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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.
π Electron Effects on Chemical Shift: Overview01:27

π Electron Effects on Chemical Shift: Overview

An applied magnetic field causes loosely bound π-electrons in organic molecules to circulate, producing a local or induced diamagnetic field over a large spatial volume. As the molecules tumble in solution, the field generated by π-electrons in spherical substituents results in a zero net field. However, the net field generated by π-electrons in non-spherical substituents is not zero. The effect of this induced field depends on the orientation of the molecule with respect to B0, resulting in...
¹³C NMR: ¹H–¹³C Decoupling01:04

¹³C NMR: ¹H–¹³C Decoupling

The probability of having two carbon-13 atoms next to each other is negligible because of the low natural abundance of carbon-13. Consequently, peak splitting due to carbon-carbon spin-spin coupling is not observed in spectra. However, protons up to three sigma bonds away split the carbon signal according to the n+1 rule, resulting in complicated spectra.
A broadband decoupling technique is used to simplify these complex, sometimes overlapping, signals. Broadband decoupling relies on a...
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...
Variables Affecting Phosphorescence and Fluorescence01:26

Variables Affecting Phosphorescence and Fluorescence

Fluorescence and phosphorescence are essential phenomena in fields like analytical chemistry, biological imaging, and materials science, where they detect molecular properties and visualize cellular structures. Understanding the variables that influence these luminescent behaviors is crucial for maximizing accuracy and efficiency in their applications. These variables can broadly be grouped into chemical structure, solvent properties, and external conditions, each playing a distinct role in...
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 15, 2026

Investigation of Early Plasma Evolution Induced by Ultrashort Laser Pulses
11:20

Investigation of Early Plasma Evolution Induced by Ultrashort Laser Pulses

Published on: July 2, 2012

脉冲星辐射的星际散射及其对NP0532的光谱的影响.

W M Cronyn

    Science (New York, N.Y.)
    |June 19, 1970
    PubMed
    概括

    星际介质的散射导致分散,影响脉冲星信号. 脉冲星NP053232 是一个脉冲星.

    科学领域:

    • 天文学和天体物理学
    • 脉冲星物理学的物理学
    • 星际媒介研究 星际媒介研究

    背景情况:

    • 星际介质中的角散射导致多路径散射.
    • 这种分散可以超过一个脉冲周期,用于短期,高分散度脉冲星.
    • 散射对脉冲流量施加了切断,与观察波长的第四次数成反比例.

    研究的目的:

    • 为了研究脉冲星NP0532.2的低频脉冲形状.
    • 为了确定观察到的低频谱切断是否是脉冲星的内在性质,还是由于散射.
    • 探索NP0532与星云的紧,低频源的潜在识别.

    主要方法:

    • 对脉冲星NP0532的低频脉冲形状的分析.
    • 观察到的光谱特性与星际散射的理论预测进行比较.
    • 检查证据,将NP0532与星云的紧低频源联系起来.

    主要成果:

    • NP0532的低频脉冲形状表明它受到星际散射的影响.
    • 观察到的低频谱切线可能不是NP0532.3的内在特征.
    • 证据支持NP0532的识别为星云的紧,低频源.
    • NP0532可能会像它的高频频谱一样辐射到10兆赫.

    更多相关视频

    Scattering And Absorption of Light in Planetary Regoliths
    11:34

    Scattering And Absorption of Light in Planetary Regoliths

    Published on: July 1, 2019

    Measuring the Behavioral Effects of Intraocular Scatter
    05:10

    Measuring the Behavioral Effects of Intraocular Scatter

    Published on: February 18, 2021

    相关实验视频

    Last Updated: Jun 15, 2026

    Investigation of Early Plasma Evolution Induced by Ultrashort Laser Pulses
    11:20

    Investigation of Early Plasma Evolution Induced by Ultrashort Laser Pulses

    Published on: July 2, 2012

    Scattering And Absorption of Light in Planetary Regoliths
    11:34

    Scattering And Absorption of Light in Planetary Regoliths

    Published on: July 1, 2019

    Measuring the Behavioral Effects of Intraocular Scatter
    05:10

    Measuring the Behavioral Effects of Intraocular Scatter

    Published on: February 18, 2021

    结论:

    • 星际散射显著影响低频脉冲星的观测.
    • 在NP0532中低频谱切断是由于散射而不是内在特性.
    • 由于散射,脉冲星NP0532的周期变化被抑制在100兆赫以下.