Jove
Visualize
联系我们
JoVE
x logofacebook logolinkedin logoyoutube logo
关于 JoVE
概览领导团队博客JoVE 帮助中心
作者
出版流程编辑委员会范围与政策同行评审常见问题投稿
图书馆员
用户评价订阅访问资源图书馆顾问委员会常见问题
研究
JoVE JournalMethods CollectionsJoVE Encyclopedia of Experiments存档
教育
JoVE CoreJoVE BusinessJoVE Science EducationJoVE Lab Manual教师资源中心教师网站
使用条款与条件
隐私政策
政策

相关概念视频

X-ray Crystallography02:18

X-ray Crystallography

21.6K
The size of the unit cell and the arrangement of atoms in a crystal may be determined from measurements of the diffraction of X-rays by the crystal, termed X-ray crystallography.
Diffraction
Diffraction is the change in the direction of travel experienced by an electromagnetic wave when it encounters a physical barrier whose dimensions are comparable to those of the wavelength of the light. X-rays are electromagnetic radiation with wavelengths about as long as the distance between neighboring...
21.6K
Detection of Black Holes01:10

Detection of Black Holes

1.7K
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...
1.7K
X-ray Diffraction of Biological Samples01:10

X-ray Diffraction of Biological Samples

3.9K
X-ray diffraction or XRD is an analytical tool that utilizes X-rays to study ordered structures such as crystalline organic and inorganic samples, polycrystalline materials, proteins, carbohydrates, and drugs.
According to Bragg's law, when X-rays strike the sample positioned on a stage, the rays are  scattered by the electron clouds around the sample atoms. The  X-ray diffraction or scattering is caused by constructive interference of the X-ray waves that reflect off the internal...
3.9K
X-ray Imaging01:24

X-ray Imaging

7.7K
German physicist Wilhelm Röntgen (1845–1923) was experimenting with electrical current when he discovered that a mysterious and invisible "ray" would pass through his flesh but leave an outline of his bones on a screen coated with a metal compound. In 1895, Röntgen made the first durable record of the internal parts of a living human: an "X-ray" image (as it came to be called) of his wife’s hand. Scientists worldwide quickly began their own experiments with...
7.7K
Atomic Emission Spectroscopy: Overview01:20

Atomic Emission Spectroscopy: Overview

3.3K
Atomic emission spectroscopy (AES) is an analytical technique used to determine the elemental composition of a sample by analyzing the light emitted from excited atoms. In AES, atoms in a sample are excited to higher energy levels by thermal energy from high-temperature sources, such as plasma, arcs, or sparks. When these excited atoms return to lower energy states, they emit light at specific wavelengths characteristic of each element. The resulting atomic emission spectrum, which consists of...
3.3K
Atomic Emission Spectroscopy: Interference01:30

Atomic Emission Spectroscopy: Interference

793
In atomic emission spectroscopy (AES), high-temperature atomizers excite a broad range of elements and molecules that generate complex emissions from sources such as oxides, hydroxides, and flame combustion products in the flame or plasma. Several strategies can be employed to minimize spectral interferences caused by overlapping emission lines or bands. These include increasing instrument resolution, choosing alternative emission lines, optimally placing the detector in low-background regions,...
793

您也可能阅读

相关文章

通过共同作者、期刊和引用图与本文相关的文章。

排序
Same author

Observations of the missing baryons in the warm-hot intergalactic medium.

Nature·2018
Same author

Assessment of welfare of finishing beef cattle kept on different types of floor after short- or long-term housing.

Animal : an international journal of animal bioscience·2015
Same author

A test of the nature of cosmic acceleration using galaxy redshift distortions.

Nature·2008
Same author

A large population of galaxies 9 to 12 billion years back in the history of the Universe.

Nature·2005
Same author

Multiscaling properties of large-scale structure in the universe.

Science (New York, N.Y.)·1995
Same author

[Validity of cardioactive glycosides].

Minerva anestesiologica·1992

相关实验视频

Updated: May 6, 2026

Structure of HIV-1 Capsid Assemblies by Cryo-electron Microscopy and Iterative Helical Real-space Reconstruction
12:38

Structure of HIV-1 Capsid Assemblies by Cryo-electron Microscopy and Iterative Helical Real-space Reconstruction

Published on: August 9, 2011

19.1K

银河系的X射线星团作为宇宙结构的痕迹.

S Borgani1, L Guzzo

  • 1INFN, Sezione di Trieste, c/o Dipartimento di Astronomia dell'Università, Via Tiepolo 11, I-34131, Trieste, Italy. borgani@ts.astro.it

Nature
|May 9, 2001
PubMed
概括

星系团是宇宙物质的可见痕迹,它们发出X射线,揭示了它们的总质量. 这使得科学家能够研究宇宙.

科学领域:

  • 宇宙学的宇宙学是什么?
  • 天体物理学 天体物理学
  • X射线天文学X射线天文学

背景情况:

  • 星系团追踪宇宙的大规模结构,表明暗物质线程汇聚的高密度区域.
  • 来自星系团的X射线辐射源于被困在它们深深的引力潜力井中的热气体.
  • 射线辐射强度与星系团的总质量直接相关.

研究的目的:

  • 利用银河系团的X射线观测来研究宇宙中物质的分布.
  • 将观测数据与宇宙组成和演变的理论预测进行比较.

主要方法:

  • 在X射线波长中观测星系团.
  • 分析X射线辐射以确定集群质量.
  • 推导质量分布与宇宙学模型的比较.

主要成果:

  • X射线辐射提供了与星系团总质量的直接联系.
  • 研究表明,星系团中的质量分布与低密度宇宙一致.
  • 观测支持一个由冷暗物质主导的宇宙.

结论:

  • 星系团作为重要的宇宙灯塔,可以通过X射线辐射观察到.

更多相关视频

Applying X-ray Imaging Crystal Spectroscopy for Use as a High Temperature Plasma Diagnostic
06:46

Applying X-ray Imaging Crystal Spectroscopy for Use as a High Temperature Plasma Diagnostic

Published on: August 25, 2016

11.1K
Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface
06:14

Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface

Published on: July 30, 2020

5.7K

相关实验视频

Last Updated: May 6, 2026

Structure of HIV-1 Capsid Assemblies by Cryo-electron Microscopy and Iterative Helical Real-space Reconstruction
12:38

Structure of HIV-1 Capsid Assemblies by Cryo-electron Microscopy and Iterative Helical Real-space Reconstruction

Published on: August 9, 2011

19.1K
Applying X-ray Imaging Crystal Spectroscopy for Use as a High Temperature Plasma Diagnostic
06:46

Applying X-ray Imaging Crystal Spectroscopy for Use as a High Temperature Plasma Diagnostic

Published on: August 25, 2016

11.1K
Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface
06:14

Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface

Published on: July 30, 2020

5.7K
  • 观测到的星系团属性与标准宇宙学模型一致.
  • 目前的数据强化了冷暗物质主导的低密度宇宙的范式.