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Electric Field Lines01:25

Electric Field Lines

8.9K
The three-dimensional representation of the electric field of a positive point charge requires tracing the electric field vectors, whose lengths decrease as the square of their distance from the charge and which point away from the charge at each point. This vector field is no doubt challenging to visualize. The visualization of electric fields becomes quickly intractable as the number of charges increases.
The solution to this problem is to use electric field lines, which are not vectors but...
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Series R—L Circuit Transients01:22

Series R—L Circuit Transients

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In a series resistor-inductor (R-L) circuit, closing the switch at the start of the time period simulates a three-phase short circuit, a fault condition where all three phases of an unloaded synchronous machine are short-circuited. When there is no fault impedance and no initial current, the initial voltage is determined by the phase angle of the source voltage.
Using Kirchhoff's Voltage Law (KVL) to analyze this circuit helps determine the total asymmetrical fault current, which consists...
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Magnetic Field Lines01:19

Magnetic Field Lines

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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:
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Electric Field01:16

Electric Field

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Consider two point charges, each exerting Coulomb force on the other. It is possible to describe the Coulomb interaction via an intermediate step by defining a new physical quantity called the electric field.
In the new picture, imagine that the first charge sets up an electric field independent of all other charges in the universe. When another charge comes in its vicinity, the second charge experiences an electric force depending on the electric field at that point. The source charge does not...
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Electrostatic Boundary Conditions01:16

Electrostatic Boundary Conditions

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Consider an external electric field propagating through a homogeneous medium. When the electric field crosses the surface boundary of the medium, it undergoes a discontinuity. The electric field can be resolved into normal and tangential components. The amount by which the field changes at any boundary is given by the difference between the field components above and below the surface boundary.
The surface integral of an electric field is given by Gauss's law in integral form and is related to...
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Precipitation of Ions03:11

Precipitation of Ions

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Predicting Precipitation
The equation that describes the equilibrium between solid calcium carbonate and its solvated ions is:
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Video Experimental Relacionado

Updated: Dec 12, 2025

Method for Recording Broadband High Resolution Emission Spectra of Laboratory Lightning Arcs
07:51

Method for Recording Broadband High Resolution Emission Spectra of Laboratory Lightning Arcs

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Pequeños relámpagos de tormentas eléctricas poco profundas en Júpiter

Heidi N Becker1, James W Alexander2, Sushil K Atreya3

  • 1Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA. Heidi.N.Becker@jpl.nasa.gov.

Nature
|August 8, 2020
PubMed
Resumen
Este resumen es generado por máquina.

Júpiter también.

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Área de la Ciencia:

  • Ciencias planetarias
  • Ciencias atmosféricas
  • Física del plasma

Sus antecedentes:

  • Las anteriores observaciones de rayos de Júpiter estaban limitadas por la sensibilidad de la cámara y la distancia.
  • Las tasas de flash se estiman en 4 × 10-3 por km2 / año, con extensiones espaciales de ~ 30 km.
  • Los destellos se interpretan como trazadores de convección de humedad cerca del nivel de 5 bares.

Objetivo del estudio:

  • Para reportar nuevas observaciones ópticas del rayo de Júpiter por la nave espacial Juno.
  • Para caracterizar las energías, duraciones y velocidades de los relámpagos con un detalle sin precedentes.
  • Para investigar el origen atmosférico y los mecanismos de generación de los rayos de Júpiter.

Principales métodos:

  • Utilizó los instrumentos ópticos de la nave espacial Juno para la detección de rayos.
  • Energías de flash analizadas que oscilan entre 105 y 108 joules.
  • Las duradas de destellos medidos son tan cortas como 5,4 milisegundos y las separaciones entre destellos en milisegundos.

Principales resultados:

  • Se observó una tasa de relámpagos de Júpiter de 6.1 × 10-2 por km2 / año, un orden de magnitud mayor que el reportado anteriormente.
  • Detectamos destellos con pequeñas extensiones espaciales, indicando orígenes por encima del nivel de 2 barras.
  • Energías de destellos medidos comparables a las del rayo terrestre.

Conclusiones:

  • El rayo de Júpiter ocurre a una tasa significativamente mayor de lo estimado anteriormente.
  • La presencia de rayos por encima del nivel de 2 bares sugiere que el agua no es esencial para la generación de relámpagos.
  • Múltiples mecanismos de generación de rayos probablemente operan en la atmósfera de Júpiter, lo que requiere una mayor investigación sobre la convección atmosférica y la composición.