Voyager Satellites Find Magnetic Bubbles at Edge of Solar System
on June 9, 2011
The sun's magnetic field spins opposite directions on the north and south poles. These oppositely pointing magnetic fields are separated by a layer of current called the heliospheric current sheet. Due to the tilt of the magnetic axis in relation to the axis of rotation of the Sun, the heliospheric current sheet flaps like a flag in the wind. The flapping current sheet separates regions of oppositely pointing magnetic field, called sectors. As the solar wind speed decreases past the termination shock, the sectors squeeze together, bringing regions of opposite magnetic field closer to each other. The Voyager spacecraft have now found that when the separation of sectors becomes very small, the sectored magnetic field breaks up into a sea of nested "magnetic bubbles" in a phenomenon called magnetic reconnection. The region of nested bubbles is carried by the solar wind to the north and south filling out the entire front region of the heliopause and the sector region in the heliosheath.
This discovery has prompted a complete revision of what the heliosheath region looks like. The smooth, streamlined look is gone, replaced with a bubbly, frothy outer layer.
For animations about the Voyager magnetic bubbles discovery, go here.
Artist's interpretation depicting the new view of the heliosphere. The heliosheath is filled with "magnetic bubbles" (shown in the red pattern) that fill out the region ahead of the heliopause. In this new view, the heliopause is not a continuous shield that separates the solar domain from the interstellar medium, but a porous membrane with fingers and indentations.
Artist's interpretation of the "standard" old view of the heliosphere: the magnetic field lines in the heliosheath connect back to the sun everywhere (some field lines are shown in red and blue). In this view, scientists expected the heliopause, the boundary that separates where the solar wind dominates from where the interstellar wind dominates, to be smooth and the associated smooth magnetic field to shield us from the interstellar medium and galactic cosmic rays.
Walt Feimer (HTSI): Lead Animator Michael Lentz (UMBC): Animator Chris Smith (HTSI): Animator Tom Bridgman (GST): Animator Scott Wiessinger (USRA): Video Editor Scott Wiessinger (USRA): Narrator Scott Wiessinger (USRA): Producer Merav Opher (Boston University): Scientist Scott Wiessinger (USRA): Writer Karen Fox (ASI): Writer
Please give credit for this item to: NASA/Goddard Space Flight Center/Conceptual Image Lab
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GCMD keywords can be found on the Internet with the following citation:
Olsen, L.M., G. Major, K. Shein, J. Scialdone, S. Ritz, T. Stevens, M. Morahan, A. Aleman, R. Vogel, S. Leicester, H. Weir, M. Meaux, S. Grebas, C.Solomon, M. Holland, T. Northcutt, R. A. Restrepo, R. Bilodeau, 2013. NASA/Global Change Master Directory (GCMD) Earth Science Keywords. Version 220.127.116.11.0