of hot plasma from the sun in all directions. It acts as a cushion that transmits the pressure from the flow of the solar wind and the barrier of the magnetic field from the object. Owing to this highly variable heating, however, a heavy atmospheric or ionospheric outflow of plasma flows during disturbed periods from the auroral zones into the magnetosphere, extending the region dominated by terrestrial material, known as the fourth or plasma geosphere, at times out to the. "NAI imaging: science background". 14 Other objects edit The magnetosphere of Jupiter is the largest planetary magnetosphere in the Solar System, extending up to 7,000,000 kilometers (4,300,000 mi) on the dayside and almost to the orbit of Saturn on the nightside. The tail region stretches well past 200 RE, and the way it ends is not well-known. The electric convection field causes charge separation at the magnetopause. These currents are the DP1 current (the auroral electrojet) and the polar DP2 current. Mercury, Earth, Jupiter, Ganymede, Saturn, Uranus, and Neptune, for example, exhibit intrinsic magnetospheres. In Bagenal,.; Dowling,.E.; McKinnon,.B.
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Because both sides of this convergence contain magnetized plasma, the interactions between them are complex. It contains two lobes, referred to as the northern and southern tail lobes. Nasa Space Plasma Physics Branch Pages. (A small counterclockwise ring current flows at the inner edge of the ring, caused by the fall-off in plasma density as Earth is approached.) The field confining the Earth's plasma and magnetic field inside the magnetospheric cavity. In the magnetosphere, a mix of free ions and electrons from both the solar wind and the Earth's ionosphere is confined by magnetic and electric forces that are much stronger than gravity and collisions. 1, the Earth's magnetosphere was first measured in 1958. Classification of magnetic fields Edit Schematic view of the different current systems which shape the Earth's magnetosphere Regardless of whether they are viewed as sources or consequences of the magnetospheric field structure, electric currents flow in closed circuits. In the direction perpendicular to the solar wind, the random motion of the solar-wind particles exerts a small pressure on the magnetic field, constricting the magnetosphere slightly. The term "magnetosphere" has also been used to describe regions dominated by the magnetic fields of celestial objects,.g.
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