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相关概念视频

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.
IR Spectrum Peak Broadening: Hydrogen Bonding01:23

IR Spectrum Peak Broadening: Hydrogen Bonding

The vibrational frequency of a bond is directly proportional to its bond strength. As a result, stronger bonds vibrate at higher frequencies, while weaker bonds vibrate at lower frequencies. The stretching vibration of the strong O–H bond in alcohols and phenols (very dilute solution or gas phase) appears as a sharp peak at 3600–3650 cm−1.
However, the extent of hydrogen bonding influences the observed stretching frequency and band broadening. Intermolecular or intramolecular hydrogen bonding...
Shock Waves01:16

Shock Waves

While deriving the Doppler formula for the observed frequency of a sound wave, it is assumed that the speed of sound in the medium is greater than the source's speed through it. When this condition is breached, a shock wave occurs.
When the source's speed approaches the speed of sound, constructive interference between successive wavefronts emitted by the source occurs immediately behind it. Initially, scientists believed that this constructive interference would result in such high pressures...
Interaction of EM Radiation with Matter: Spectroscopy01:12

Interaction of EM Radiation with Matter: Spectroscopy

Electromagnetic (EM) radiation can be considered an oscillating electric and magnetic field propagating through a medium that can interact with matter in its path. The electric field in the radiation can interact with electrical charges in the atoms or molecules in the matter. On the other hand, the magnetic field can interact with the magnetic field in the atomic nucleus. The study of the interaction between electromagnetic radiation and matter is termed spectroscopy. Spectroscopy is the study...
Atomic Emission Spectroscopy: Overview01:20

Atomic Emission Spectroscopy: Overview

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...
Atomic Emission Spectroscopy: Interference01:30

Atomic Emission Spectroscopy: Interference

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,...

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相关实验视频

Updated: Jun 1, 2026

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

一个具有高能光谱成分的马射线爆发与同步子冲击模型不一致.

M M González1, B L Dingus, Y Kaneko

  • 1Physics Department, University of Wisconsin, Madison, Wisconsin 53706, USA. magda@whopper.lanl.gov

Nature
|August 15, 2003
PubMed
概括

在1994年的马射线爆发 (GRB) 中观察到一种新的高能马射线成分. 这一发现挑战了标准模型,表明GRB中的新型粒子加速或质子-光子相互作用.

科学领域:

  • 天体物理学 天体物理学
  • 高能天体物理学 高能天体物理学
  • 宇宙射线物理学 宇宙射线物理学

背景情况:

  • 马射线爆发 (GRBs) 是宇宙中最有能量的现象.
  • GRBs以光子 (30 keV MeV) 的形式发射了大部分能量,具有较低能量的后照.
  • 标准模型将GRB辐射归因于冲击加速电子的同步子辐射.

研究的目的:

  • 报告GRB中一个独特的高能光谱元件的观测.
  • 为了调查GRBs标准同步子冲击模型的偏差.

主要方法:

  • 1994年10月17日发生的马射线爆发的观测.
  • 高能 (多MeV) 光子的光谱分析.
  • 观察数据与标准相对论冲击模型的比较.

主要成果:

  • 观察到一种独特的高能 (多MeV) 光谱成分,与低能马射线不同.
  • 高能组件表现出较慢的流量衰变和更大的流动性.
  • 这个组件遵循功率规律,达到~200 MeV (光子指数~-1).

结论:

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Method for Recording Broadband High Resolution Emission Spectra of Laboratory Lightning Arcs
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Method for Recording Broadband High Resolution Emission Spectra of Laboratory Lightning Arcs

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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

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Last Updated: Jun 1, 2026

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

Method for Recording Broadband High Resolution Emission Spectra of Laboratory Lightning Arcs
07:51

Method for Recording Broadband High Resolution Emission Spectra of Laboratory Lightning Arcs

Published on: August 27, 2019

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

  • 观察到的高能元件挑战了GRBs的标准同步子冲击模型.
  • 可能涉及到新的现象,例如替代的非热电子过程.
  • 源头上的质子-光子相互作用是观察到的高能发射的潜在解释.