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相关概念视频

The Electromagnetic Spectrum02:37

The Electromagnetic Spectrum

The electromagnetic spectrum consists of all the types of electromagnetic radiation arranged according to their frequency and wavelength. Each of the various colors of visible light has specific frequencies and wavelengths associated with them, and you can see that visible light makes up only a small portion of the electromagnetic spectrum. Because the technologies developed to work in various parts of the electromagnetic spectrum are different, for reasons of convenience and historical...
The Electromagnetic Spectrum01:24

The Electromagnetic Spectrum

Electromagnetic waves are categorized according to their wavelengths and frequencies, giving the electromagnetic spectrum. These waves are classified as radio, infrared, ultraviolet, etc. Radio waves refer to electromagnetic radiation with wavelengths ranging from millimeters to kilometers. Radio waves are commonly used for audio communications (i.e., radios) and typically result from an alternating current in the wires of a broadcast antenna. They cover a broad wavelength range and are used...
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...
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:
Emission Spectra02:39

Emission Spectra

When solids, liquids, or condensed gases are heated sufficiently, they radiate some of the excess energy as light. Photons produced in this manner have a range of energies, and thereby produce a continuous spectrum in which an unbroken series of wavelengths is present.
Schwarzschild Radius and Event Horizon01:21

Schwarzschild Radius and Event Horizon

No object with a finite mass can travel faster than the speed of light in a vacuum. This fact has an interesting consequence in the domain of extremely high gravitational fields.
The minimum speed required to launch a projectile from the surface of an object to which it is gravitationally bound so that it eventually escapes the object’s gravitational field is called the escape velocity. The escape velocity is independent of the mass of the object. Merging the idea of escape velocity with the...

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相关实验视频

Updated: Jul 11, 2026

Characterizing Far-infrared Laser Emissions and the Measurement of Their Frequencies
09:38

Characterizing Far-infrared Laser Emissions and the Measurement of Their Frequencies

Published on: December 18, 2015

类星体,黑星和玛射线等等.

C D Dermer, R Schlickeiser

    Science (New York, N.Y.)
    |September 18, 1992
    PubMed
    概括

    康普顿马射线天文台 (CGRO) 发现了13个新的银河系外马射线源,主要是闪光灯,扩大了我们对活跃银河系核的理解. 这些发现揭示了宇宙中的能量过程,起源于超大质量黑洞.

    科学领域:

    • 高能天体物理学 高能天体物理学
    • 银河系外的天文学.
    • 宇宙射线物理学 宇宙射线物理学

    背景情况:

    • 在此之前,只有3C 273类星体被认为是超银河系的超大于100 MeV的马辐射源.
    • 康普顿马射线天文台 (CGRO) 上的能量马射线实验望远镜 (EGRET) 发射,用于测量马射线天空.

    研究的目的:

    • 为了识别和描述高能玛辐射的银河系外源.
    • 研究这些源的特性及其与活跃星系核 (AGN) 的关系.

    主要方法:

    • 使用来自康普顿马射线天文台 (CGRO) 的能量马射线实验望远镜 (EGRET) 的数据.
    • 分析来自银河系外来源的马射线辐射.
    • 将马射线发现与多波长观测 (无线电,光学) 相关联,以确定闪电星的特性.

    主要成果:

    • 在不到一年的CGRO观测中发现了13个新的银河系外马射线源,使总数达到14个.
    • 所有已识别的源都表现出闪光灯的特征,包括高光学极化,可变性和平面频谱无线电辐射.
    • 这些来源很可能是罕见的,有利地对齐的射电星系和带有相对论喷射的类星体.

    结论:

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    Femtosecond Laser Filaments for Use in Sub-Diffraction-Limited Imaging and Remote Sensing
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    Femtosecond Laser Filaments for Use in Sub-Diffraction-Limited Imaging and Remote Sensing

    Published on: April 25, 2019

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    Characterizing Far-infrared Laser Emissions and the Measurement of Their Frequencies
    09:38

    Characterizing Far-infrared Laser Emissions and the Measurement of Their Frequencies

    Published on: December 18, 2015

    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

    Femtosecond Laser Filaments for Use in Sub-Diffraction-Limited Imaging and Remote Sensing
    06:16

    Femtosecond Laser Filaments for Use in Sub-Diffraction-Limited Imaging and Remote Sensing

    Published on: April 25, 2019

    • CGRO的EGRET仪器显著增加了已知的银河系外马射线源的数量.
    • 星是我们银河系以外的高能马射线的主要来源.
    • 马射线观测为AGN和极端天体物理过程的中央引擎提供了关键的见解.