相关实验视频
Updated: Nov 19, 2025

11:34
Scattering And Absorption of Light in Planetary Regoliths
Published on: July 1, 2019
10.6K
选择性吸收过程是来自太阳令人费解的光谱线偏振的起源
J Trujillo Bueno1, E Landi Degl'Innocenti, M Collados
1Instituto de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain. jtb@ll.iac.es
Nature
|January 25, 2002
概括
研究人员在太阳冠状丝中观察到奇特的极化光. 这一发现揭示了几高斯的磁场倾向于太阳半径向量,挑战了以前关于磁场诊断的假设.
科学领域:
- 天体物理学 天体物理学
- 太阳物理 太阳物理
- 原子物理 原子物理
背景情况:
- 磁场在天体物理系统中至关重要,影响从太阳活动到活跃的银河系核的现象.
- 极化光谱线提供了一种方法,通过观察磁场对原子能水平的影响来研究磁场.
- 不同类型的辐射送过程可以在原子水平上产生人口不平衡,然后由磁场调节.
研究的目的:
- 为了研究在太阳冠状丝中的He I 10,830-A多重体中观察到的奇特的极化光.
- 确定这种偏光对理解太阳磁场的影响.
- 挑战现有的关于人口不平衡在倾斜磁场中的意义的信念.
主要方法:
- 在太阳冠状丝中观察He I 10,830-A多重体.
- 对极化光信号的分析,以推断原子水平人口不平衡.
- 模拟异型辐射与弱,倾斜的磁场的相互作用.
主要成果:
- 在He I 10,830-A多重体中检测到特殊的极化光.
- 极化光源于三重系统内的选择性吸收.
- 这些观测暗示存在几个高斯的磁场,高度倾向于太阳半径向量.
结论:
- 这项研究驳斥了这样一种观点,即在存在几高斯倾斜的磁场的情况下,人口失衡是微不足道的.
- 这一发现为研究太阳磁场开辟了一条新的诊断途径.
- 这些发现有助于更深入地了解太阳等离子体中的磁场行为.
更多相关视频
相关概念视频
Light as Energy
86.3K
The energy required to carry out photosynthesis is light— typically electromagnetic radiation from the sun. The range of all possible wavelengths is known as the electromagnetic spectrum.
Photons
A photon is a discrete electromagnetic particle or bundle of energy. Photons are characterized by their frequency, wavelength, and amplitude, similar to the properties of a wave. Waves with higher frequencies transmit more energy and have shorter wavelengths than longer wavelengths that transmit...
Photons
A photon is a discrete electromagnetic particle or bundle of energy. Photons are characterized by their frequency, wavelength, and amplitude, similar to the properties of a wave. Waves with higher frequencies transmit more energy and have shorter wavelengths than longer wavelengths that transmit...
86.3K
Emission Spectra
73.7K
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.
73.7K
UV–Vis Spectroscopy: Molecular Electronic Transitions
2.3K
In Ultraviolet–Visible (UV–Vis) spectroscopy, the absorption of electromagnetic radiation is used to probe the electronic structure of molecules. This technique provides insights into molecular electronic transitions, particularly the movement of electrons between different molecular orbitals. Radiation is absorbed if the energy of the electromagnetic radiation passing through the molecule is precisely equal to the energy difference between the excited and ground states. During this...
2.3K
UV–Vis Spectroscopy of Conjugated Systems
7.8K
Organic compounds with conjugated double bonds show strong absorption features in the UV–visible region of the electromagnetic spectrum attributed to π → π* electronic excitations. Generally, a UV–vis absorption spectrum is recorded as a plot of absorbance vs wavelength. The wavelength of maximum absorbance, which manifests as a peak in the absorption spectrum, is denoted as λmax.
One of the factors influencing λmax is the extent of conjugation in...
One of the factors influencing λmax is the extent of conjugation in...
7.8K
Energy Transfer in Chemical Reactions
10.2K
Chemical reactions require sufficient energy to cause the matter to collide with enough precision and force that old chemical bonds can be broken and new ones formed. In general, kinetic energy is the form of energy powering any type of matter in motion. Imagine a person building a brick wall. The energy it takes to lift and place one brick on top of another is the kinetic energy—the energy matter possesses because of its motion. Once the wall is in place, it stores potential energy.
10.2K
Ultraviolet and Visible (UV–Vis) Spectroscopy: Overview
3.9K
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...
3.9K

