossed the heliopause from the solar wind into the very local interstellar medium (VLISM), but neither observed the expected rotation of the magnetic field when they crossed that boundary

New insights from NASA’s near-Earth Magnetospheric Multiscale (MMS) mission show that this mysterious magnetic field signature might be caused by merging of solar and VLISM magnetic field lines, a process known as magnetic reconnection. The reconnected VLISM field lines are twisted toward the solar wind field direction as observed

This solution indicates that the heliopause is a thick but porous boundary layer, not a thin surface, which has implications ranging from the shape of the heliosphere to particle acceleration and cosmic ray accessibility

This new perspective on the data suggests that Voyager 1 may not have transited into pure interstellar space and offers new insight on the nature of the heliosphere’s interaction with the LISM.

Helio-pause (the interface between the heliosphere and the interstellar medium [ISM]) show shown as a closed surface in yellow. The ISM magnetic field and the heliosphere magnetic field are also shown.

Mind the Gap

Discrepancy of Observed & Predicted ENA Intensity below the Solar Wind Energy

(Galli et al. ApJ, [2023];

An energetic neutral atom (ENA) is created when a fast ion exchanges its charge with a neutral atom. Measuring such ENAs allows scientists to study the utmost boundary regions of our sun’s astrosphere, called the heliosphere, from afar. ENAs provide the means to place the in-situ plasma measurements in a global context and image large parts of the sky simultaneously.

Plot of pick-up ion differential flux comparing the observed flux and the predicted flux. Plot shows a gap between the two where the prediction is much lower in a certain energy range.

Space scientists measure the number of ENAs coming from the heliosphere’s boundary using NASA spacecraft, such as the Interstellar Boundary Explorer (IBEX; SHIELD researchers use computer models to make predictions about these ENA measurements. A recent work analyzed the number of observed ENAs that are less energetic than the solar wind coming from all parts of the heliosphere’s boundary over the course of an 11-year solar cycle. This showed that there is a large gap between measurements and models for all sky directions. The predicted ENA intensity derived from the models is as much as 100 times less than seen in the observations. This drastic difference indicates that we do not fully understand the ENA observations below the solar wind energy and that our computer models need to be improved. SHIELD researchers will continue working on improving our understanding of the important processes in the heliosphere, our home in the interstellar environment.