Jove
Visualize
Contáctanos

Videos de Conceptos Relacionados

Kepler's First Law of Planetary Motion01:10

Kepler's First Law of Planetary Motion

4.9K
In the early 17th century, German astronomer and mathematician Johannes Kepler postulated three laws for the motion of planets in the solar system. He formulated his first two laws based on the observations of his forebears, Nikolaus Copernicus and Tycho Brahe.
Polish astronomer Nikolaus Copernicus put forth a theory that stated a heliocentric model for the solar system. According to this heliocentric theory, all the planets, including Earth, orbit the Sun in circular orbits.
On the other hand,...
4.9K
Kepler's Third Law of Planetary Motion01:18

Kepler's Third Law of Planetary Motion

3.6K
In the early 17th century, German astronomer and mathematician Johannes Kepler postulated three laws for the motion of planets in the solar system. In 1909, he formulated his first two laws based on the observations of his forebears, Nikolaus Copernicus and Tycho Brahe. However, in 1918, he published his third law of planetary motion, which gives a precise mathematical relationship between a planet's average distance from the Sun and the amount of time it takes to revolve around the Sun. It...
3.6K
Plane Electromagnetic Waves II01:29

Plane Electromagnetic Waves II

3.1K
Consider a plane wavefront traveling in position x-direction with a constant speed. This wavefront can be utilized to obtain the relationship between electric and magnetic fields with the help of Faraday's law.
3.1K
Graphing the Wave Function01:13

Graphing the Wave Function

3.3K
Consider the wave equation for a sinusoidal wave moving in the positive x-direction. The wave equation is a function of both position and time. From the wave equation, two different graphs can be plotted.
3.3K
Inductively Coupled Plasma Atomic Emission Spectroscopy: Principle01:19

Inductively Coupled Plasma Atomic Emission Spectroscopy: Principle

2.4K
Inductively coupled plasma (ICP) is the most widely used plasma source in atomic emission spectroscopy (AES), also known as Inductively Coupled Plasma Optical Emission Spectroscopy (ICP-OES). The ICP source, or torch, consists of three concentric quartz tubes with argon gas flowing through them. A spark from a Tesla coil initiates the ionization of argon, generating a high-temperature plasma.
The ions and electrons produced interact with the fluctuating magnetic field created by a water-cooled...
2.4K
Inductively Coupled Plasma Atomic Emission Spectroscopy: Instrumentation01:26

Inductively Coupled Plasma Atomic Emission Spectroscopy: Instrumentation

1.1K
Inductively coupled plasma (ICP) is the common plasma source used in atomic emission spectroscopy (AES), a technique that detects and analyzes various elements in a sample. This method is often called inductively coupled plasma atomic emission spectroscopy (ICP-AES).
There are three main types of inductively coupled plasma atomic emission spectroscopy  (ICP-AES) instruments: sequential, simultaneous multichannel, and Fourier transform instruments, with the latter being less commonly used....
1.1K

También podría leer

Artículos Relacionados

Artículos vinculados a este trabajo por autores compartidos, revista y gráfico de citas.

Ordenar por
Same author

The origins of patchy aurora at Jupiter.

Nature communications·2026
Same author

In situ and remote observations of the ultraviolet footprint of the moon Callisto by the Juno spacecraft.

Nature communications·2025
Same author

New Plasma Regime in Jupiter's Auroral Zones.

Physical review letters·2025
Same author

Evidence of Magnetic Reconnection in Ganymede's Wake Region From Juno.

Journal of geophysical research. Space physics·2024
Same author

In situ evidence of the magnetospheric cusp of Jupiter from Juno spacecraft measurements.

Nature communications·2024
Same author

The Electric and Magnetic Fields Instrument Suite and Integrated Science (EMFISIS): Science, Data, and Usage Best Practices.

Space science reviews·2023
Same journal

Erratum for the Research Article "Detecting supramolecular organic nanoparticles during heat wave".

Science (New York, N.Y.)·2026
Same journal

Local signals, systemic decline.

Science (New York, N.Y.)·2026
Same journal

The mechanics of liver regeneration.

Science (New York, N.Y.)·2026
Same journal

Computing in a memory with physics.

Science (New York, N.Y.)·2026
Same journal

Retraction.

Science (New York, N.Y.)·2026
Same journal

Making time.

Science (New York, N.Y.)·2026
Ver todos los artículos relacionados
JoVE
x logofacebook logolinkedin logoyoutube logo
ACERCA DE JoVE
Visión GeneralLiderazgoBlogCentro de Ayuda JoVE
AUTORES
Proceso de PublicaciónConsejo EditorialAlcance y PolíticasRevisión por ParesPreguntas FrecuentesEnviar
BIBLIOTECARIOS
TestimoniosSuscripcionesAccesoRecursosConsejo Asesor de BibliotecasPreguntas Frecuentes
INVESTIGACIÓN
JoVE JournalMethods CollectionsJoVE Encyclopedia of ExperimentsArchivo
EDUCACIÓN
JoVE CoreJoVE BusinessJoVE Science EducationJoVE Lab ManualCentro de Recursos para ProfesoresSitio de Profesores
Términos y Condiciones de Uso
Política de Privacidad
Políticas

Video Experimental Relacionado

Updated: May 2, 2026

Investigation of Early Plasma Evolution Induced by Ultrashort Laser Pulses
11:20

Investigation of Early Plasma Evolution Induced by Ultrashort Laser Pulses

Published on: July 2, 2012

16.9K

Observaciones de la primera onda de plasma en el urano.

D A Gurnett, W S Kurth, F L Scarf

    Science (New York, N.Y.)
    |July 4, 1986
    PubMed
    Resumen
    Este resumen es generado por máquina.

    La Voyager 2 detectó emisiones de radio y ondas de plasma alrededor de Urano, revelando detalles sobre su magnetosfera y impactos de polvo. Estos hallazgos mejoran nuestra comprensión del entorno uraniano y las magnetosferas planetarias.

    Más Videos Relacionados

    Emission Spectroscopic Boundary Layer Investigation during Ablative Material Testing in Plasmatron
    09:41

    Emission Spectroscopic Boundary Layer Investigation during Ablative Material Testing in Plasmatron

    Published on: June 9, 2016

    15.0K
    Experimental Methods of Dust Charging and Mobilization on Surfaces with Exposure to Ultraviolet Radiation or Plasmas
    07:54

    Experimental Methods of Dust Charging and Mobilization on Surfaces with Exposure to Ultraviolet Radiation or Plasmas

    Published on: April 3, 2018

    8.0K

    Videos de Experimentos Relacionados

    Last Updated: May 2, 2026

    Investigation of Early Plasma Evolution Induced by Ultrashort Laser Pulses
    11:20

    Investigation of Early Plasma Evolution Induced by Ultrashort Laser Pulses

    Published on: July 2, 2012

    16.9K
    Emission Spectroscopic Boundary Layer Investigation during Ablative Material Testing in Plasmatron
    09:41

    Emission Spectroscopic Boundary Layer Investigation during Ablative Material Testing in Plasmatron

    Published on: June 9, 2016

    15.0K
    Experimental Methods of Dust Charging and Mobilization on Surfaces with Exposure to Ultraviolet Radiation or Plasmas
    07:54

    Experimental Methods of Dust Charging and Mobilization on Surfaces with Exposure to Ultraviolet Radiation or Plasmas

    Published on: April 3, 2018

    8.0K

    Área de la Ciencia:

    • Ciencias planetarias Ciencias planetarias.
    • Física del plasma es la física del plasma.
    • Ingeniería Aeroespacial Ingeniería Aeroespacial.

    Sus antecedentes:

    • La misión de la Voyager 2 proporcionó mediciones in situ sin precedentes de Urano.
    • Comprender las magnetosferas planetarias es crucial para la exploración espacial.

    Objetivo del estudio:

    • Para analizar los datos de las ondas de plasma del encuentro con Urano de la Voyager 2.
    • Para caracterizar las emisiones de radio, los fenómenos magnetosféricos y los impactos de polvo.

    Principales métodos:

    • Utilizó datos del instrumento de ondas de plasma de la Voyager 2.
    • Se analizaron las emisiones de radio a frecuencias de kilohertz.
    • Identificó turbulencias de plasma, emisiones de ondas e impactos de polvo.

    Principales resultados:

    • Las emisiones de radio detectadas antes de la aproximación más cercana.
    • Se observó un arco de choque, un silbido en modo silbido y emisiones de coro dentro de la magnetosfera.
    • Se registraron altas tasas de impactos de partículas de polvo de tamaño micrométrico cerca del plano del anillo.

    Conclusiones:

    • Las observaciones de la Voyager 2 ofrecen información sobre la dinámica magnetosférica de Urano.
    • El estudio pone de relieve la presencia y el impacto de partículas de polvo en el sistema de anillos de Urano.
    • Los datos contribuyen a una comprensión más amplia de los entornos de los planetas exteriores.