相关实验视频
Updated: Jul 7, 2026

10:35
Bringing the Visible Universe into Focus with Robo-AO
Published on: February 12, 2013
在木星的极光耀斑.
J H Waite1, G R Gladstone, W S Lewis
1Department of Atmospheric, Oceanic, and Space Sciences, University of Michigan, Ann Arbor, Michigan 48109, USA. hunterw@umich.edu
Nature
|April 12, 2001
概括
科学家们在木星附近发现了一种新的,快速变亮的极光辐射.
科学领域:
- 行星科学 行星科学
- 空间物理 空间物理
- 天体物理学 天体物理学
背景情况:
- 木星的极光是太阳系中最强大的极光,主要是由行星的旋转驱动的,次要的是太阳风.
- 与由太阳风驱动的地球极光不同,木星的极光辐射呈现出不同的特征,如主要圆和扩散区域.
研究的目的:
- 报道发现了一种新型,快速演变的极光发射极向木星北方主圆形的发现.
- 描述这种新观察到的木星极光现象的强度,时间尺度和潜在驱动因素.
主要方法:
- 使用远紫外线,近红外线和可见波长仪器观测木星的极光.
- 对特定的四分钟曝光的分析,捕捉了短暂的极光事件.
主要成果:
- 发现一个局部的,明亮的极光发射北方主要圆的极向.
- 观察到强度快速增加 (在70秒内增加30倍),随后出现类似的下降.
- 这种耀斑的辐射与木星的外磁层有关,并且可能受到太阳风变化的影响.
结论:
- 这种短暂的极光耀斑事件是木星以前未报告的现象.
- 这一发现表明,太阳风动力学与木星的强烈,局部的极光辐射之间存在潜在的直接联系.
- 需要进一步的研究才能充分了解驱动这些快速极光事件的机制.
相关概念视频
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.
Electric Flux
The concept of flux describes how much of something goes through a given area. More formally, it is the dot product of a vector field within an area. For a better understanding, consider an open rectangular surface with a small area that is placed in a uniform electric field. The larger the area, the more field lines go through it and, hence, the greater the flux; similarly, the stronger the electric field (represented by a greater density of lines), the greater the flux. On the other hand, if...
Magnetic Field Lines
The representation of magnetic fields by magnetic field lines is very useful in visualizing the strength and direction of the magnetic field. Each of the magnetic field lines forms a closed loop. The field lines emerge from the north pole (N), loop around to the south pole (S), and continue through the bar magnet back to the north pole.
Magnetic field lines follow several hard-and-fast rules:
Magnetic field lines follow several hard-and-fast rules:
Magnetic Flux
The magnetic flux measures the number of magnetic field lines passing through a given surface area. The SI unit for magnetic flux is the weber (Wb). Magnetic flux is a scalar quantity. It depends on three factors: the strength of the magnetic field B, the area through which the field lines pass, and the relative orientation of the field with the surface area.
Suppose a surface is divided into elements of area dA. For each element, the component of the magnetic field that is normal to the...
Suppose a surface is divided into elements of area dA. For each element, the component of the magnetic field that is normal to the...
Flame Photometry: Overview
Flame photometry, also known as flame emission spectrometry, is a technique used for the qualitative and quantitative analysis of elements present in a sample using a flame as the source of excitation energy. The concept of flame photometry was realized in the early 1860s by Kirchhoff and Bunsen, who discovered that specific elements emit characteristic radiation when excited in flames. The first instrument developed for this purpose was used to measure sodium (Na) in plant ash using a Bunsen...
Flame Photometry: Lab
In a flame photometer, when a solution like potassium chloride is aspirated into the flame, the solvent evaporates, leaving behind dehydrated salt. This salt dissociates into free gaseous atoms in their ground state. Some of these atoms absorb energy from the flame, leading to their excitation. The excited atoms return to the ground state, emitting photons at characteristic wavelengths. Because only electronic transitions are involved, the resulting emission lines are very narrow. The intensity...

