Jove
Visualize
Contáctanos

Videos de Conceptos Relacionados

Apparent Weight and the Earth's Rotation01:28

Apparent Weight and the Earth's Rotation

Since all objects on the Earth's surface move through a circle every 24 hours, there must be a net centripetal force on each object, directed towards the center of that circle. The points of the north and south poles are the only exception to this rule.
For an object on the Earth's equator, the net centripetal force that accounts for its rotation is the Earth's pull towards its center, or the weight minus the normal force that prevents it from piercing into the Earth's surface. This force,...
Gyroscope: Precession01:24

Gyroscope: Precession

Precession can be demonstrated effectively through a spinning top. If a spinning top is placed on a flat surface near the surface of the Earth at a vertical angle and is not spinning, it will fall over due to the force of gravity producing a torque acting on its center of mass. However, if the top is spinning on its axis, it precesses about the vertical direction, rather than topple over due to this torque. Precessional motion is a combination of a steady circular motion of the axis and the...
Relative Motion Analysis using Rotating Axes01:25

Relative Motion Analysis using Rotating Axes

Consider a component AB undergoing a linear motion. Along with a linear motion, point B also rotates around point A. To comprehend this complex movement, position vectors for both points A and B are established using a stationary reference frame.
However, to express the relative position of point B relative to point A, an additional frame of reference, denoted as x'y', is necessary. This additional frame not only translates but also rotates relative to the fixed frame, making it instrumental in...
Rotational Motion about a Fixed Axis01:26

Rotational Motion about a Fixed Axis

A rigid body's rotation around a fixed axis makes every point within it trace a circular path around a specific line or point. The term given to this type of spinning is defined by the angular position, symbolized by the angle θ. This angle is gauged from a static reference line to the revolving object. From this angular position, any variation is referred to as angular displacement, denoted by dθ. The extent of this displacement can be calculated in degrees, radians, or revolutions, where one...
Kinematic Equations for Rotation01:30

Kinematic Equations for Rotation

In mechanics, when one observes a rigid body in rotational motion with constant angular acceleration, it is possible to establish equations for its rotational kinematics. This process resembles how linear kinematics are dealt with in simpler motion studies.
For instance, imagine a point A on a rigid body engaged in circular motion. The translational velocity of this particular point can be calculated by taking the time derivatives of the displacement equation, which essentially measures the...
Relative Motion Analysis using Rotating Axes - Acceleration01:22

Relative Motion Analysis using Rotating Axes - Acceleration

Consider a component AB undergoing a linear motion. Along with a linear motion, point B also rotates around point A. To comprehend this complex movement, position vectors for both points A and B are established using a stationary reference frame. The absolute velocity of point B is determined by adding the absolute velocity of point A, the relative velocity of point B in the rotating frame, and the effects caused by the angular velocity within the rotating frame.
Time differentiation is...

También podría leer

Artículos Relacionados

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

Ordenar por
Same author

A versatile thermoelectric temperature controller with 10 mK reproducibility and 100 mK absolute accuracy.

The Review of scientific instruments·2010
Same author

Cylindrically symmetric Green's function approach for modeling the crystal growth morphology of ice.

Physical review. E, Statistical physics, plasmas, fluids, and related interdisciplinary topics·2002
Same author

Advances in helioseismology.

Science (New York, N.Y.)·1991
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: Jul 12, 2026

Methods for Measuring the Orientation and Rotation Rate of 3D-printed Particles in Turbulence
12:34

Methods for Measuring the Orientation and Rotation Rate of 3D-printed Particles in Turbulence

Published on: June 24, 2016

Observaciones de la variación del tiempo en la rotación del Sol.

M F Woodard, K G Libbrecht

    Science (New York, N.Y.)
    |June 18, 1993
    PubMed
    Resumen

    Las variaciones del ciclo solar causan pequeños cambios en la rotación subterránea del Sol. Estos cambios de velocidad angular, principalmente en latitudes altas, están vinculados a la actividad solar.

    Área de la Ciencia:

    • * Física del Sol Física del Sol * Física del Sol * Física del Sol * Física del Sol * Física del Sol * Física del Sol
    • * Helioseismología
    • * Solar Dynamo es un sistema de energía solar.

    Sus antecedentes:

    • * Las divisiones de frecuencia del modo p solar proporcionan información sobre la estructura interna y la dinámica del Sol.
    • * Anteriores observaciones heliosísmicas indicaron variaciones relacionadas con el ciclo solar en el interior del Sol.

    Objetivo del estudio:

    • * Para investigar los cambios en la velocidad angular del subsuelo del Sol durante un ciclo solar utilizando datos heliosísmicos.
    • * Para determinar la dependencia de latitud de las variaciones de la velocidad de rotación solar.
    • * Explorar los vínculos potenciales entre los cambios de velocidad angular observados y la actividad solar.

    Principales métodos:

    Más Videos Relacionados

    Measurement of Aerosols Optical Thickness of the Atmosphere using the GLOBE Handheld Sun Photometer
    06:27

    Measurement of Aerosols Optical Thickness of the Atmosphere using the GLOBE Handheld Sun Photometer

    Published on: May 29, 2019

    A Method of Trigonometric Modelling of Seasonal Variation Demonstrated with Multiple Sclerosis Relapse Data
    10:46

    A Method of Trigonometric Modelling of Seasonal Variation Demonstrated with Multiple Sclerosis Relapse Data

    Published on: December 9, 2015

    Videos de Experimentos Relacionados

    Last Updated: Jul 12, 2026

    Methods for Measuring the Orientation and Rotation Rate of 3D-printed Particles in Turbulence
    12:34

    Methods for Measuring the Orientation and Rotation Rate of 3D-printed Particles in Turbulence

    Published on: June 24, 2016

    Measurement of Aerosols Optical Thickness of the Atmosphere using the GLOBE Handheld Sun Photometer
    06:27

    Measurement of Aerosols Optical Thickness of the Atmosphere using the GLOBE Handheld Sun Photometer

    Published on: May 29, 2019

    A Method of Trigonometric Modelling of Seasonal Variation Demonstrated with Multiple Sclerosis Relapse Data
    10:46

    A Method of Trigonometric Modelling of Seasonal Variation Demonstrated with Multiple Sclerosis Relapse Data

    Published on: December 9, 2015

  • * Análisis de los datos de división de la frecuencia solar en modo p del Observatorio Solar Big Bear (1986 y 1988-90).
  • * Aplicación de técnicas de inversión asintótica a los datos heliosísmicos.
  • * Comparación de las tasas de rotación en diferentes latitudes solares y períodos de tiempo.
  • Principales resultados:

    • * Pequeño (aprox. 1%) se detectaron cambios en la velocidad angular subterránea que se correlacionan con el ciclo solar.
    • * Las mayores variaciones de velocidad angular (aprox. 4 nHz) ocurrió entre 1986 y 1988-90 en altas latitudes solares (aprox. 60 grados). también se llama 60 grados.
    • * La heliosismología reveló cambios en la velocidad de rotación dependientes de la latitud.

    Conclusiones:

    • * La velocidad de rotación subterránea del Sol varía con el ciclo solar, particularmente en latitudes altas.
    • * Los cambios de velocidad angular observados son consistentes en magnitud con las sugerencias anteriores con respecto a las influencias del ciclo solar en la zona de convección solar.
    • * Todavía se necesita un modelo detallado que explique estas variaciones de velocidad angular inducidas por el ciclo solar.