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相关概念视频

Hess's Law03:40

Hess's Law

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.
IR Spectrum Peak Splitting: Symmetric vs Asymmetric Vibrations01:08

IR Spectrum Peak Splitting: Symmetric vs Asymmetric Vibrations

Identical bonds within a polyatomic group can stretch symmetrically (in-phase) or asymmetrically (out-of-phase). Similar to hydrogen bonding, these vibrations also influence the shape of the IR peak. Generally, asymmetric stretching frequencies are higher than symmetric stretching frequencies. For example, primary amines exhibit two distinct IR peaks between 3300–3500 cm−1 corresponding to the symmetric and asymmetric N-H stretching, while secondary amines exhibit a single stretching vibration...
Kepler's Second Law of Planetary Motion01:29

Kepler's Second Law of Planetary Motion

In the early 17th century, German astronomer and mathematician Johannes Kepler postulated three laws for the motion of planets in the solar system. His first law states that all planets orbit the Sun in an elliptical orbit, with the Sun at one of the ellipse's foci. Therefore, the distance of a planet from the Sun varies throughout its revolution around the Sun.
While in an elliptical orbit, the total energy of the planet is conserved. Therefore, the planet slows down when it is at apogee and...
IR Spectroscopy: Molecular Vibration Overview01:24

IR Spectroscopy: Molecular Vibration Overview

When Infrared (IR) radiation passes through a covalently bonded molecule, the bonds transition from lower to higher vibrational levels. The fundamental vibrational motions that result in infrared absorption can be classified as stretching or bending vibrations.
Stretching vibrations are vibrational motions that occur along the bond line, changing the bond length or distance between two bonded atoms. They are further distinguished as symmetric or asymmetric. In symmetric stretching, the...
The Principle of Superposition and the Gravitational Field01:17

The Principle of Superposition and the Gravitational Field

The principle of superposition applies to gravitational forces of objects that are sufficiently far apart. It states that the net gravitational force on a point object is the vector sum of the gravitational forces on it due to various objects. The principle helps calculate the force by listing the individual forces and then vectorially summing them up. However, it should be noted that the principle of superposition is not always apparent. In the presence of a second force, the first force could...
Atomic Emission Spectroscopy: Overview01:20

Atomic Emission Spectroscopy: Overview

Atomic emission spectroscopy (AES) is an analytical technique used to determine the elemental composition of a sample by analyzing the light emitted from excited atoms. In AES, atoms in a sample are excited to higher energy levels by thermal energy from high-temperature sources, such as plasma, arcs, or sparks. When these excited atoms return to lower energy states, they emit light at specific wavelengths characteristic of each element. The resulting atomic emission spectrum, which consists of...

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相关实验视频

Updated: Jul 26, 2026

Hemi-laryngeal Setup for Studying Vocal Fold Vibration in Three Dimensions
10:13

Hemi-laryngeal Setup for Studying Vocal Fold Vibration in Three Dimensions

Published on: November 25, 2017

在地震学的观点.

Gough1, Leibacher, Scherrer

  • 1D. O. Gough is with the Institute of Astronomy, University of Cambridge, Cambridge, CB3 OHA UK. J. W. Leibacher is with the National Solar Observatory, Tucson, AZ, USA. P. H. Scherrer is with the Department of Physics, Stanford University, Stanford, CA, USA. J. Toomre is with JILA, University of Colorado, Boulder, CO, USA.

Science (New York, N.Y.)
|May 31, 1996
PubMed
概括

太阳地震学使用太阳振荡频率来研究太阳的内部. 来自全球振荡网络集团 (GONG) 和太阳和日球天文台 (SoHO) 的新数据推动了我们对恒星物理学的理解.

科学领域:

  • 太阳物理 太阳物理
  • 恒星天体物理学 恒星天体物理学
  • 太阳地震学 (Helioseismology) 是一个关于太阳的学科.

背景情况:

  • 天文地震学提供了一个独特的实验室,用于研究极端条件下的物理过程.
  • 了解太阳的内部对于理解恒星运行至关重要.

研究的目的:

  • 以高精度探测太阳的内部结构和动态.
  • 用太阳振荡频率进行详细分析.

主要方法:

  • 在太阳大气层中观察了近1000万个共振振荡模式.
  • 利用来自全球振荡网络集团 (GONG) 和太阳和日球天文台 (SoHO) 的连续,高频率成像数据.

主要成果:

  • 太阳振荡的高精度频率测量对于室内建模至关重要.
  • 刚刚的早期结果正在解决现有问题,并提出新的理论问题.

结论:

  • GONG和SoHO数据的结合标志着日系地震学的新时代.
  • 需要进一步的理论研究来解释这些发现并了解太阳能运行.

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Hemi-laryngeal Setup for Studying Vocal Fold Vibration in Three Dimensions
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Hemi-laryngeal Setup for Studying Vocal Fold Vibration in Three Dimensions

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Scattering And Absorption of Light in Planetary Regoliths
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Scattering And Absorption of Light in Planetary Regoliths

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