Интересы
Earth's magnetosphere formed by the impact of he solar wind on the Earth's magnetic field. It forms an obstacle to the solar wind, diverting it, at a distance of about 70, 000 km, forming a bow shock 12, 000 to 15, 000 further upstream. The width of the magnetosphere abreast of Earth, is typically 190, 000 km, and on the night side a long "magnetotail" of stretched field lines extends to great distances.
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Auroras are common near the Poles. They are occasionally seen in temperate latitudes, when a magnetic storm temporarily expands the auroral oval. Large magnetic storms are most common during the peak of the eleven-year sunspot cycle or during the three years after that peak.[citation needed] However, within the auroral zone the likelihood of an aurora occurring depends mostly on the slant of IMF lines (the slant is known as Bz), being greater with southward slants. Geomagnetic storms that ignite auroras a
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