New research suggests that the sun's magnetic field controls the large-scale shape of the heliosphere much more than expected. The new model shows that the magnetic field squeezes the solar wind along the sun's north-south axis, producing two jets. These jets are then dragged downstream by the flow of the interstellar medium -- the gases and dust that lie between star systems.
from News -- ScienceDaily http://ift.tt/19DMI5s via Karis World
from News -- ScienceDaily http://ift.tt/19DMI5s via Karis World
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