相关实验视频
Updated: Jul 12, 2026

06:14
Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface
Published on: July 30, 2020
太阳冠冕中的 Alfven 波
S Tomczyk1, S W McIntosh, S L Keil
1High Altitude Observatory (HAO), National Center for Atmospheric Research (NCAR), Post Office Box 3000, Boulder, CO 80307-3000, USA. tomczyk@ucar.edu
概括
在太阳的冠冕中检测到阿尔夫文波,但观察到的波似乎太弱,无法解释冠冕升温. 未解决的波可能仍然是了解太阳冠状热机制的关键.
科学领域:
- 太阳物理 太阳物理
- 等离子体天体物理学
- 太空物理学 太空物理学
背景情况:
- 太阳的日冕达到数百万度,这一现象目前的模型无法完全解释.
- 建议阿尔弗文波将能量从光球运送到冠状,可能驱动这种升温.
- 了解冠状热对于预测太空天气及其对地球的影响至关重要.
研究的目的:
- 为了检测和描述太阳冠冕中的阿尔夫文波.
- 评估观察到的阿尔夫文波对冠状热的能量传输能力.
- 为了研究阿尔夫文波在太阳大气能量平衡中的作用.
主要方法:
- 使用了国家太阳能天文台的冠状多通道极度计 (CoMP) 仪器.
- 分析了太阳冠冕的强度,视线速度和线性极化数据.
- 专注于FeXIII 1074.7纳米的冠状排放线.
主要成果:
- 在太阳冠冕中检测到无处不在的向上传播的阿尔弗温波.
- 测量波段速度在每秒1至4兆米之间.
- 推断波轨迹与磁场方向相一致,来自极化测量.
结论:
- 检测到的空间分辨率高的阿尔弗文波带有不足的能量来加热太阳冠状.
- 仍然有可能未解决或较小规模的阿尔弗文波可以为冠状热提供必要的能量.
- 需要对未解决的波群进行进一步的研究,以充分理解冠状能量传输.
相关概念视频
Electromagnetic Waves
James Clerk Maxwell formulated a single theory combining all the electric and magnetic effects scientists knew during that time, calling the phenomena his theory predicted “Electromagnetic waves”. He brought together all the work that had been done by brilliant physicists such as Oersted, Coulomb, Gauss, and Faraday and added his own insights to develop the overarching theory of electromagnetism. Maxwell’s equations, combined with the Lorentz force law, encompass all the laws of electricity and...
Propagation of Waves
When a wave propagates from one medium to another, part of it may get reflected in the first medium, and part of it may get transmitted to the second medium. In such a case, the interface of the two mediums can be considered as a boundary that is neither fixed nor free.
Consider a scenario where a wave propagates from a string of low linear mass density to a string of high linear mass density. In such a case, the reflected wave is out of phase with respect to the incident wave, however the...
Consider a scenario where a wave propagates from a string of low linear mass density to a string of high linear mass density. In such a case, the reflected wave is out of phase with respect to the incident wave, however the...
Standing Waves
Sometimes waves do not seem to move; rather, they just vibrate in place. Unmoving waves can be seen on the surface of a glass of milk kept in a refrigerator, which is one example of standing waves. Vibrations from the refrigerator motor create waves on the milk that oscillate up and down but do not seem to move across the surface. These waves are formed or created by the superposition of two or more identical moving waves in opposite directions. The waves move through each other, with their...
Electromagnetic Wave Equation
Maxwell's equations for electromagnetic fields are related to source charges, either static or moving. These fields act on a test charge, whose trajectory can thus be determined using suitable boundary conditions. The objective of electromagnetism is thus theoretically complete.
However, although electric and magnetic fields were first introduced as mathematical constructs to simplify the description of mutual forces between charges, a natural question emerges from Maxwell's equations: What...
However, although electric and magnetic fields were first introduced as mathematical constructs to simplify the description of mutual forces between charges, a natural question emerges from Maxwell's equations: What...
Equations of Wave Motion
Mathematically, the motion of a wave can be studied using a wavefunction. Consider a string oscillating up and down in simple harmonic motion, having a period T. The wave on the string is sinusoidal and is translated in the positive x-direction as time progresses. Sine is a function of the angle θ, oscillating between +A and −A and repeating every 2π radians. To construct a wave model, the ratio of the angle θ and the position x is considered.
Standing Waves in a Cavity
A household microwave and lasers are examples of standing electromagnetic waves in a cavity. When two conducting metal plates are placed parallel at the nodal planes, it creates a cavity where standing waves are formed. The cavity between the two planes is analogous to a stretched string held at the points x = 0 and x = L. Here, the distance 'L' between the two planes must be an integer multiple of half of the wavelength. The wavelengths that satisfy this condition are given by:

