相关实验视频
Updated: May 30, 2025

11:34
Scattering And Absorption of Light in Planetary Regoliths
Published on: July 1, 2019
10.2K
太阳辐射不透明性的太阳地震推断
Gaël Buldgen1,2, Jean-Christophe Pain3,4, Philippe Cossé3,4
1STAR Institute, Université de Liège, Allée du 6 août, 19C, 4000, Liège, Belgium. gbuldgen@uliege.be.
Nature communications
|January 27, 2025
概括
太阳地震推断显示,太阳的不透明度比目前的模型高出10%,约200万度. 量化比较对于解决太阳物理数据中的差异至关重要.
科学领域:
- 恒星天体物理学 恒星天体物理学
- 太阳物理 太阳物理
背景情况:
- 太阳作为恒星模型的基准,但它的内部物理,特别是辐射不透明,仍然存在争议.
- 在实验测量和太阳不透明度的理论计算之间存在差异.
研究的目的:
- 以理论计算来比较从日地震推断中得出的不透明度概况.
- 调查太阳不透明度值的差异及其对太阳模型的影响.
主要方法:
- 地震数据被用来推断太阳不透明度的概况.
- 理论上的不透明度计算是使用三个不同的计算代码进行的.
- 地震不透明度与理论和实验值进行了比较.
主要成果:
- 地震不透明度大约比当前太阳能模型中使用的价值高出10%,接近200万凯尔文.
- 地震不透明度比最近一些理论不透明度值低35%.
- 在日流地震,理论和实验不透明度数据之间仍然存在显著的差异.
结论:
- 太阳作为基本物理学的重要实验室,突出了准确的不透明度计算的需要.
- 不同的不透明度表的定量比较对于解决当前不一致性至关重要.
- 需要进一步的研究来协调日地震,理论和实验性不透明度测量,以改进太阳能模型.
相关概念视频
Emission Spectra
50.3K
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.
50.3K
Hess's Law
44.4K
There are two ways to determine the amount of heat involved in a chemical change: measure it experimentally, or calculate it from other experimentally determined enthalpy changes. Some reactions are difficult, if not impossible, to investigate and make accurate measurements for experimentally. And even when a reaction is not hard to perform or measure, it is convenient to be able to determine the heat involved in a reaction without having to perform an experiment.
44.4K
Maxwell-Boltzmann Distribution: Problem Solving
1.4K
Individual molecules in a gas move in random directions, but a gas containing numerous molecules has a predictable distribution of molecular speeds, which is known as the Maxwell-Boltzmann distribution, f(v).
This distribution function f(v) is defined by saying that the expected number N (v1,v2) of particles with speeds between v1 and v2 is given by
This distribution function f(v) is defined by saying that the expected number N (v1,v2) of particles with speeds between v1 and v2 is given by
1.4K
IR Spectroscopy: Hooke's Law Approximation of Molecular Vibration
1.2K
A covalently bonded heteronuclear diatomic molecule can be modeled as two vibrating masses connected by a spring. The vibrational frequency of the bond can be expressed using an equation derived from Hooke's law, which describes how the force applied to stretch or compress a spring is proportional to the displacement of the spring. In this case, the atoms behave like masses, and the bond acts like a spring.
According to Hooke's law, the vibrational frequency is directly proportional to...
According to Hooke's law, the vibrational frequency is directly proportional to...
1.2K
Atomic Emission Spectroscopy: Interference
163
In atomic emission spectroscopy (AES), high-temperature atomizers excite a broad range of elements and molecules that generate complex emissions from sources such as oxides, hydroxides, and flame combustion products in the flame or plasma. Several strategies can be employed to minimize spectral interferences caused by overlapping emission lines or bands. These include increasing instrument resolution, choosing alternative emission lines, optimally placing the detector in low-background regions,...
163
Radiation Pressure: Problem Solving
308
The radiation pressure applied by an electromagnetic wave on a perfectly absorbing surface equals the energy density of the wave. The wave's momentum also gets transferred to the surface when an electromagnetic wave is entirely absorbed by it. The rate at which momentum is transmitted to an absorbing surface perpendicular to the propagation direction equals the force on the surface.
The average value of the rate of momentum transfer divided by the absorbing area represents the average force...
The average value of the rate of momentum transfer divided by the absorbing area represents the average force...
308

