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  2. Magnetohydrodynamics - Wikipedia

    en.wikipedia.org/wiki/Magnetohydrodynamics

    Schematic view of the different current systems which shape the Earth's magnetosphere. In many MHD systems most of the electric current is compressed into thin nearly-two-dimensional ribbons termed current sheets. [10] These can divide the fluid into magnetic domains, inside of which the currents are relatively weak.

  3. Jupiter - Wikipedia

    en.wikipedia.org/wiki/Jupiter

    The temperature and pressure inside Jupiter increase steadily inward as the heat of planetary formation can only escape by convection. [55] At a surface depth where the atmospheric pressure level is 1 bar (0.10 MPa), the temperature is around 165 K (−108 °C; −163 °F). The region where supercritical hydrogen changes gradually from a ...

  4. Birkeland current - Wikipedia

    en.wikipedia.org/wiki/Birkeland_current

    A Birkeland current (also known as field-aligned current, FAC) is a set of electrical currents that flow along geomagnetic field lines connecting the Earth's magnetosphere to the Earth's high latitude ionosphere. In the Earth's magnetosphere, the currents are driven by the solar wind and interplanetary magnetic field (IMF) and by bulk motions ...

  5. Magnetosphere - Wikipedia

    en.wikipedia.org/wiki/Magnetosphere

    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. [17] Jupiter's magnetosphere is stronger than Earth's by an order of magnitude, and its magnetic moment is approximately 18,000 times ...

  6. Magnetosonic wave - Wikipedia

    en.wikipedia.org/wiki/Magnetosonic_wave

    Under the assumption that the background temperature is zero, it follows from the ideal gas law that the thermal pressure is also zero, p 0 = 0, and, as a result, that the sound speed vanishes, c s = 0. In this case, the slow mode disappears from the system, ω 2 sl = 0, and the fast mode propagates isotropically with the Alfvén speed, ω 2 f ...

  7. 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 ...

  8. Dynamo theory - Wikipedia

    en.wikipedia.org/wiki/Dynamo_theory

    Dynamo theory describes the process through which a rotating, convecting, and electrically conducting fluid acts to maintain a magnetic field. This theory is used to explain the presence of anomalously long-lived magnetic fields in astrophysical bodies. The conductive fluid in the geodynamo is liquid iron in the outer core, and in the solar ...

  9. Pressure system - Wikipedia

    en.wikipedia.org/wiki/Pressure_system

    A pressure system is a peak or lull in the sea level pressure distribution. The surface pressure at sea level varies minimally, with the lowest value measured 87 kilopascals (26 inHg) and the highest recorded 108.57 kilopascals (32.06 inHg). High- and low-pressure systems evolve due to interactions of temperature differentials in the atmosphere ...