相关实验视频
Updated: Sep 11, 2025

06:14
Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface
Published on: July 30, 2020
5.0K
太阳极端紫外线辐射对近地空间中人造非常低频波的影响
K X Cheng1,2, L Y Li3,4, L Yang1,2
1School of Space and Earth Sciences, Beihang University, Beijing, China.
Scientific reports
|August 13, 2025
概括
增强的太阳极紫外线 (EUV) 辐射在全球范围内削弱了地球内部辐射带中的非常低频 (VLF) 发射波. 这种衰减,在较低度特别强,是由于电离层等离子体碰撞的增加.
科学领域:
- 空间物理 空间物理
- 大气科学 大气科学
- 等离子体物理学的物理学
背景情况:
- 基于地面的非常低频 (VLF) 发射波影响地球的辐射带.
- 太阳极紫外线 (EUV) 辐射对内部辐射带和槽区域的VLF波强度的影响仍然不清楚.
研究的目的:
- 为了研究太阳EUV辐射如何改变人造VLF波强度.
- 为了确定在不同的太阳EUV条件下VLF波减弱的度依赖.
主要方法:
- 对卫星观测的分析.
- 定量计算建模. 定量计算建模.
- 检查VLF波传播和电离层等离子体特性.
主要成果:
- 增强的太阳EUV辐射导致低度发射器 (L < 1.8 RE) 的VLF波的全球衰减.
- 从中度发射器 (L > 1.8 RE) 发出的VLF波在EUV高期中在中午左右略有减弱.
- 低度的电离层等离子体的碰撞阻尼增加解释了显著的VLF波衰减.
结论:
- 太阳能EUV辐射在调节内部辐射带的VLF波传播方面发挥着至关重要的作用.
- 离子层等离子体密度和碰撞频率是VLF波衰减的关键因素.
- 了解这些相互作用对于空间天气预测和辐射带动力学至关重要.
相关概念视频
The Electromagnetic Spectrum
29.8K
Electromagnetic waves are categorized according to their wavelengths and frequencies, giving the electromagnetic spectrum. These waves are classified as radio, infrared, ultraviolet, etc. Radio waves refer to electromagnetic radiation with wavelengths ranging from millimeters to kilometers. Radio waves are commonly used for audio communications (i.e., radios) and typically result from an alternating current in the wires of a broadcast antenna. They cover a broad wavelength range and are used...
29.8K
Mutations
40.1K
Mutations are changes in the sequence of DNA. These changes can occur spontaneously or they can be induced by exposure to environmental factors. Mutations can be characterized in a number of different ways: whether and how they alter the amino acid sequence of the protein, whether they occur over a small or large area of DNA, and whether they occur in somatic cells or germline cells.
Chromosomal Alterations Are Large-Scale Mutations
While point mutations are changes in a single nucleotide in...
Chromosomal Alterations Are Large-Scale Mutations
While point mutations are changes in a single nucleotide in...
40.1K
The Wave Nature of Light
51.4K
The nature of light has been a subject of inquiry since antiquity. In the seventeenth century, Isaac Newton performed experiments with lenses and prisms and was able to demonstrate that white light consists of the individual colors of the rainbow combined together. Newton explained his optics findings in terms of a "corpuscular" view of light, in which light was composed of streams of extremely tiny particles traveling at high speeds according to Newton's laws of motion.
51.4K
Intensity Of Electromagnetic Waves
4.8K
The energy transport per unit area per unit time, or the Poynting vector, gives the energy flux of an electromagnetic wave at any specific time. For a plane electromagnetic wave with E0 and B0 as the peak electric and magnetic fields and traveling along the x-axis, the time-varying energy flux can be given by the following equation:
4.8K
Electromagnetic Waves
9.3K
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...
9.3K
Ultraviolet and Visible (UV–Vis) Spectroscopy: Overview
3.1K
Ultraviolet–visible (UV–visible or UV–Vis) spectroscopy is an analytical technique that investigates the interaction between matter and UV–Vis light within the electromagnetic spectrum. This method is widely used for its versatility, simplicity, and relatively quick data acquisition, making it valuable for both qualitative and quantitative analysis. When UV–Vis radiation passes through a material, molecules absorb light depending on the energy required for...
3.1K

