IS THE MAGNETIC FIELD IN THE HELIOSHEATH LAMINAR OR A TURBULENT SEA OF BUBBLES?

IS THE MAGNETIC FIELD IN THE HELIOSHEATH LAMINAR OR A TURBULENT SEA OF BUBBLES?

All current global models of the heliosphere are based on the assumption that the magnetic field in the heliosheath, in the region close to the heliopause (HP), is laminar. We argue that in that region the heliospheric magnetic field is not laminar but instead consists of magnetic bubbles. We refer...

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Bibliographic Details
Main Authors: Opher, M. (Author), Drake, J. F. (Author), Swisdak, M. (Author), Schoeffler, K. M. (Author), Richardson, John D (Author), Decker, R. B. (Author), Toth, G. (Author), Richardson, John D. (Contributor)
Other Authors: MIT Kavli Institute for Astrophysics and Space Research (Contributor)
Format: Article
Language:English
Published: Institute of Physics/American Astronomical Society, 2015-02-27T14:38:40Z.
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