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相关概念视频

Nuclear Fusion02:45

Nuclear Fusion

The process of converting very light nuclei into heavier nuclei is also accompanied by the conversion of mass into large amounts of energy, a process called fusion. The principal source of energy in the sun is a net fusion reaction in which four hydrogen nuclei fuse and ultimately produce one helium nucleus and two positrons.
A helium nucleus has a mass that is 0.7% less than that of four hydrogen nuclei; this lost mass is converted into energy during the fusion. This reaction produces about...
Inductively Coupled Plasma Atomic Emission Spectroscopy: Principle01:19

Inductively Coupled Plasma Atomic Emission Spectroscopy: Principle

Inductively coupled plasma (ICP) is the most widely used plasma source in atomic emission spectroscopy (AES), also known as Inductively Coupled Plasma Optical Emission Spectroscopy (ICP-OES). The ICP source, or torch, consists of three concentric quartz tubes with argon gas flowing through them. A spark from a Tesla coil initiates the ionization of argon, generating a high-temperature plasma.
The ions and electrons produced interact with the fluctuating magnetic field created by a water-cooled...
Inductively Coupled Plasma–Mass Spectrometry (ICP–MS): Overview01:19

Inductively Coupled Plasma–Mass Spectrometry (ICP–MS): Overview

In inductively coupled plasma–mass spectrometry (ICP–MS), an inductively coupled plasma (ICP) torch is used as an atomizer and ionizer. Solid samples are dissolved and volatilized before being introduced into the high-temperature argon plasma, while solution samples are nebulized and passed through the high-temperature argon plasma. Plasma dissociates the analytes and ionizes their component atoms to form a mixture of positive ions and molecular species. The positive ions are then passed on to...
Continuous Charge Distributions01:17

Continuous Charge Distributions

Imagine a bucket of water. It contains many molecules, of the order of 1026 molecules. Thus, although it contains discrete elements (molecules) at the microscopic level, macroscopically, it can be considered continuous. Small volume elements of water, infinitesimal compared to the bulk of the bucket's volume, still contain many molecules. Under this framework, quantized matter is approximated as continuous for practical purposes.
The electric charge can also be subjected to an analogical...
Atomic Nuclei: Nuclear Spin State Population Distribution01:14

Atomic Nuclei: Nuclear Spin State Population Distribution

Near absolute zero temperatures, in the presence of a magnetic field, the majority of nuclei prefer the lower energy spin-up state to the higher energy spin-down state. As temperatures increase, the energy from thermal collisions distributes the spins more equally between the two states. The Boltzmann distribution equation gives the ratio of the number of spins predicted in the spin −½ (N−) and spin +½ (N+) states.
Energy Associated With a Charge Distribution01:21

Energy Associated With a Charge Distribution

The work done to bring a charge through a distance r is given by the potential difference between the initial and the final position. To assemble a collection of point charges, the total work done can be expressed in terms of the product of each pair of charges divided by their separation distance, defined with respect to a suitable origin. Solving this expression gives the energy stored in a point charge distribution.

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相关实验视频

Updated: Jul 12, 2026

An Atmospheric Pressure Plasma Setup to Investigate the Reactive Species Formation
08:36

An Atmospheric Pressure Plasma Setup to Investigate the Reactive Species Formation

Published on: November 3, 2016

原子云作为IO等离子体的分布式源.

R A Brown, W H Ip

    Science (New York, N.Y.)
    |September 25, 1981
    PubMed
    概括

    最近的发现揭示了木星 Io torus 中的热硫离子,这表明中性硫云是关键来源. 这些含氧和硫的中性云对木星的磁层和岩石圈环境至关重要.

    科学领域:

    • 行星科学 行星科学
    • 空间物理 空间物理
    • 等离子体物理学的物理.

    背景情况:

    • 木星的磁层是一个复杂的系统,受到内部和外部等离子体来源的影响.
    • 体是围绕木星的等离子体体,主要由来自木星的卫星Io的离子组成.
    • 了解中性粒子环境对于解释磁层动态至关重要.

    研究的目的:

    • 调查最近的发展对木星中性粒子环境的影响.
    • 为了探索在体中检测到的非常热的硫离子的起源.
    • 评估中性氧和硫云在木星磁层中的作用.

    主要方法:

    • 分析了对电流中的离子旋转速度的观测数据.
    • 关于中性云的存在和属性的假设测试.
    • 模拟中性云对离子和能源的贡献.

    主要成果:

    • 在Io torus中检测到非常热的硫离子,其旋转速度接近旋转速度.
    • 证据支持木星磁层中存在广泛的中性氧和硫云的存在.
    • 这些云被认定为 Io torus 重要的离子和能量来源.

    结论:

    更多相关视频

    How to Ignite an Atmospheric Pressure Microwave Plasma Torch without Any Additional Igniters
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    How to Ignite an Atmospheric Pressure Microwave Plasma Torch without Any Additional Igniters

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    Non-equilibrium Microwave Plasma for Efficient High Temperature Chemistry
    07:17

    Non-equilibrium Microwave Plasma for Efficient High Temperature Chemistry

    Published on: August 1, 2017

    相关实验视频

    Last Updated: Jul 12, 2026

    An Atmospheric Pressure Plasma Setup to Investigate the Reactive Species Formation
    08:36

    An Atmospheric Pressure Plasma Setup to Investigate the Reactive Species Formation

    Published on: November 3, 2016

    How to Ignite an Atmospheric Pressure Microwave Plasma Torch without Any Additional Igniters
    08:42

    How to Ignite an Atmospheric Pressure Microwave Plasma Torch without Any Additional Igniters

    Published on: April 16, 2015

    Non-equilibrium Microwave Plasma for Efficient High Temperature Chemistry
    07:17

    Non-equilibrium Microwave Plasma for Efficient High Temperature Chemistry

    Published on: August 1, 2017

    • 在木星的磁层中可能存在氧和硫的中性云.
    • 这些中性云在向电流提供离子和能量方面发挥着至关重要的作用.
    • 对中性粒子环境的进一步研究对于全面了解木星磁层过程至关重要.