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Generating Electromagnetic Radiations01:10

Generating Electromagnetic Radiations

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The German physicist Heinrich Hertz (1857–1894) was the first to generate and detect certain types of electromagnetic waves in the laboratory. Starting in 1887, he performed a series of experiments that confirmed the existence of electromagnetic waves and verified that they travel at the speed of light. Hertz used an alternating-current RLC (resistor-inductor-capacitor) circuit that resonated at a known frequency and connected it to a loop of wire. High voltages induced across the gap in...
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Electromagnetic Waves01:30

Electromagnetic Waves

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James Clerk Maxwell formulated a single theory combining all the electric and magnetic effects scientists knew during that time, calling the phenomena his theory predicted “Electromagnetic waves”. He brought together all the work that had been done by brilliant physicists such as Oersted, Coulomb, Gauss, and Faraday and added his own insights to develop the overarching theory of electromagnetism. Maxwell’s equations, combined with the Lorentz force law, encompass all the laws...
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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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Standing Electromagnetic Waves01:15

Standing Electromagnetic Waves

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Electromagnetic waves can be reflected; the surface of a conductor or a dielectric can act as a reflector. As electric and magnetic fields obey the superposition principle, so do electromagnetic waves. The superposition of an incident wave and a reflected electromagnetic wave produces a standing wave analogous to the standing waves created on a stretched string.
Suppose a sheet of a perfect conductor is placed in the yz-plane, and a linearly polarized electromagnetic wave traveling in the...
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Electromagnetic Fields01:30

Electromagnetic Fields

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Electric fields generated by static charges, often referred to as electrostatic fields, are characteristically different from electric fields created by time-varying magnetic fields. While the former is a conservative field, implying that no net work is done on a test charge if it goes around in a complete loop in the field, the latter is, by definition, not a conservative field; net work is done, and it is proportional to the rate of change of magnetic flux.
However, the observation of...
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Intensity Of Electromagnetic Waves01:22

Intensity Of Electromagnetic Waves

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The energy transport per unit area per unit time, or the Poynting vector, gives the energy flux of an electromagnetic wave at any specific time. For a plane electromagnetic wave with E0 and B0 as the peak electric and magnetic fields and traveling along the x-axis, the time-varying energy flux can be given by the following equation:
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Updated: Mar 1, 2026

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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Ondas generadas por rayos detectadas en Marte

František Němec1, Kateřina Rosická1,2, Ivana Kolmašová1,2

  • 1Faculty of Mathematics and Physics, Charles University, Prague, Czech Republic.

Science advances
|February 27, 2026
PubMed
Resumen
Este resumen es generado por máquina.

Científicos detectaron ondas electromagnéticas generadas por rayos en la ionosfera de Marte utilizando la nave espacial MAVEN. Esto proporciona evidencia de descargas eléctricas, o rayos, que ocurren en la atmósfera marciana.

Palabras clave:
rayosMarteondas electromagnéticasionosferaMAVENdescargas eléctricasatmósfera marciana

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Área de la Ciencia:

  • Ciencia Planetaria
  • Física Atmosférica
  • Electromagnetismo

Sus antecedentes:

  • Los rayos se confirman en Júpiter, Saturno y Neptuno a través de ondas electromagnéticas.
  • La presencia de rayos en Venus y Marte no está confirmada actualmente.
  • La comprensión de los rayos planetarios proporciona información sobre la dinámica atmosférica y los procesos eléctricos.

Objetivo del estudio:

  • Investigar la posible ocurrencia de rayos en Marte.
  • Analizar las señales de ondas electromagnéticas detectadas en la ionosfera marciana.
  • Proporcionar evidencia directa a favor o en contra de las descargas eléctricas en Marte.

Principales métodos:

  • Se utilizaron datos de la nave espacial MAVEN de la NASA.
  • Se detectó y analizó una señal de whistler dispersa en frecuencia en la ionosfera marciana.
  • Se modeló la propagación de ondas desde la atmósfera marciana hasta la nave espacial.
  • Se incorporaron modelos realistas del campo magnético de la corteza y de la ionosfera para el análisis.

Principales resultados:

  • Se observó una señal de whistler dispersa en frecuencia, indicativa de ondas electromagnéticas generadas por rayos.
  • Se demostró la plausibilidad de la propagación de ondas desde la atmósfera marciana hasta la nave espacial MAVEN.
  • Se demostró que la dispersión de la señal observada se alinea con las expectativas teóricas basadas en modelos marcianos.
  • Atribución de la señal a una fuente impulsiva en la atmósfera marciana.

Conclusiones:

  • El whistler detectado proporciona evidencia directa de ondas electromagnéticas originadas en una fuente impulsiva en Marte.
  • Estos hallazgos sugieren fuertemente que las descargas eléctricas, similares a los rayos, pueden ocurrir en la atmósfera marciana.
  • Este descubrimiento abre nuevas vías para el estudio de la electricidad atmosférica en otros planetas.