PLASMA FLOWS IN THE HELIOSHEATH ALONG THE VOYAGER 1 AND 2 TRAJECTORIES DUE TO EFFECTS OF THE 11 YR SOLAR CYCLE

We investigate the role of the 11 yr solar cycle variations in the solar wind (SW) parameters on the flows in the heliosheath using a new three-dimensional time-dependent model of the interaction between the SW and the interstellar medium. For boundary conditions in the model we use realistic time a...

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Bibliographic Details
Main Authors: Provornikova, E. (Author), Opher, M. (Author), Izmodenov, V. V. (Author), Toth, G. (Author), Richardson, John D. (Contributor)
Other Authors: MIT Kavli Institute for Astrophysics and Space Research (Contributor)
Format: Article
Language:English
Published: IOP Publishing, 2015-01-22T16:53:33Z.
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