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関連する概念動画

Electron Orbital Model01:18

Electron Orbital Model

Orbitals are the areas outside of the atomic nucleus where electrons are most likely to reside. They are characterized by different energy levels, shapes, and three-dimensional orientations. The location of electrons is described most generally by a shell or principal energy level, then by a subshell within each shell, and finally, by individual orbitals found within the subshells.The first shell is closest to the nucleus, and it has only one subshell with a single spherical orbital called the...
Subatomic Particles03:37

Subatomic Particles

Dalton was only partially correct about the particles that make up matter. All matter is composed of atoms, and atoms are composed of three smaller subatomic particles: protons, neutrons, and electrons. These three particles account for the mass and the charge of an atom.
Kinetic Theory of an Ideal Gas01:12

Kinetic Theory of an Ideal Gas

A mole is defined as the amount of any substance that contains as many molecules as there are atoms in exactly 12 grams of carbon-12. An Italian scientist Amedeo Avogadro (1776–1856) formed the  hypothesis that equal volumes of gas at equal pressure and temperature contain equal numbers of molecules, independent of the type of gas. Later, the hypothesis was developed to form the SI unit for measuring the amount of any substance.
The number of molecules in one mole is called Avogadro's number...
Faraday Disk Dynamo01:23

Faraday Disk Dynamo

A Faraday disk dynamo is a DC generator, producing an emf that is constant in time. It consists of a conducting disk that rotates with a constant angular velocity in the magnetic field, perpendicular to the disk's plane. The rotation of the disk causes a change in magnetic flux, which induces an emf, causing opposite charges to develop on the rim and in the center of the disk. The polarity of the induced emf can be determined by the direction of the magnetic field and the direction of the...
Thomson's e/m Experiment01:19

Thomson's e/m Experiment

In a beam of charged particles created by a heated cathode, the particles move at different speeds. However, many applications need a beam with uniform particle speeds. An arrangement known as a velocity selector uses electric and magnetic fields to pick particles with a particular speed from the beam.
A particle with charge q, speed v, and mass m enters an area from the top, where the magnetic and electric fields are perpendicular both to the particle's motion and to one another. The magnetic...
Vectors in Space: Problem Solving01:26

Vectors in Space: Problem Solving

A chandelier suspended by multiple cables can be analyzed using principles of three-dimensional static equilibrium. In this setup, a chandelier weighing 1000 N is positioned at the origin of a three-dimensional coordinate system, while three ceiling anchor points are fixed at known locations above it. Each cable connects the chandelier to one anchor point and transmits a tensile force along its length.To find out the forces in the cables, the spatial direction of each cable must first be...

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関連する実験動画

Updated: Jul 8, 2026

Gold Nanostar Synthesis with a Silver Seed Mediated Growth Method
12:39

Gold Nanostar Synthesis with a Silver Seed Mediated Growth Method

Published on: January 15, 2012

VEGAのヴェーナスの気球実験.

R Z Sagdeev, V M Linkin, J E Blamont

    Science (New York, N.Y.)
    |March 21, 1986
    PubMed
    まとめ

    2つの風船は1985年に金星の大気を調査し,重要な環境要因と風を測定しました. このVEGAミッションのデータは,金星の大気動力学と条件についての洞察を提供した.

    科学分野:

    • 惑星科学は惑星科学である.
    • 大気科学 大気科学
    • エアロノミーはエアロノミーです.

    背景:

    • 金星は,複雑なダイナミクスを持つ濃厚な大気を持っています.
    • 以前の金星の大気探査は,限られたデータに依存していた.
    • 金星の大気条件を理解することは,比較惑星学にとって極めて重要です.

    研究 の 目的:

    • 金星の大気圏に計測式気球を展開し,運用する.
    • 大気特性の in-situ 測定を収集する.
    • 先進的な追跡技術を使用して,金星の風のパターンを監視する.

    主な方法:

    • 1985年のVEGAミッション中に2つの計測気球を展開.
    • 圧力,気温,風速,雲の反射,光,雷のインサイトセンサー.
    • 世界的な無線アンテナネットワークを使用して,非常に長いベースライン干渉計 (VLBI) による気球の追跡.

    主要な成果:

    • バルーンは,金星の周りの約30%を成功裏に通過しました.
    • ~54kmの高度で大気変数に関する包括的なデータを収集しました.
    • VLBIは,風速測定のための正確な追跡を提供しました.

    さらに関連する動画

    Experimental Procedure for Warm Spinning of Cast Aluminum Components
    07:36

    Experimental Procedure for Warm Spinning of Cast Aluminum Components

    Published on: February 1, 2017

    Magnetically Induced Rotating Rayleigh-Taylor Instability
    06:42

    Magnetically Induced Rotating Rayleigh-Taylor Instability

    Published on: March 3, 2017

    関連する実験動画

    Last Updated: Jul 8, 2026

    Gold Nanostar Synthesis with a Silver Seed Mediated Growth Method
    12:39

    Gold Nanostar Synthesis with a Silver Seed Mediated Growth Method

    Published on: January 15, 2012

    Experimental Procedure for Warm Spinning of Cast Aluminum Components
    07:36

    Experimental Procedure for Warm Spinning of Cast Aluminum Components

    Published on: February 1, 2017

    Magnetically Induced Rotating Rayleigh-Taylor Instability
    06:42

    Magnetically Induced Rotating Rayleigh-Taylor Instability

    Published on: March 3, 2017

    結論:

    • VEGA風船実験は,金星の主要な大気のパラメータを成功裏に特徴付けました.
    • 収集されたデータは,金星の大気循環と構成に関する貴重な洞察を提供します.
    • この実験は,金星の長期間の大気モニタリングの実現可能性を実証した.