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Magnetism01:30

Magnetism

Magnets are commonly found in everyday objects, such as toys, hangers, elevators, doorbells, and computer devices. Experimentation on these magnets shows that all magnets have two poles: one is labeled north (N) and the other south (S). Magnetic poles repel if they are alike and attract if unlike. Moreover, both poles of a magnet attract unmagnetized pieces of iron.
An individual magnetic pole cannot be isolated. No matter how small, every piece of a magnet contains a north pole and a south...
Magnetic Fields01:27

Magnetic Fields

A moving charge or a current creates a magnetic field in the surrounding space, in addition to its electric field. The magnetic field exerts a force on any other moving charge or current that is present in the field. Like an electric field, the magnetic field is also a vector field. At any position, the direction of the magnetic field is defined as the direction in which the north pole of a compass needle points.
A magnetic field is defined by the force that a charged particle experiences...
Magnetic Field Lines01:19

Magnetic Field Lines

The representation of magnetic fields by magnetic field lines is very useful in visualizing the strength and direction of the magnetic field. Each of the magnetic field lines forms a closed loop. The field lines emerge from the north pole (N), loop around to the south pole (S), and continue through the bar magnet back to the north pole.
Magnetic field lines follow several hard-and-fast rules:
Energy In A Magnetic Field01:24

Energy In A Magnetic Field

If a magnetic field is sustained, there must be a current in a closed circuit or loop, implying some energy has been spent in creating the field. If this energy is not dissipated via the circuit's resistance, it is stored in the field.
Take an ideal inductor with zero resistance. Although it's practically impossible, assume that the coil's resistance is so small that it is practically negligible. The loss of the field's energy to dissipate thermal energy (or heat) is thus negligible.
The energy...
Magnetic Field due to Moving Charges01:23

Magnetic Field due to Moving Charges

A stationary charge creates and interacts with the electric field, while a moving charge creates a magnetic field.
Consider a point charge moving with a constant velocity. Like the electric field, the magnetic field at any point is directly proportional to the magnitude of the charge and inversely proportional to the square of the distance between the source point and the field point. However, unlike the electric field, the magnetic field is always perpendicular to the plane containing the line...
Magnetic Flux01:18

Magnetic Flux

The magnetic flux measures the number of magnetic field lines passing through a given surface area. The SI unit for magnetic flux is the weber (Wb). Magnetic flux is a scalar quantity. It depends on three factors: the strength of the magnetic field B, the area through which the field lines pass, and the relative orientation of the field with the surface area.
Suppose a surface is divided into elements of area dA. For each element, the component of the magnetic field that is normal to the...

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A 100 KW Class Applied-field Magnetoplasmadynamic Thruster
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A 100 KW Class Applied-field Magnetoplasmadynamic Thruster

Published on: December 22, 2018

Los campos magnéticos en Neptuno.

N F Ness, M H Acuña, L F Burlaga

    Science (New York, N.Y.)
    |December 15, 1989
    PubMed
    Resumen
    Este resumen es generado por máquina.

    La Voyager 2 detectó el planeta Neptuno.

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    Área de la Ciencia:

    • Ciencias planetarias Ciencias planetarias.
    • La magnetohidrodinámica es una dinámica magnético-hidrodinámica.
    • La astrofísica es la astrofísica.

    Sus antecedentes:

    • El campo magnético intrínseco y la magnetosfera de Neptuno no se habían caracterizado previamente.
    • La comprensión de los campos magnéticos planetarios es crucial para el estudio del clima espacial y la evolución planetaria.

    Objetivo del estudio:

    • Para caracterizar el campo magnético intrínseco y la magnetosfera de Neptuno.
    • Para analizar la interacción de la magnetosfera de Neptuno con el viento solar.

    Principales métodos:

    • Mediciones in situ realizadas por el experimento de campo magnético de la nave espacial Voyager 2.
    • Análisis de los datos del campo magnético para modelar la magnetosfera de Neptuno.

    Principales resultados:

    • Descubrimiento de un fuerte y complejo campo magnético intrínseco y magnetosfera.
    • Detección de un arco de choque separado a 34,9 radios de Neptuno (R(N)) y una magnetopausa a 26,5 R(N).
    • El campo magnético modelado como un dipolo inclinado offset (OTD) desplazado 0,55 R ((N) con una inclinación de 47 grados.

    Conclusiones:

    • El campo magnético de Neptuno está significativamente desplazado e inclinado, similar a Urano.
    • La estructura de la magnetosfera influye en las zonas aurorales y los cinturones de radiación.
    • Se necesita una investigación adicional para las fuentes de campo magnético localizadas dentro de 4 R (((N)).