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  2. Magnetosphere - Wikipedia

    en.wikipedia.org/wiki/Magnetosphere

    A rendering of the magnetic field lines of the magnetosphere of the Earth. In astronomy and planetary science, a magnetosphere is a region of space surrounding an astronomical object in which charged particles are affected by that object's magnetic field. [1] [2] It is created by a celestial body with an active interior dynamo.

  3. Scientists uncover a magnetic misunderstanding about Uranus - AOL

    www.aol.com/news/scientists-uncover-magnetic...

    Science & Tech. Sports. Weather. 24/7 ... Uranus just a few days after the solar wind had squashed its magnetosphere - the planet's protective magnetic bubble - to about 20% of its usual volume ...

  4. Magnetosphere of Saturn - Wikipedia

    en.wikipedia.org/wiki/Magnetosphere_of_Saturn

    As with Earth's magnetosphere, the boundary separating the solar wind's plasma from that within Saturn's magnetosphere is called the magnetopause. [2] The magnetopause distance from the planet's center at the subsolar point [note 1] varies widely from 16 to 27 R s (R s =60,330 km is the equatorial radius of Saturn).

  5. Heliophysics - Wikipedia

    en.wikipedia.org/wiki/Heliophysics

    It is primarily concerned with the magnetosphere, ionosphere, thermosphere, mesosphere, and upper atmosphere of the Earth and other planets. Heliophysics combines the science of the Sun, corona, heliosphere and geospace, and encompasses a wide variety of astronomical phenomena, including "cosmic rays and particle acceleration, space weather and ...

  6. Magnetosphere of Jupiter - Wikipedia

    en.wikipedia.org/wiki/Magnetosphere_of_Jupiter

    The magnetosphere of Jupiter is the cavity created in the solar wind by Jupiter's magnetic field.Extending up to seven million kilometers in the Sun's direction and almost to the orbit of Saturn in the opposite direction, Jupiter's magnetosphere is the largest and most powerful of any planetary magnetosphere in the Solar System, and by volume the largest known continuous structure in the Solar ...

  7. Mercury's magnetic field - Wikipedia

    en.wikipedia.org/wiki/Mercury's_magnetic_field

    A dynamo is generated by a large iron core that has sunk to a planet's center of mass, has not cooled over the years, an outer core that has not been completely solidified, and circulates around the interior. Before the discovery of its magnetic field in 1974, it was thought that because of Mercury's small size, its core had cooled over the years.

  8. Van Allen radiation belt - Wikipedia

    en.wikipedia.org/wiki/Van_Allen_radiation_belt

    The Van Allen radiation belt is a zone of energetic charged particles, most of which originate from the solar wind, that are captured by and held around a planet by that planet's magnetosphere. Earth has two such belts, and sometimes others may be temporarily created.

  9. Dynamo theory - Wikipedia

    en.wikipedia.org/wiki/Dynamo_theory

    This means that dynamo theory was originally used to explain the Sun's magnetic field in its relationship with that of the Earth. However, this hypothesis, which was initially proposed by Joseph Larmor in 1919, has been modified due to extensive studies of magnetic secular variation , paleomagnetism (including polarity reversals ), seismology ...