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相关概念视频

Doppler Effect - I00:56

Doppler Effect - I

The Doppler effect and Doppler shift were named after the Austrian physicist and mathematician Christian Johann Doppler in 1842, who conducted experiments with both moving sources and moving observers. Consider an observer standing on a street corner, observing an ambulance with a siren sound passing by at a constant speed. The observer experiences two characteristic changes in the sound of the siren. Initially, the sound increases in loudness as the ambulance approaches and decreases in...
Doppler Effect - II01:05

Doppler Effect - II

The Doppler effect has several practical, real-world applications. For instance, meteorologists use Doppler radars to interpret weather events based on the Doppler effect. Typically, a transmitter emits radio waves at a specific frequency toward the sky from a weather station. The radio waves bounce off the clouds and precipitation and travel back to the weather station. The radio frequency of the waves reflected back to the station appears to decrease if the clouds or precipitation are moving...
¹H NMR: Interpreting Distorted and Overlapping Signals01:02

¹H NMR: Interpreting Distorted and Overlapping Signals

Spin systems where the difference in chemical shifts of the coupled nuclei is greater than ten times J are called first-order spin systems. These nuclei are weakly coupled, and their chemical shifts and coupling constant can generally be estimated from the well-separated signals in the spectrum.
As Δν decreases and the signals move closer, the doublets appear increasingly distorted. The intensities of the inner lines increase at the cost of those of the outer lines as the signals are slanted or...
NMR Spectroscopy: Chemical Shift Overview01:15

NMR Spectroscopy: Chemical Shift Overview

The position of the absorption signal of a sample is reported relative to the position of the signal of tetramethylsilane (TMS), which is added as an internal reference while recording spectra. The difference between the absorption frequencies of the sample and TMS (in Hz) is divided by the spectrometer operating frequency (in MHz) to obtain a dimensionless quantity called the chemical shift. It is reported on the δ (delta) scale and expressed in parts per million.
For instance, the proton...
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...
Detection of Black Holes01:10

Detection of Black Holes

Although black holes were theoretically postulated in the 1920s, they remained outside the domain of observational astronomy until the 1970s.
Their closest cousins are neutron stars, which are composed almost entirely of neutrons packed against each other, making them extremely dense. A neutron star has the same mass as the Sun but its diameter is only a few kilometers. Therefore, the escape velocity from their surface is close to the speed of light.
Not until the 1960s, when the first neutron...

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相关实验视频

Updated: Jul 12, 2026

High Resolution Phonon-assisted Quasi-resonance Fluorescence Spectroscopy
10:40

High Resolution Phonon-assisted Quasi-resonance Fluorescence Spectroscopy

Published on: June 28, 2016

类星体的多普勒解释红移.

H S Zapolsky

    Science (New York, N.Y.)
    |August 5, 1966
    PubMed
    概括

    这项研究探讨了类星体是否是局部,快速移动的物体. 这些发现表明,这个假设与观测数据以及类星体的宇宙红移模型一致.

    科学领域:

    • 天文学 天文学
    • 天体物理学 天体物理学

    背景情况:

    • 准星体源 (类星体) 对它们的性质和起源构成了宇宙学难题.
    • 主流的宇宙学模型解释说,类星体红移是宇宙膨胀的结果.

    研究的目的:

    • 为了调查类星体是以相对论速度移动的局部物体的替代假设.
    • 将本局运动假设的观测预测与现有的类星体数据进行比较.

    主要方法:

    • 对速度同otropic 分布的横向多普勒效应的分析.
    • 建模具有红移小于z的对象数量 (N(z)) .
    • 基于局部类星体的两个极端起源假设计算红移大小曲线.

    主要成果:

    • 横向多普勒效应预测蓝变移比红变移更少,用于同otropic局部运动.
    • 导出的N(z) 函数与当前的观测数据一致.
    • 基于类星体的银河系爆炸起源的红移大小曲线与宇宙红移模型相比,适合观测.

    结论:

    • 关于局部,高速类星体的假设与当前的天文观测并不矛盾.
    • 这种局部运动模型为类星体特性提供了另一种解释,与标准宇宙学解释相竞争.

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    Last Updated: Jul 12, 2026

    High Resolution Phonon-assisted Quasi-resonance Fluorescence Spectroscopy
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    Published on: June 28, 2016

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    Published on: March 22, 2019

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