It exhibits regions of compressed plasma(*) known as corotating interaction regions.
This region's current sheet can be modeled by the Ballerina model and is inclined relative to the radial direction by the Parker angle. It exhibits regions of compressed plasma(*) known as corotating interaction regions. It is believed to extend from it source for about 100 AU before ending in a termination shock, which should be seen by Voyagers I and II. For ten points, identify this bubble within the interstellar medium that arises from solar wind.
This region's current sheet can be modeled by the Ballerina model and is inclined relative to the radial direction by the Parker angle.
heliosphere