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関連する概念動画

Types of Radioactivity03:23

Types of Radioactivity

The most common types of radioactivity are α decay, β decay, γ decay, neutron emission, and electron capture.
Alpha (α) decay is the emission of an α particle from the nucleus. For example, polonium-210 undergoes α decay:
Subatomic Particles03:37

Subatomic Particles

Dalton was only partially correct about the particles that make up matter. All matter is composed of atoms, and atoms are composed of three smaller subatomic particles: protons, neutrons, and electrons. These three particles account for the mass and the charge of an atom.
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...
Average Acceleration01:30

Average Acceleration

The importance of understanding acceleration spans our day-to-day experiences, as well as the vast reaches of outer space and the tiny world of subatomic physics. In everyday conversation, to accelerate means to speed up. For instance, we are familiar with the acceleration of our car; the harder we apply our foot to the gas pedal, the faster we accelerate. The greater the acceleration, the greater the change in velocity over a given time. Acceleration is widely seen in experimental physics. In...
Radioactive Decay and Radiometric Dating02:48

Radioactive Decay and Radiometric Dating

Radioactivity is a spontaneous disintegration of an unstable nuclide and is a random process, as all the nuclei in the sample do not decay simultaneously. The number of disintegrations per unit time is called the activity (A), which is directly proportional to the number of nuclei in the sample. The decay constant (λ) is an average probability of decay per nucleus in unit time.
Atomic Radii and Effective Nuclear Charge03:08

Atomic Radii and Effective Nuclear Charge

The elements in groups of the periodic table exhibit similar chemical behavior. This similarity occurs because the members of a group have the same number and distribution of electrons in their valence shells.

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関連する実験動画

Updated: Jul 11, 2026

Visualization of Low-Level Gamma Radiation Sources Using a Low-Cost, High-Sensitivity, Omnidirectional Compton Camera
06:28

Visualization of Low-Level Gamma Radiation Sources Using a Low-Cost, High-Sensitivity, Omnidirectional Compton Camera

Published on: January 30, 2020

過去8万年にわたる太陽宇宙線におけるアルファ粒子

L J Lanzerotti, R C Reedy, J R Arnold

    Science (New York, N.Y.)
    |March 23, 1973
    PubMed
    まとめ

    太陽宇宙線のアルファ粒子の流れは,月面のサンプルのコバルト-57,コバルト-58,ニッケル-59の生産率を計算するために使用されました. これらの発見は,長期および現在の太陽アルファ粒子の流れが類似することを示唆しています.

    科学分野:

    • 宇宙線物理学 宇宙線物理学
    • 月科学 月科学 月科学
    • 核天体物理学 核天体物理学とは

    背景:

    • 太陽宇宙線 (SCR) は,太陽から発生するエネルギー粒子です.
    • SCR流の理解は,地球外物質の組成を解釈する上で極めて重要です.
    • 以前の研究では,SCRの相互作用と月のサンプルを分析した.

    研究 の 目的:

    • 月面サンプルにおける特定の同位体 (コバルト-57,コバルト-58,ニッケル-59) の生産率を計算する.
    • ニッケル-59の計算された生産率と測定された活動を比較する.
    • 現在と長期の太陽アルファ粒子の流れの一貫性を評価する.

    主な方法:

    • 太陽宇宙線からのアルファ粒子の流れの衛星測定 (1967年−1969年) を利用した.
    • 月面の材料におけるコバルト-57,コバルト-58,ニッケル-59の計算された生産率.
    • 月面サンプルにおけるニッケル-59の実験的に決定された活動と計算された生産率を比較した.

    主要な成果:

    • コバルト-57,コバルト-58,ニッケル-59の生産率は,当時のSCRの流れに基づいて決定されました.
    • 月面のサンプルで測定されたニッケル-59の活動は,計算された割合と一致することが判明しました.

    さらに関連する動画

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    Scattering And Absorption of Light in Planetary Regoliths
    11:34

    Scattering And Absorption of Light in Planetary Regoliths

    Published on: July 1, 2019

    関連する実験動画

    Last Updated: Jul 11, 2026

    Visualization of Low-Level Gamma Radiation Sources Using a Low-Cost, High-Sensitivity, Omnidirectional Compton Camera
    06:28

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    Published on: January 30, 2020

    X-ray Beam Induced Current Measurements for Multi-Modal X-ray Microscopy of Solar Cells
    10:16

    X-ray Beam Induced Current Measurements for Multi-Modal X-ray Microscopy of Solar Cells

    Published on: August 20, 2019

    Scattering And Absorption of Light in Planetary Regoliths
    11:34

    Scattering And Absorption of Light in Planetary Regoliths

    Published on: July 1, 2019

  • 長期と現在の太陽のアルファ粒子の流れは,約4の因数で比較可能であることが判明しました.
  • 結論:

    • 現在の太陽宇宙線のアルファ粒子の流動は,長期的な平均流動の信頼できる指標です.
    • 月面のサンプルのニッケル-59のようなコスモゲンイソトープの生成は,衛星からの流量データを用いて正確にモデル化することができます.
    • この研究は,月のサンプル分析のための関連する時間スケールにおける太陽のアルファ粒子の放出の安定性に関する証拠を提供します.