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関連する概念動画

Momentum And Radiation Pressure01:20

Momentum And Radiation Pressure

An object absorbing an electromagnetic wave would experience a force in the direction of propagation of the wave. This force occurs because electromagnetic waves contain and transport momentum. The force accounts for the wave's radiation pressure exerted on the object. Maxwell's prediction was confirmed in 1903 by Nichols and Hull by precisely measuring radiation pressures with a torsion balance. The measuring instrument had mirrors suspended from a fiber kept inside a glass container. Nichols...
Diamagnetic Shielding of Nuclei: Local Diamagnetic Current01:14

Diamagnetic Shielding of Nuclei: Local Diamagnetic Current

An applied magnetic field causes the electrons present in the molecule to circulate, setting up a local diamagnetic current within the molecule. The local diamagnetic current arising from circulating sigma-bonding electrons induces a magnetic field, Blocal that opposes the applied magnetic field, B0. The effective magnetic field experienced by these nuclei is given by the difference between the applied and local magnetic fields in a phenomenon called local diamagnetic shielding. Essentially,...
Atomic Nuclei: Nuclear Spin State Population Distribution01:14

Atomic Nuclei: Nuclear Spin State Population Distribution

Near absolute zero temperatures, in the presence of a magnetic field, the majority of nuclei prefer the lower energy spin-up state to the higher energy spin-down state. As temperatures increase, the energy from thermal collisions distributes the spins more equally between the two states. The Boltzmann distribution equation gives the ratio of the number of spins predicted in the spin −½ (N−) and spin +½ (N+) states.
Atomic Nuclei: Larmor Precession Frequency01:11

Atomic Nuclei: Larmor Precession Frequency

The earth's gravitational field produces a 'twisting force' perpendicular to the angular momentum of a spinning mass (such as a spinning top) that causes the mass to 'wobble' around the gravitational field axis in a phenomenon called precession. Similarly, the magnetic moment (μ) of a spinning nucleus precesses due to an external magnetic field directed along the z-axis. The precession of the magnetic moment vector about the magnetic field is called Larmor precession, and the angular frequency...
Atomic Nuclei: Nuclear Magnetic Moment00:59

Atomic Nuclei: Nuclear Magnetic Moment

All atomic nuclei are positively charged. When they have a nonzero spin, they behave like rotating charges. As a consequence of their charge and spin, these nuclei generate a magnetic field (B). This, in turn, gives rise to a magnetic moment (μ), which is randomly oriented in the absence of an external magnetic field. When an external magnetic field (B0) is applied, the magnetic moment vectors can align with the field or against it in 2 + 1 orientations. A hydrogen nucleus, which is just a...
Atomic Nuclei: Nuclear Spin State Overview01:03

Atomic Nuclei: Nuclear Spin State Overview

NMR-active nuclei have energy levels called 'spin states' that are associated with the orientations of their nuclear magnetic moments. In the absence of a magnetic field, the nuclear magnetic moments are randomly oriented, and the spin states are degenerate. When an external magnetic field is applied, the spin states have only 2 + 1 orientations available to them. A proton with = ½ has two available orientations. Similarly, for a quadrupolar nucleus with a nuclear spin value of one, the...

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関連する実験動画

Updated: Jul 12, 2026

Scattering And Absorption of Light in Planetary Regoliths
11:34

Scattering And Absorption of Light in Planetary Regoliths

Published on: July 1, 2019

彗星核の可視性について

E P Ney

    Science (New York, N.Y.)
    |January 22, 1982
    PubMed
    まとめ

    ハレー彗星のイメージング

    科学分野:

    • 天文学と天体物理学について
    • 彗星科学は彗星科学である.

    背景:

    • 彗星核のイメージングは,宇宙ミッションにとって極めて重要です.
    • 彗星を囲む塵雲は,核の表面を覆い隠す可能性があります.
    • 塵の密度を理解することは,観測の成功の鍵です.

    研究 の 目的:

    • 彗星核の可視性を評価するために.
    • ハレー彗星の核を画像化できるかどうかを判断するために.
    • 彗星画像の塵遮蔽効果を評価するために.

    主な方法:

    • 9つの彗星からのブロードバンドフォトメトリーデータの分析.
    • 1910年に観測された彗星とハレー彗星の視覚的明るさの比較.
    • 塵の密度とそのイメージングへの影響を評価する.

    主要な成果:

    • 彗星からの塵雲は,核画像撮影にほとんど干渉しない.
    • 彗星ウエストの核は,周日点の近くの塵によって遮られていました.
    • ハレーの核は,塵によって著しく遮られる可能性は低い.

    結論:

    さらに関連する動画

    Using Computer Vision Libraries to Streamline Nuclei Quantification
    06:25

    Using Computer Vision Libraries to Streamline Nuclei Quantification

    Published on: June 6, 2025

    Detection of DNA Breaks in Dividing Human Cells by Neutral Comet Assay
    05:55

    Detection of DNA Breaks in Dividing Human Cells by Neutral Comet Assay

    Published on: August 23, 2024

    関連する実験動画

    Last Updated: Jul 12, 2026

    Scattering And Absorption of Light in Planetary Regoliths
    11:34

    Scattering And Absorption of Light in Planetary Regoliths

    Published on: July 1, 2019

    Using Computer Vision Libraries to Streamline Nuclei Quantification
    06:25

    Using Computer Vision Libraries to Streamline Nuclei Quantification

    Published on: June 6, 2025

    Detection of DNA Breaks in Dividing Human Cells by Neutral Comet Assay
    05:55

    Detection of DNA Breaks in Dividing Human Cells by Neutral Comet Assay

    Published on: August 23, 2024

    • ハレー彗星の核の画像撮影は可能である.
    • 塵の遮蔽はハレー観測に重大な障壁ではない.
    • 将来の宇宙ミッションでは,核写真撮影を進めることができます.