Earth's magnetotail is formed as the solar wind compresses the side of the magnetosphere facing the Sun and stretches the opposite, night side of the magnetosphere away from Earth into a tail. Our Sun emits a continuous outflowing stream of electrons and protons into the solar system, called the solar wind. The solar wind plasma which has charged particles embedded in the extended magnetic field of the Sun, moves at speeds of a few hundred km per second. Almost all of Earth's water is contained in its ocean, which covers 70. Field lines of the northern "tail lobe" connect to the vicinity of the northern magnetic pole, and are directed towards the earth, while those in. Explore the earth magnetic field shift, what drives geomagnetic changes, and how wandering poles, anomalies, and field weakening impact navigation, satellites, and modern technology.
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