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関連する概念動画

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...

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関連する実験動画

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

太陽の自転における時間変動の観測

M F Woodard, K G Libbrecht

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

    太陽の周期の変化は,太陽の地下回転の小さな変化を引き起こします. これらの角速度の変化は,主に高緯度では,太陽活動と関連しています.

    科学分野:

    • * 太陽物理学 太陽物理学
    • *ヘリオ地震学について
    • * ソーラーダイナモ

    背景:

    • *太陽のpモード周波数分割は,太陽の内部構造と動力学についての洞察を提供します.
    • * 過去のヘリオ地震観測は,太陽の内部の太陽周期に関連する変動を示していた.

    研究 の 目的:

    • *太陽の地下表面の角速度の変化を太陽周期でヘリオ地震データを用いて調査する.
    • * 太陽の回転速度の変動の緯度依存を決定する.
    • * 観測された角速度の変化と太陽活動との潜在的な関連性を探求する.

    主な方法:

    • * ビッグベア太陽観測所 (1986年と1988-90年) の太陽pモード周波数分割データの分析.
    • * アシンプトティック・インバーション・テクニックをヘリオ・シズミック・データに適用.
    • * 太陽の異なる緯度と時間帯における自転速度の比較.

    主要な成果:

    • * 小さい (約. 1%) で,太陽周期と相関する地下角速度の変化が検出されました.
    • * 最大の角速度変動 (約. 4 nHz) が1986年から1988-90年の間に,太陽の高緯度 (約. 60度) となる.
    • *ヘリオ地震学により,緯度に依存する回転速度の変化が明らかになった.

    さらに関連する動画

    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

    関連する実験動画

    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

    結論:

    • *太陽の地下回転率は,太陽の周期によって変化し,特に高緯度では変化します.
    • *観測された角速度の変化の大きさは,太陽のコンベクションゾーンにおける太陽周期の影響に関する以前の示唆と一致しています.
    • *これらの太陽周期によって引き起こされる角速度の変化を説明する詳細なモデルはまだ必要である.